SpaceSolarSystem

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License = https://en.wikipedia.org/wiki/File:Planets2013.svg
Title = The solar system from inner to outer. Title picture: The Sun and planets (distances not to scale)
URL = https://upload.wikimedia.org/wikipedia/commons/thumb/c/cb/Planets2013.svg/1280px-Planets2013.svg.png
010_Sun/License = https://en.wikipedia.org/wiki/File:The_Sun_by_the_Atmospheric_Imaging_Assembly_of_NASA's_Solar_Dynamics_Observatory_-_20100819.jpg
010_Sun/Title = The Sun photographed at 304 angstroms by the Atmospheric Imaging Assembly (AIA 304) of NASA's Solar Dynamics Observatory (SDO). This is a false-color image of the Sun observed in the extreme ultraviolet region of the spectrum.
010_Sun/URL = https://upload.wikimedia.org/wikipedia/commons/b/b4/The_Sun_by_the_Atmospheric_Imaging_Assembly_of_NASA's_Solar_Dynamics_Observatory_-_20100819.jpg
010_Sun/02_Compare/License = https://en.wikipedia.org/wiki/File:Planets_and_sun_size_comparison.jpg
010_Sun/02_Compare/Title = Size comparison of the Sun and the planets (clickable).
010_Sun/02_Compare/URL = https://upload.wikimedia.org/wikipedia/commons/d/d7/Planets_and_sun_size_comparison.jpg
010_Sun/03_Flare/License = https://en.wikipedia.org/wiki/File:Skylab_Solar_flare.jpg
010_Sun/03_Flare/Title =  This photograph of the Sun, taken on December 19, 1973, during the third and final manned Skylab mission, shows one of the most spectacular solar prominences ever recorded, spanning more than 588,000 kilometers (365,000 miles) across the solar surface. The loop prominence gives the distinct impression of a twisted sheet of gas in the process of unwinding itself.
010_Sun/03_Flare/URL = https://upload.wikimedia.org/wikipedia/commons/3/37/Skylab_Solar_flare.jpg
010_Sun/04_Chromosphere/License = https://en.wikipedia.org/wiki/File:171879main_LimbFlareJan12_lg.jpg
010_Sun/04_Chromosphere/Title = Taken by Hinode's Solar Optical Telescope on Jan. 12, 2007, this image of the sun reveals the filamentary nature of the plasma connecting regions of different magnetic polarity. Hinode captures these very dynamic pictures of the chromosphere. The chromosphere is a thin "layer" of solar atmosphere "sandwiched" between the visible surface, photosphere, and corona.
010_Sun/04_Chromosphere/URL = https://upload.wikimedia.org/wikipedia/commons/d/da/171879main_LimbFlareJan12_lg.jpg
010_Sun/05_Sunspot/License = https://en.wikipedia.org/wiki/File:172197main_NASA_Flare_Gband_lg-withouttext.jpg
010_Sun/05_Sunspot/Title = Granules-like structure of surface of sun and sunspots (size around 20'000km). Visible light. Taken by Hinode's Solar Optical Telescope (SOT).
010_Sun/05_Sunspot/URL = https://upload.wikimedia.org/wikipedia/commons/4/44/172197main_NASA_Flare_Gband_lg-withouttext.jpg
010_Sun/06_Prominence/License = https://en.wikipedia.org/wiki/File:Giant_prominence_on_the_sun_erupted.jpg
010_Sun/06_Prominence/Title = On Aug. 31, 2012, a giant prominence on the sun erupted, sending out particles and a shock wave that traveled near Earth. This event may have been one of the causes of a third radiation belt that appeared around Earth a few days later, a phenomenon that was observed for the very first time by the newly-launched Van Allen Probes. This image of the prominence before it erupted was captured by NASA's Solar Dynamics Observatory (SDO).
010_Sun/06_Prominence/URL = https://upload.wikimedia.org/wikipedia/commons/a/a3/Giant_prominence_on_the_sun_erupted.jpg
010_Sun/90_Explore_50_ParkerSolarProbe_1/License = https://en.wikipedia.org/wiki/File:Parker_Solar_Probe.jpg
010_Sun/90_Explore_50_ParkerSolarProbe_1/Title = Artist0x2019s concept of the Parker Solar Probe spacecraft approaching the sun. On 29 October 2018, at about 18:04 UTC, the spacecraft became the closest ever artificial object to the Sun. As of its perihelion on 27 September 2020, the Parker Solar Probe's closest approach is 13.5 million kilometres. This will be surpassed after each successive flyby of Venus.
010_Sun/90_Explore_50_ParkerSolarProbe_1/URL = https://upload.wikimedia.org/wikipedia/commons/1/1c/Parker_Solar_Probe.jpg
010_Sun/90_Explore_50_ParkerSolarProbe_2_ThermalTesting/License = https://en.wikipedia.org/wiki/File:Thermal_testing_of_the_solar_array_cooling_system_for_the_Parker_Solar_Probe.jpg
010_Sun/90_Explore_50_ParkerSolarProbe_2_ThermalTesting/Title = The solar array cooling system for the Parker Solar Probe spacecraft0x2014one element of which is the large, square black radiator visible at center, one of two that will be installed0x2014is shown undergoing thermal testing at NASA Goddard Space Flight Center in Greenbelt, Maryland in late February 2017.
010_Sun/90_Explore_50_ParkerSolarProbe_2_ThermalTesting/URL = https://upload.wikimedia.org/wikipedia/commons/4/49/Thermal_testing_of_the_solar_array_cooling_system_for_the_Parker_Solar_Probe.jpg
010_Sun/90_Explore_50_ParkerSolarProbe_3_Launch/License = https://en.wikipedia.org/wiki/File:Parker_Solar_Probe_Launch_(NHQ201808120013).jpg
010_Sun/90_Explore_50_ParkerSolarProbe_3_Launch/Title = The United Launch Alliance Delta IV Heavy rocket launches NASA's Parker Solar Probe to touch the Sun, Sunday, Aug. 12, 2018 from Launch Complex 37 at Cape Canaveral Air Force Station, Florida. Parker Solar Probe is humanity0x2019s first-ever mission into a part of the Sun0x2019s atmosphere called the corona.
010_Sun/90_Explore_50_ParkerSolarProbe_3_Launch/URL = https://upload.wikimedia.org/wikipedia/commons/0/00/Parker_Solar_Probe_Launch_(NHQ201808120013).jpg
110_Mercury/License = https://en.wikipedia.org/wiki/File:Mercury_in_color_-_Prockter07-edit1.jpg
110_Mercury/Title = Mercury is the smallest and innermost planet in the Solar System. Its orbit around the Sun takes 87.97 Earth days, the shortest of all the planets in the Solar System. It is named after the Greek god Hermes (0x03950x03C10x03BC0x03AE0x03C2), translated into Latin Mercurius Mercury, god of commerce, messenger of the gods, mediator between gods and mortals.
110_Mercury/URL = https://upload.wikimedia.org/wikipedia/commons/d/d9/Mercury_in_color_-_Prockter07-edit1.jpg
110_Mercury/10_CompareEarth/License = https://en.wikipedia.org/wiki/File:Mercury,_Earth_size_comparison.jpg
110_Mercury/10_CompareEarth/Title = Size comparison of Mercury and Earth. Approximate scale is 29 km/px.
110_Mercury/10_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/8/8c/Mercury,_Earth_size_comparison.jpg
110_Mercury/11_CompareEarthMarsVenus/License = https://en.wikipedia.org/wiki/File:Terrestrial_planet_sizes2.jpg
110_Mercury/11_CompareEarthMarsVenus/Title = This diagram shows the approximate relative sizes of the terrestrial planets, from left to right: Mercury, Venus, Earth and Mars. Distances are not to scale. A terrestrial planet is a planet that is primarily composed of silicate rocks. The term is derived from the Latin word for Earth, "Terra", so an alternate definition would be that these are planets which are, in some notable fashion, "Earth-like". Terrestrial planets are substantially different from gas giants, which might not have solid surfaces and are composed mostly of some combination of hydrogen, helium, and water existing in various physical states. Terrestrial planets all have roughly the same structure: a central metallic core, mostly iron, with a surrounding silicate mantle. Terrestrial planets have canyons, craters, mountains, volcanoes and secondary atmospheres.
110_Mercury/11_CompareEarthMarsVenus/URL = https://upload.wikimedia.org/wikipedia/commons/7/7c/Terrestrial_planet_sizes2.jpg
110_Mercury/2_Tolstoj/License = https://en.wikipedia.org/wiki/File:EW1027346412Gnomap.png
110_Mercury/2_Tolstoj/Title = The Tolstoj basin (355 km in diameter) can be seen at the bottom edge of the frame, its center filled with smooth plains and surrounded by a large region of low-reflectance ejecta. The fresh, bright-rayed crater Nureyev is visible near the limb.
110_Mercury/2_Tolstoj/URL = https://upload.wikimedia.org/wikipedia/commons/0/0e/EW1027346412Gnomap.png
110_Mercury/3_Abedin/License = https://en.wikipedia.org/wiki/File:Oblique_Abedin_2015.png
110_Mercury/3_Abedin/Title = This mosaic of oblique images highlights the spectacular interior of Abedin crater. The crater floor is covered with once-molten rock melted by the impact event that formed Abedin. Cracks that formed as this melt cooled are visible. Particularly intriguing is the shallow depression that lies amidst the central peaks of the crater and may be volcanic in origin. Color imaging shows that this depression is surrounded by reddish material, as seen at other sites of explosive volcanism across Mercury.
110_Mercury/3_Abedin/URL = https://upload.wikimedia.org/wikipedia/commons/e/e2/Oblique_Abedin_2015.png
110_Mercury/4_NorthPole/License = https://en.wikipedia.org/wiki/File:North_pole_of_Mercury_--_NASA.jpg
110_Mercury/4_NorthPole/Title = The dark region at the center of this image, pieced together from photographs taken by NASA's Messenger spacecraft, includes the north pole of Mercury. Because Mercury's spin axis is almost exactly vertical, sunlight never reaches the bottoms of craters near the poles, and water ice can persist in the ultra cold temperatures there
110_Mercury/4_NorthPole/URL = https://upload.wikimedia.org/wikipedia/commons/9/93/North_pole_of_Mercury_--_NASA.jpg
110_Mercury/5_Transit/License = https://en.wikipedia.org/wiki/File:Transit_Of_Mercury,_May_9th,_2016.png
110_Mercury/5_Transit/Title = Transit of Mercury. Mercury is visible as a black dot below and to the left of center. The dark area above the center of the solar disk is a sunspot.
110_Mercury/5_Transit/URL = https://upload.wikimedia.org/wikipedia/commons/2/2c/Transit_Of_Mercury,_May_9th,_2016.png
110_Mercury/9_Explore_1_Mariner/License = https://en.wikipedia.org/wiki/File:Mariner_10.jpg
110_Mercury/9_Explore_1_Mariner/Title = Mariner 10 was an American robotic space probe launched by NASA on 3 November 1973, to fly by the planets Mercury and Venus. It was the first spacecraft to perform flybys of multiple planets. This model of Mariner 10 shows the spacecraft as it appeared during flight. The Mariner 10 mission required more course corrections than any previous mission and was the first spacecraft to use the gravitational pull of one planet to help it reach another planet. This craft was also the first to use the solar wind as a means of locomotion0x003B when the probe's thruster fuel ran low, scientists used the solar panels as sails to make course corrections.
110_Mercury/9_Explore_1_Mariner/URL = https://upload.wikimedia.org/wikipedia/commons/thumb/f/fe/Mariner_10.jpg/3008px-Mariner_10.jpg
110_Mercury/9_Explore_2_Messenger/License = https://en.wikipedia.org/wiki/File:MESSENGER_-_spacecraft_at_mercury_-_atmercury_lg.jpg
110_Mercury/9_Explore_2_Messenger/Title = Artist depiction of the MESSENGER spacecraft in orbit around Mercury. MESSENGER was a NASA robotic space probe that orbited the planet Mercury between 2011 and 2015, studying Mercury's chemical composition, geology, and magnetic field. MESSENGER was launched aboard a Delta II rocket in August 2004. Its path involved a complex series of flybys 0x2013 the spacecraft flew by Earth once, Venus twice, and Mercury itself three times, allowing it to decelerate relative to Mercury using minimal fuel.
110_Mercury/9_Explore_2_Messenger/URL = https://upload.wikimedia.org/wikipedia/commons/6/6c/MESSENGER_-_spacecraft_at_mercury_-_atmercury_lg.jpg
110_Mercury/9_Explore_2_Messenger_2_Assembly/License = https://en.wikipedia.org/wiki/File:MESSENGER_Assembly.jpg
110_Mercury/9_Explore_2_Messenger_2_Assembly/Title = Technicians prepare MESSENGER.
110_Mercury/9_Explore_2_Messenger_2_Assembly/URL = https://upload.wikimedia.org/wikipedia/commons/b/b6/MESSENGER_Assembly.jpg
110_Mercury/9_Explore_2_Messenger_3_DeltaII/License = https://en.wikipedia.org/wiki/File:MESSENGER_-_exploded_launch_vehicle_diagram.png
110_Mercury/9_Explore_2_Messenger_3_DeltaII/Title = Exploded diagram of the Delta II launch vehicle for the MESSENGER spacecraft.
110_Mercury/9_Explore_2_Messenger_3_DeltaII/URL = https://upload.wikimedia.org/wikipedia/commons/2/2c/MESSENGER_-_exploded_launch_vehicle_diagram.png
110_Mercury/9_Explore_2_Messenger_4_Launch/License = https://en.wikipedia.org/wiki/File:MESSENGER_launch_on_Delta_7925_rocket.jpg
110_Mercury/9_Explore_2_Messenger_4_Launch/Title = The tip of the Boeing Delta II rocket with its MESSENGER spacecraft on top breaks through the billows of smoke below as it lifts.
110_Mercury/9_Explore_2_Messenger_4_Launch/URL = https://upload.wikimedia.org/wikipedia/commons/d/dd/MESSENGER_launch_on_Delta_7925_rocket.jpg
110_Mercury/9_Explore_3_BepiColombo/License = https://en.wikipedia.org/wiki/File:BepiColombo_spacecraft_model.png
110_Mercury/9_Explore_3_BepiColombo/Title = BepiColombo is a joint mission of the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA) to the planet Mercury.0x005B40x005D The mission comprises two satellites launched together: the Mercury Planetary Orbiter (MPO) and Mio (Mercury Magnetospheric Orbiter, MMO)
110_Mercury/9_Explore_3_BepiColombo/URL = https://upload.wikimedia.org/wikipedia/commons/d/d4/BepiColombo_spacecraft_model.png
110_Mercury/9_Explore_3_BepiColombo_2_MPO/License = https://en.wikipedia.org/wiki/File:BepiColombo_MPO_ESTEC.jpg
110_Mercury/9_Explore_3_BepiColombo_2_MPO/Title = BepiColombo Mercury Planetary Orbiter in ESTEC, before launch.
110_Mercury/9_Explore_3_BepiColombo_2_MPO/URL = https://upload.wikimedia.org/wikipedia/commons/3/34/BepiColombo_MPO_ESTEC.jpg
110_Mercury/9_Explore_3_BepiColombo_3_MMO/License = https://en.wikipedia.org/wiki/File:BepiColombo_MMO_ESTEC.jpg
110_Mercury/9_Explore_3_BepiColombo_3_MMO/Title = BepiColombo Mercury Magnetospheric Orbiter in ESTEC, before launch.
110_Mercury/9_Explore_3_BepiColombo_3_MMO/URL = https://upload.wikimedia.org/wikipedia/commons/a/a0/BepiColombo_MMO_ESTEC.jpg
115_Venus/License = https://en.wikipedia.org/wiki/File:PIA23791-Venus-NewlyProcessedView-20200608.jpg
115_Venus/Title = Venus is the second planet from the Sun. It is named after the Roman goddess of love and beauty. As the second-brightest natural object in Earth's night sky after the Moon, Venus can cast shadows and can be, on rare occasion, visible to the naked eye in broad daylight.0x005B150x005D0x005B160x005D Venus lies within Earth's orbit, and so never appears to venture far from the Sun, either setting in the west just after dusk or rising in the east a bit before dawn.
115_Venus/URL = https://upload.wikimedia.org/wikipedia/commons/a/a9/PIA23791-Venus-NewlyProcessedView-20200608.jpg
115_Venus/2_CompareEarth/License = https://en.wikipedia.org/wiki/File:Venus,_Earth_size_comparison.jpg
115_Venus/2_CompareEarth/Title = Size comparison of Venus (using a false-colour, radar-based image of the surface) and Earth
115_Venus/2_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/9/92/Venus,_Earth_size_comparison.jpg
115_Venus/3_Rotation_1_Topographic/License = https://en.wikipedia.org/wiki/File:Topographic_Globe_of_Venus.gif
115_Venus/3_Rotation_1_Topographic/Title = Topographic Globe of Venus from Magellan radar altimetry data
115_Venus/3_Rotation_1_Topographic/URL = https://upload.wikimedia.org/wikipedia/commons/0/0b/Topographic_Globe_of_Venus.gif
115_Venus/3_Rotation_2_Radar/License = https://en.wikipedia.org/wiki/File:Radar_Globe_of_Venus.gif
115_Venus/3_Rotation_2_Radar/Title = Radar map of Venus
115_Venus/3_Rotation_2_Radar/URL = https://upload.wikimedia.org/wikipedia/commons/8/8b/Radar_Globe_of_Venus.gif
115_Venus/4_LaviniaPlanitia/License = https://en.wikipedia.org/wiki/File:PIA00103_Venus_-_3-D_Perspective_View_of_Lavinia_Planitia.jpg
115_Venus/4_LaviniaPlanitia/Title = Impact craters on the surface of Venus (false-colour image reconstructed from radar data). Three impact craters are displayed in this three-dimensional perspective view of the surface of Venus. The center of the image is located at approximately 27 degrees south latitude, 339 degrees east longitude in the northwestern portion of Lavinia Planitia. Magellan synthetic aperture radar data is combined with radar altimetry to develop a three-dimensional map of the surface.
115_Venus/4_LaviniaPlanitia/URL = https://upload.wikimedia.org/wikipedia/commons/6/60/PIA00103_Venus_-_3-D_Perspective_View_of_Lavinia_Planitia.jpg
115_Venus/5_RadarView/License = https://en.wikipedia.org/wiki/File:Venus_globe.jpg
115_Venus/5_RadarView/Title = False-color global radar view of Venus (without the clouds) from Magellan between 1990 and 1994. This global view of the surface of Venus is centered at 180 degrees east longitude. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a computer-simulated globe to create this image. Data gaps are filled with Pioneer Venus Orbiter data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. The image was produced by the Solar System Visualization project and the Magellan science team at the JPL Multimission Image Processing Laboratory and is a single frame from a video released at the October 29, 1991, JPL news conference. It is important to note that Venus is completely shrouded in clouds. A bright elongated region in the center is Aphrodite Terra.
115_Venus/5_RadarView/URL = https://upload.wikimedia.org/wikipedia/commons/8/85/Venus_globe.jpg
115_Venus/6_FromEarth/License = https://en.wikipedia.org/wiki/File:Venus-pacific-levelled.jpg
115_Venus/6_FromEarth/Title = Venus reflected on the Pacific Ocean. Venus, pictured center-right, is always brighter than all other planets or stars as seen from Earth. Jupiter is visible at the top of the image.
115_Venus/6_FromEarth/URL = https://upload.wikimedia.org/wikipedia/commons/5/52/Venus-pacific-levelled.jpg
115_Venus/7_GroundVenera9/License = https://en.wikipedia.org/wiki/File:Foto_de_Venera_9.png
115_Venus/7_GroundVenera9/Title = Image of the surface of Venus taken by Venera 9 in 1975. 
115_Venus/7_GroundVenera9/URL = https://upload.wikimedia.org/wikipedia/commons/f/ff/Foto_de_Venera_9.png
115_Venus/90_Explore_1_Vega2/License = https://en.wikipedia.org/wiki/File:Vega_model_-_Udvar-Hazy_Center.JPG
115_Venus/90_Explore_1_Vega2/Title = Vega solar system probe bus and landing apparatus (model) 
115_Venus/90_Explore_1_Vega2/URL = https://upload.wikimedia.org/wikipedia/commons/5/52/Vega_model_-_Udvar-Hazy_Center.JPG
115_Venus/90_Explore_1_Vega2_2_Balloon/License = https://en.wikipedia.org/wiki/File:Russian_"Vega"_balloon_mission_to_Venus_on_display_at_the_Udvar-Hazy_museum.jpg
115_Venus/90_Explore_1_Vega2_2_Balloon/Title = Russian "Vega" balloon mission to the atmosphere of Venus on display at the Steven F. Udvar-Hazy Center of the Smithsonian Institution. 
115_Venus/90_Explore_1_Vega2_2_Balloon/URL = https://upload.wikimedia.org/wikipedia/commons/3/33/Russian_"Vega"_balloon_mission_to_Venus_on_display_at_the_Udvar-Hazy_museum.jpg
115_Venus/90_Explore_3_VEX/License = https://en.wikipedia.org/wiki/File:Venus_Express_in_orbit_(crop).jpg
115_Venus/90_Explore_3_VEX/Title = Venus Express (VEX) was the first Venus exploration mission of the European Space Agency (ESA). Launched in November 2005, it arrived at Venus in April 2006 and began continuously sending back science data from its polar orbit around Venus. Equipped with seven scientific instruments, the main objective of the mission was the long term observation of the Venusian atmosphere. The observation over such long periods of time had never been done in previous missions to Venus.
115_Venus/90_Explore_3_VEX/URL = https://upload.wikimedia.org/wikipedia/commons/0/0b/Venus_Express_in_orbit_(crop).jpg
115_Venus/90_Explore_4_Akatsuki/License = https://en.wikipedia.org/wiki/File:H-IIA_F17_launching_AKATSUKI.jpg
115_Venus/90_Explore_4_Akatsuki/Title = H-IIA Launch Vehicle Flight 17, launching Venus Climate Orbiter "AKATSUKI".
115_Venus/90_Explore_4_Akatsuki/URL = https://upload.wikimedia.org/wikipedia/commons/f/fb/H-IIA_F17_launching_AKATSUKI.jpg
120_Earth/License = https://en.wikipedia.org/wiki/File:The_Earth_seen_from_Apollo_17.jpg
120_Earth/Title = "The Blue Marble" is a famous photograph of the Earth taken on December 7, 1972, by the crew of the Apollo 17 spacecraft en route to the Moon at a distance of about 29,000 kilometres (18,000 mi). It shows Africa, Antarctica, and the Arabian Peninsula.
120_Earth/URL = https://upload.wikimedia.org/wikipedia/commons/9/97/The_Earth_seen_from_Apollo_17.jpg
120_Earth/2_Earthrise/License = https://en.wikipedia.org/wiki/File:NASA-Apollo8-Dec24-Earthrise.jpg
120_Earth/2_Earthrise/Title = Taken by Apollo 8 crewmember Bill Anders on December 24, 1968 while in orbit around the Moon, showing the Earth rising above the lunar horizon. Note that this phenomenon ("Earthrise") is only visible to an observer in motion relative to the lunar surface. Because of the Moon's synchronous rotation relative to the Earth (i.e., the same side of the Moon is always facing Earth), the Earth appears to be stationary (measured in anything less than a geological timescale) in the lunar "sky". In order to observe the effect of Earth rising or setting over the Moon's horizon, an observer must travel towards or away from the point on the lunar surface where the Earth is most directly overhead (centred in the sky).
120_Earth/2_Earthrise/URL = https://upload.wikimedia.org/wikipedia/commons/a/a8/NASA-Apollo8-Dec24-Earthrise.jpg
121_Moon/License = https://en.wikipedia.org/wiki/File:FullMoon2010.jpg
121_Moon/Title = By Gregory H. Revera. Full Moon photograph taken 10-22-2010 from Madison, Alabama, USA. Photographed with a Celestron 9.25 Schmidt-Cassegrain telescope. Acquired with a Canon EOS Rebel T1i (EOS 500D), 20 images stacked to reduce noise. 200 ISO 1/640 sec.
121_Moon/URL = https://upload.wikimedia.org/wikipedia/commons/e/e1/FullMoon2010.jpg
121_Moon/10_CompareEarth/License = https://en.wikipedia.org/wiki/File:Earth-moon-to-scale.svg
121_Moon/10_CompareEarth/Title = Illustration of Earth and Moon at the average distance from each other (semi-major axis) as seen from distant space.
121_Moon/10_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/thumb/3/3f/Earth-moon-to-scale.svg/3200px-Earth-moon-to-scale.svg.png
121_Moon/2_FarSide/License = https://en.wikipedia.org/wiki/File:Moon_Farside_LRO.jpg
121_Moon/2_FarSide/Title =  Far side of the moon, by NASA's Lunar Reconnaissance Orbiter. Orthographic projection centred at 1800x00B0 longitude, 00x00B0 latitude. Because the moon is tidally locked (meaning the same side always faces Earth), it was not until 1959 that the farside was first imaged by the Soviet Luna 3 spacecraft (hence the Russian names for prominent farside features, such as Mare Moscoviense). And what a surprise 0x2013 unlike the widespread maria on the nearside, basaltic volcanism was restricted to a relatively few, smaller regions on the farside, and the battered highlands crust dominated. A different world from what we saw from Earth.
121_Moon/2_FarSide/URL = https://upload.wikimedia.org/wikipedia/commons/thumb/0/04/Moon_Farside_LRO.jpg/1024px-Moon_Farside_LRO.jpg
121_Moon/4_TransitEarth/License = https://en.wikipedia.org/wiki/File:Dscovrepicmoontransitfull.gif
121_Moon/4_TransitEarth/Title = This animation features satellite images of the far side of the Moon, illuminated by the Sun, as it crosses between the DSCOVR spacecraft's Earth Polychromatic Imaging Camera (EPIC) and telescope, and the Earth 0x2014 one million miles (1.6 million km) away. The times of the images span from 3:50 p.m. to 8:45 p.m. EDT on July 16, 2015.
121_Moon/4_TransitEarth/URL = https://upload.wikimedia.org/wikipedia/commons/5/50/Dscovrepicmoontransitfull.gif
121_Moon/5_Libration/License = https://en.wikipedia.org/wiki/File:Lunar_libration_with_phase_Oct_2007_(continuous_loop).gif
121_Moon/5_Libration/Title = The libration of the Moon over a single lunar month. Also visible is the slight variation in the Moon's visual size from Earth.
121_Moon/5_Libration/URL = https://upload.wikimedia.org/wikipedia/commons/c/ca/Lunar_libration_with_phase_Oct_2007_(continuous_loop).gif
121_Moon/6_Apollo11/License = https://en.wikipedia.org/wiki/File:As11-40-5886,_uncropped.jpg
121_Moon/6_Apollo11/Title = Neil Armstrong works at the LM in one of the few photos taken of him on the moon.
121_Moon/6_Apollo11/URL = https://upload.wikimedia.org/wikipedia/commons/f/fb/As11-40-5886,_uncropped.jpg
121_Moon/7_Apollo15LunarRover/License = https://en.wikipedia.org/wiki/File:Apollo_15_Lunar_Rover_and_Irwin.jpg
121_Moon/7_Apollo15LunarRover/Title = Image from Apollo 15, taken by Commander David Scott at the end of EVA-1. Lunar Module Pilot Jim Irwin is seen with the Lunar Roving Vehicle, with Mount Hadley in the background. Seen on the back of the Rover are two SCBs mounted on the gate, along with the rake, both pairs of tongs, the extension handle with scoop probably attached, and the penetrometer. Note that the TV camera is pointed down, in the stowed position.
121_Moon/7_Apollo15LunarRover/URL = https://upload.wikimedia.org/wikipedia/commons/2/2e/Apollo_15_Lunar_Rover_and_Irwin.jpg
122_Eros/License = https://en.wikipedia.org/wiki/File:Eros_-_PIA02923_(color).jpg
122_Eros/Title = Eros is a stony and elongated asteroid of the Amor group and the first discovered and second-largest near-Earth object with a mean diameter of approximately 16.8 kilometers. Visited by the NEAR Shoemaker space probe in 1998, it became the first asteroid ever studied from orbit. The eccentric asteroid was discovered by German astronomer Carl Gustav Witt at the Berlin Observatory on 13 August 1898, and later named after Eros, a god from Greek mythology0x003B the son of Aphrodite who is identified with the planet Venus.
122_Eros/URL = https://upload.wikimedia.org/wikipedia/commons/e/e5/Eros_-_PIA02923_(color).jpg
122_Eros/02_Rotation/License = https://en.wikipedia.org/wiki/File:Eros_rotation_Dec._3-4_2000.gif
122_Eros/02_Rotation/Title = NEAR Shoemaker captured this movie on December 3-4, 2000, while in orbit 200 kilometers from the center of Eros. Covering a full rotation of the 21-mile-long asteroid, the movie opens with a look at one of Eros' battered ends and a sweep over the saddle-shaped depression named Himeros. The sequence then includes a view of Shoemaker Regio - the large boulder patch beside Himeros - before swinging over the opposite end and providing a stunning view of a sunset inside Psyche, the asteroid's large, 5-kilometer (3-mile) impact crater. The movie wraps up with a return to the asteroid's heavily cratered tip.
122_Eros/02_Rotation/URL = https://upload.wikimedia.org/wikipedia/commons/5/5f/Eros_rotation_Dec._3-4_2000.gif
122_Eros/03_SixViews/License = https://en.wikipedia.org/wiki/File:PIA02475_Eros'_Bland_Butterscotch_Colors.jpg
122_Eros/03_SixViews/Title = Six different views of Eros in approximate natural color from NEAR-Shoemaker in February 2000
122_Eros/03_SixViews/URL = https://upload.wikimedia.org/wikipedia/commons/6/68/PIA02475_Eros'_Bland_Butterscotch_Colors.jpg
122_Eros/04_CloseUpRegolith/License = https://en.wikipedia.org/wiki/File:Erosregolith.jpg
122_Eros/04_CloseUpRegolith/Title = Regolith of Eros, seen during NEAR's descent0x003B area shown is about 12 meters (40 feet) across
122_Eros/04_CloseUpRegolith/URL = https://upload.wikimedia.org/wikipedia/commons/a/a6/Erosregolith.jpg
122_Eros/90_Explore_01_NEARShoemaker_01/License = https://en.wikipedia.org/wiki/File:NEAR_Shoemaker_spacecraft_model.png
122_Eros/90_Explore_01_NEARShoemaker_01/Title = The Near Earth Asteroid Rendezvous 0x2013 Shoemaker (NEAR Shoemaker), renamed after its 1996 launch in honor of planetary scientist Eugene Shoemaker, was a robotic space probe designed by the Johns Hopkins University Applied Physics Laboratory for NASA to study the near-Earth asteroid Eros from close orbit over a period of a year. The mission succeeded in closing in with the asteroid and orbited it several times, finally terminating by touching down on the asteroid on February 12, 2001.
122_Eros/90_Explore_01_NEARShoemaker_01/URL = https://upload.wikimedia.org/wikipedia/commons/c/cb/NEAR_Shoemaker_spacecraft_model.png
122_Eros/90_Explore_01_NEARShoemaker_02_InsideRocket/License = https://en.wikipedia.org/wiki/File:NEARCraft.jpg
122_Eros/90_Explore_01_NEARShoemaker_02_InsideRocket/Title = NEAR spacecraft inside its Delta II rocket.
122_Eros/90_Explore_01_NEARShoemaker_02_InsideRocket/URL = https://upload.wikimedia.org/wikipedia/commons/f/fa/NEARCraft.jpg
122_Eros/90_Explore_01_NEARShoemaker_03_Launch/License = https://en.wikipedia.org/wiki/File:NEARlaunch.jpg
122_Eros/90_Explore_01_NEARShoemaker_03_Launch/Title = Launch of the NEAR spacecraft, February 1996.
122_Eros/90_Explore_01_NEARShoemaker_03_Launch/URL = https://upload.wikimedia.org/wikipedia/commons/9/94/NEARlaunch.jpg
123_162173Ryugu/License = https://en.wikipedia.org/wiki/File:162173_Ryugu.jpg
123_162173Ryugu/Title = 162173 Ryugu, provisional designation 1999 JU3, is a near-Earth object and a potentially hazardous asteroid of the Apollo group. It measures approximately 1 kilometre in diameter and is a dark object of the rare spectral type Cb, with qualities of both a C-type asteroid and a B-type asteroid. In June 2018, the Japanese spacecraft Hayabusa2 arrived at the asteroid. After making measurements and taking samples, Hayabusa2 left Ryugu for Earth in November 2019 and returned the sample capsule to Earth on 5 December 2020. Photograph of the full disc of the asteroid 162173 Ryugu, as it appeared to the Hayabusa2 spacecraft at 03:50 UTC on 26 June 2018. The photograph was taken by the spacecraft's Optical Navigation Camera 0x2013 Telescopic (ONC-T) at a distance of 20 kilometres.
123_162173Ryugu/URL = https://upload.wikimedia.org/wikipedia/en/7/75/162173_Ryugu.jpg
123_162173Ryugu/2_Rotation/License = https://en.wikipedia.org/wiki/File:Ryugu_rotation.gif
123_162173Ryugu/2_Rotation/Title = Rotation gif of 162173 Ryugu. Image Credit: JAXA Hayabusa 2 ONC-T v-filter. Date observation: 2018-07-10.
123_162173Ryugu/2_Rotation/URL = https://upload.wikimedia.org/wikipedia/commons/f/f4/Ryugu_rotation.gif
123_162173Ryugu/9_Explore_1_Hayabusa2/License = https://en.wikipedia.org/wiki/File:Hayabusa2_Ion_thruster.jpg
123_162173Ryugu/9_Explore_1_Hayabusa2/Title = Artist's impression of Hayabusa2 firing its ion thrusters
123_162173Ryugu/9_Explore_1_Hayabusa2/URL = https://upload.wikimedia.org/wikipedia/commons/5/5f/Hayabusa2_Ion_thruster.jpg
124_25143Itokawa/License = https://en.wikipedia.org/wiki/File:Hayabausa_Image_of_the_asteroid_Itokawa.jpg
124_25143Itokawa/Title = 25143 Itokawa is a sub-kilometer near-Earth object of the Apollo group and a potentially hazardous asteroid. It was discovered by the LINEAR program in 1998 and later named after Japanese rocket engineer Hideo Itokawa. The peanut-shaped S-type asteroid has a rotation period of 12.1 hours and measures approximately 330 meters (1,100 feet) in diameter. Due to its low density and high porosity, Itokawa is considered to be a rubble pile, consisting of numerous boulders of different sizes rather than of a single solid body. Itokawa is the smallest asteroid ever photographed and visited by a spacecraft.
124_25143Itokawa/URL = https://upload.wikimedia.org/wikipedia/en/d/d1/Hayabausa_Image_of_the_asteroid_Itokawa.jpg
130_Mars/License = https://en.wikipedia.org/wiki/File:OSIRIS_Mars_true_color.jpg
130_Mars/Title = True color image of Mars taken by the OSIRIS instrument on the ESA Rosetta spacecraft during its February 2007 flyby of the planet. The image was generated using the OSIRIS orange (red), green, and blue filters.
130_Mars/URL = https://upload.wikimedia.org/wikipedia/commons/0/02/OSIRIS_Mars_true_color.jpg
130_Mars/02_CompareEarth/License = https://en.wikipedia.org/wiki/File:Mars,_Earth_size_comparison.jpg
130_Mars/02_CompareEarth/Title = Size comparison of Earth and Mars.
130_Mars/02_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/c/cf/Mars,_Earth_size_comparison.jpg
130_Mars/03_KorolevCrater/License = https://en.wikipedia.org/wiki/File:Perspective_view_of_Korolev_crater.jpg
130_Mars/03_KorolevCrater/Title = Perspective view of Korolev crater shows 1.9 kilometres (1.2 mi) deep water ice. Image taken by ESA's Mars Express. Korolev crater is an 82-kilometre-across feature found in the northern lowlands of Mars.
130_Mars/03_KorolevCrater/URL = https://upload.wikimedia.org/wikipedia/commons/7/75/Perspective_view_of_Korolev_crater.jpg
130_Mars/04_MountSharp/License = https://en.wikipedia.org/wiki/File:PIA19912-MarsCuriosityRover-MountSharp-20151002.jpg
130_Mars/04_MountSharp/Title = This composite image looking toward the higher regions of Mount Sharp was taken on September 9, 2015, by NASA's Curiosity rover. In the foreground -- about 2 miles (3 kilometers) from the rover -- is a long ridge teeming with hematite, an iron oxide. Just beyond is an undulating plain rich in clay minerals. And just beyond that are a multitude of rounded buttes, all high in sulfate minerals.
130_Mars/04_MountSharp/URL = https://upload.wikimedia.org/wikipedia/commons/b/b0/PIA19912-MarsCuriosityRover-MountSharp-20151002.jpg
130_Mars/05_Rock/License = https://en.wikipedia.org/wiki/File:PIA16452-MarsCuriosityRover-Rocknest3Rock-20121005.jpg
130_Mars/05_Rock/Title = A Martian Rock Called 'Rocknest 3'
130_Mars/05_Rock/URL = https://upload.wikimedia.org/wikipedia/commons/b/b1/PIA16452-MarsCuriosityRover-Rocknest3Rock-20121005.jpg
130_Mars/06_SoilAndTracks/License = https://en.wikipedia.org/wiki/File:PIA17944-MarsCuriosityRover-AfterCrossingDingoGapSanddune-20140209.jpg
130_Mars/06_SoilAndTracks/Title = This look back at a dune that NASA's Curiosity Mars rover drove across was taken by the rover's Mast Camera (Mastcam). The rover had driven over the dune three days earlier. 
130_Mars/06_SoilAndTracks/URL = https://upload.wikimedia.org/wikipedia/commons/d/dc/PIA17944-MarsCuriosityRover-AfterCrossingDingoGapSanddune-20140209.jpg
130_Mars/07_DustDevil/License = https://en.wikipedia.org/wiki/File:PIA24039-MarsCuriosityRover-DustDevil-20200809.gif
130_Mars/07_DustDevil/Title = NASA's Curiosity Mars rover spotted this dust devil with one of its Navigation Cameras around 11:35 a.m. local Mars time on Aug. 9, 2020 (the 2,847th Martian day, or sol, of the mission). The frames in this GIF were shot over 4 minutes and 15 seconds.
130_Mars/07_DustDevil/URL = https://upload.wikimedia.org/wikipedia/commons/1/10/PIA24039-MarsCuriosityRover-DustDevil-20200809.gif
130_Mars/08_DustStorm/License = https://en.wikipedia.org/wiki/File:PIA03170_fig1duststroms.jpg
130_Mars/08_DustStorm/Title = Mars without a dust storm on June 2001 (on left) and with a dust storm on July 2001 (on right), as seen by Mars Global Surveyor.
130_Mars/08_DustStorm/URL = https://upload.wikimedia.org/wikipedia/commons/e/ee/PIA03170_fig1duststroms.jpg
130_Mars/09_Rabe/License = https://en.wikipedia.org/wiki/File:Rabe_Crater_perspective_ESA310887.jpg
130_Mars/09_Rabe/Title = Rabe Crater is a 108 km-wide impact crater with an intricately shaped dune field. The dune material likely comprises locally eroded sediments that have been shaped by prevailing winds. Other smaller craters in the region also contain these dark deposits. One relatively young and deep crater can be seen in the upper left0x003B as well as the dark material, channels and grooves are clearly visible in its crater walls.
130_Mars/09_Rabe/URL = https://upload.wikimedia.org/wikipedia/commons/d/d2/Rabe_Crater_perspective_ESA310887.jpg
130_Mars/90_Explore_05_GlobalSurveyor/License = https://en.wikipedia.org/wiki/File:Mars_global_surveyor.jpg
130_Mars/90_Explore_05_GlobalSurveyor/Title = Artist concept of the Mars Global Surveyor.
130_Mars/90_Explore_05_GlobalSurveyor/URL = https://upload.wikimedia.org/wikipedia/commons/d/d8/Mars_global_surveyor.jpg
130_Mars/90_Explore_10_MER/License = https://en.wikipedia.org/wiki/File:NASA_Mars_Rover.jpg
130_Mars/90_Explore_10_MER/Title = Artist's rendering of a Mars Exploration Rover
130_Mars/90_Explore_10_MER/URL = https://upload.wikimedia.org/wikipedia/commons/d/d8/NASA_Mars_Rover.jpg
130_Mars/90_Explore_20_Curiosity_1/License = https://en.wikipedia.org/wiki/File:Curiosity_Self-Portrait_at_'Big_Sky'_Drilling_Site.jpg
130_Mars/90_Explore_20_Curiosity_1/Title = This self-portrait of NASA's Curiosity Mars rover shows the vehicle at the "Big Sky" site, where its drill collected the mission's fifth taste of Mount Sharp.  It does not include the rover's robotic arm, though the shadow of the arm is visible on the ground.
130_Mars/90_Explore_20_Curiosity_1/URL = https://upload.wikimedia.org/wikipedia/commons/f/f3/Curiosity_Self-Portrait_at_'Big_Sky'_Drilling_Site.jpg
130_Mars/90_Explore_20_Curiosity_2/License = https://en.wikipedia.org/wiki/File:PIA15279_3rovers-stand_D2011_1215_D521.jpg
130_Mars/90_Explore_20_Curiosity_2/Title = Two spacecraft engineers stand with a group of vehicles providing a comparison of three generations of Mars rovers developed at NASA's Jet Propulsion Laboratory, Pasadena, Calif. The setting is JPL's Mars Yard testing area. Front and center is the flight spare for the first Mars rover, Sojourner, which landed on Mars in 1997 as part of the Mars Pathfinder Project. On the left is a Mars Exploration Rover Project test rover that is a working sibling to Spirit and Opportunity, which landed on Mars in 2004. On the right is a Mars Science Laboratory test rover the size of that project's Mars rover, Curiosity, which landed on Mars in 2012.
130_Mars/90_Explore_20_Curiosity_2/URL = https://upload.wikimedia.org/wikipedia/commons/4/42/PIA15279_3rovers-stand_D2011_1215_D521.jpg
141_Ceres/License = https://en.wikipedia.org/wiki/File:PIA21906-Ceres-DwarfPlanet-HighResolution-Dawn-20170920.jpg
141_Ceres/Title = Ceres is the largest object in the main asteroid belt that lies between the orbits of Mars and Jupiter. With a diameter of 940 km (580 mi), Ceres is both the largest of the asteroids and the only dwarf planet inside Neptune's orbit. It is the 25th-largest body in the Solar System within the orbit of Neptune
141_Ceres/URL = https://upload.wikimedia.org/wikipedia/commons/thumb/2/25/PIA21906-Ceres-DwarfPlanet-HighResolution-Dawn-20170920.jpg/1024px-PIA21906-Ceres-DwarfPlanet-HighResolution-Dawn-20170920.jpg
141_Ceres/02_CompareEarthMoon/License = https://en.wikipedia.org/wiki/File:Ceres,_Earth_&_Moon_size_comparison.jpg
141_Ceres/02_CompareEarthMoon/Title = Diameter comparison of Ceres, Moon, and Earth.
141_Ceres/02_CompareEarthMoon/URL = https://upload.wikimedia.org/wikipedia/commons/1/12/Ceres,_Earth_&_Moon_size_comparison.jpg
141_Ceres/03_Rotation/License = https://en.wikipedia.org/wiki/File:PIA19547-Ceres-DwarfPlanet-Dawn-RC3-Animation-20150504.gif
141_Ceres/03_Rotation/Title = This animation shows a sequence of images taken by NASA's Dawn spacecraft on May 4, 2015, from a distance of 8,400 miles (13,600 kilometers), in its RC3 mapping orbit. The image resolution is 0.8 mile (1.3 kilometers) per pixel.
141_Ceres/03_Rotation/URL = https://upload.wikimedia.org/wikipedia/commons/0/04/PIA19547-Ceres-DwarfPlanet-Dawn-RC3-Animation-20150504.gif
141_Ceres/05_CompareVestaEros/License = https://en.wikipedia.org/wiki/File:Eros,_Vesta_and_Ceres_size_comparison.jpg
141_Ceres/05_CompareVestaEros/Title = The size comparison of the asteroids are Ceres, Vesta, and Eros.
141_Ceres/05_CompareVestaEros/URL = https://upload.wikimedia.org/wikipedia/commons/9/9b/Eros,_Vesta_and_Ceres_size_comparison.jpg
142_Vesta/License = https://en.wikipedia.org/wiki/File:Vesta_in_natural_color.jpg
142_Vesta/Title = Vesta (minor-planet designation: 4 Vesta) is one of the largest objects in the asteroid belt, with a mean diameter of 525 kilometres (326 mi).0x005B90x005D It was discovered by the German astronomer Heinrich Wilhelm Matthias Olbers on 29 March 18070x005B70x005D and is named after Vesta, the virgin goddess of home and hearth from Roman mythology. Vesta is the second-largest asteroid, both by mass and by volume, after the dwarf planet Ceres.0x005B170x005D0x005B180x005D0x005B190x005D It constitutes an estimated 9% of the mass of the asteroid belt
142_Vesta/URL = https://upload.wikimedia.org/wikipedia/commons/5/51/Vesta_in_natural_color.jpg
142_Vesta/02_CompareCeresMoon/License = https://en.wikipedia.org/wiki/File:Ceres_and_Vesta,_Moon_size_comparison.jpg
142_Vesta/02_CompareCeresMoon/The asteroid (4) Vesta and the dwarf planet (1) Ceres shown alongside the Earth's Moon.
142_Vesta/02_CompareCeresMoon/URL = https://upload.wikimedia.org/wikipedia/commons/f/f9/Ceres_and_Vesta,_Moon_size_comparison.jpg
142_Vesta/03_Rotation/License = https://en.wikipedia.org/wiki/File:Vesta_Rotation.gif
142_Vesta/03_Rotation/Title = A full rotation of the asteroid Vesta as seen from the Dawn spacecraft. Sixty-four images were extracted from the NASA video and animated. Vesta's actual rotation period is 5.342 hours.
142_Vesta/03_Rotation/URL = https://upload.wikimedia.org/wikipedia/commons/f/ff/Vesta_Rotation.gif
142_Vesta/90_Explore_01_Dawn/License = https://en.wikipedia.org/wiki/File:Dawn_spacecraft_model.png
142_Vesta/90_Explore_01_Dawn/Title = Illustration of the Dawn spacecraft. Dawn is the first spacecraft to orbit two extraterrestrial bodies, the first spacecraft to visit either Vesta or Ceres, and the first to orbit a dwarf planet. It was the first NASA exploratory mission to use ion propulsion, which enabled it to enter and leave the orbit of two celestial bodies. Previous multi-target missions using conventional drives, such as the Voyager program, were restricted to flybys.
142_Vesta/90_Explore_01_Dawn/URL = https://upload.wikimedia.org/wikipedia/commons/f/fe/Dawn_spacecraft_model.png
142_Vesta/90_Explore_01_Dawn_2_PriorToLaunch/License = https://en.wikipedia.org/wiki/File:Dawn_at_Launch_Pad.jpg
142_Vesta/90_Explore_01_Dawn_2_PriorToLaunch/Title = NASA's Dawn spacecraft waits for fairing encapsulation in the mobile service tower of Launch Pad 17-B at Cape Canaveral Air Force Station in Florida.
142_Vesta/90_Explore_01_Dawn_2_PriorToLaunch/URL = https://upload.wikimedia.org/wikipedia/commons/9/95/Dawn_at_Launch_Pad.jpg
142_Vesta/90_Explore_01_Dawn_3_Launch/License = https://en.wikipedia.org/wiki/File:Dawn_ignition.jpg
142_Vesta/90_Explore_01_Dawn_3_Launch/Title = Dawn launching on a Delta II rocket from Cape Canaveral Air Force Station Space Launch Complex 17 on September 27, 2007
142_Vesta/90_Explore_01_Dawn_3_Launch/URL = https://upload.wikimedia.org/wikipedia/commons/c/c2/Dawn_ignition.jpg
150_Jupiter/License = https://en.wikipedia.org/wiki/File:PIA22946-Jupiter-RedSpot-JunoSpacecraft-20190212.jpg
150_Jupiter/Title = This striking view of Jupiters Great Red Spot and turbulent southern hemisphere was captured by NASAs Juno spacecraft as it performed a close pass of the gas giant planet.
150_Jupiter/URL = https://upload.wikimedia.org/wikipedia/commons/7/71/PIA22946-Jupiter-RedSpot-JunoSpacecraft-20190212.jpg
150_Jupiter/02_CompareEarth/License = https://en.wikipedia.org/wiki/File:Jupiter,_Earth_size_comparison.jpg
150_Jupiter/02_CompareEarth/Title = Rough visual comparison of Jupiter, Earth, and the Great Red Spot.
150_Jupiter/02_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/c/c2/Jupiter,_Earth_size_comparison.jpg
150_Jupiter/03_Clouds/License = https://en.wikipedia.org/wiki/File:PIA21972_Jupiter_Blues.jpg
150_Jupiter/03_Clouds/Title = Jovian clouds in striking shades of blue in this new view taken by NASA's Juno spacecraft. The Juno spacecraft captured this image when the spacecraft was only 11,747 miles (18,906 kilometers) from the tops of Jupiter's clouds. The higher-altitude clouds can be seen casting shadows on their surroundings. The behavior is most easily observable in the whitest regions in the image, but also in a few isolated spots in both the bottom and right areas of the image.
150_Jupiter/03_Clouds/URL = https://upload.wikimedia.org/wikipedia/commons/5/5c/PIA21972_Jupiter_Blues.jpg
150_Jupiter/04_SouthernStorms/License = https://en.wikipedia.org/wiki/File:PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg
150_Jupiter/04_SouthernStorms/Title = This image shows Jupiter's south pole, as seen by NASA's Juno spacecraft from an altitude of 32,000 miles (52,000 kilometers). The oval features are cyclones, up to 600 miles (1,000 kilometers) in diameter.
150_Jupiter/04_SouthernStorms/URL = https://upload.wikimedia.org/wikipedia/commons/b/b0/PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg
150_Jupiter/05_TimelapseVoyager1/License = https://en.wikipedia.org/wiki/File:790106-0203_Voyager_58M_to_31M_reduced.gif
150_Jupiter/05_TimelapseVoyager1/Title = Jupiter seen by Voyager 1 probe with blue filter. One image was taken every Jupiter day (approximately 10 hours). These pictures were taken from 01/06 to 02/03, 1979 0x003B and Voyager 1 flew from 58 million to 31 million kilometers from Jupiter during that time. The small, round, dark spots appearing in some frames are the shadows cast by the moons passing between Jupiter and the Sun, while the small, white flashes around the planet, are the moons themselves.
150_Jupiter/05_TimelapseVoyager1/URL = https://upload.wikimedia.org/wikipedia/commons/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif
150_Jupiter/79_Moons_Orbiting/License = https://en.wikipedia.org/wiki/File:Jupiter_and_the_Galilean_moons_animation.gif
150_Jupiter/79_Moons_Orbiting/Title = Animation of a sequence of photographs taken by JunoCam aboard the Juno spacecraft, in June 2016, of Jupiter and the motion of the four Galilean moons, as the spacecraft approached the planet.
150_Jupiter/79_Moons_Orbiting/URL = https://upload.wikimedia.org/wikipedia/commons/6/66/Jupiter_and_the_Galilean_moons_animation.gif
150_Jupiter/80_Moons_Europa_1/License = https://en.wikipedia.org/wiki/File:Europa-moon-with-margins.jpg
150_Jupiter/80_Moons_Europa_1/Title = Europa is the smallest of the four Galilean moons orbiting Jupiter, and the sixth-closest to the planet of all the 79 known moons of Jupiter. It is also the sixth-largest moon in the Solar System. Europa was discovered in 1610 by Galileo Galilei and was named after Europa, the Phoenician mother of King Minos of Crete and lover of Zeus (the Greek equivalent of the Roman god Jupiter). Slightly smaller than Earth's Moon, Europa is primarily made of silicate rock and has a water-ice crust and probably an iron0x2013nickel core. It has a very thin atmosphere, composed primarily of oxygen. Its surface is striated by cracks and streaks, but craters are relatively few. 
150_Jupiter/80_Moons_Europa_1/URL = https://upload.wikimedia.org/wikipedia/commons/e/e4/Europa-moon-with-margins.jpg
150_Jupiter/80_Moons_Europa_2_CloseUp/License = https://en.wikipedia.org/wiki/File:Europa_PIA2387x_-_Chaos_Transition,_Crisscrossing_Bands_&_Chaos_Near_Agenor_Linea.jpg
150_Jupiter/80_Moons_Europa_2_CloseUp/Title = The surface of Jupiter's moon Europa features a widely varied landscape, including ridges, bands, small rounded domes and disrupted spaces that geologists called "chaos terrain."
150_Jupiter/80_Moons_Europa_2_CloseUp/URL = https://upload.wikimedia.org/wikipedia/commons/b/b3/Europa_PIA2387x_-_Chaos_Transition,_Crisscrossing_Bands_&_Chaos_Near_Agenor_Linea.jpg
150_Jupiter/80_Moons_Ganymede/License = https://en.wikipedia.org/wiki/File:Ganymede_g1_true-edit1.jpg
150_Jupiter/80_Moons_Ganymede/Title = Ganymede is the largest and most massive of the Solar System's moons. The ninth-largest object in the Solar System, it is the largest without a substantial atmosphere. It has a diameter of 5,268 km (3,273 mi), making it 26% larger than the planet Mercury by volume, although it is only 45% as massive.0x005B160x005D Possessing a metallic core, it has the lowest moment of inertia factor of any solid body in the Solar System and is the only moon known to have a magnetic field.
150_Jupiter/80_Moons_Ganymede/URL = https://upload.wikimedia.org/wikipedia/commons/f/f2/Ganymede_g1_true-edit1.jpg
150_Jupiter/80_Moons_Ganymede_2_CompareEarthMoon/License = https://en.wikipedia.org/wiki/File:Ganymede,_Earth_&_Moon_size_comparison.jpg
150_Jupiter/80_Moons_Ganymede_2_CompareEarthMoon/Title = Diameter comparison of Ganymede, Moon, and Earth.
150_Jupiter/80_Moons_Ganymede_2_CompareEarthMoon/URL = https://upload.wikimedia.org/wikipedia/commons/7/76/Ganymede,_Earth_&_Moon_size_comparison.jpg
150_Jupiter/80_Moons_Ganymede_3_CraterChain/License = https://en.wikipedia.org/wiki/File:Chain_of_impact_craters_on_Ganymede.jpg
150_Jupiter/80_Moons_Ganymede_3_CraterChain/Title = A chain of craters on Ganymede, probably caused by a similar impact event to Shoemaker-Levy crashing into Jupiter. The picture covers an area approximately 190 km (120 mi) across.
150_Jupiter/80_Moons_Ganymede_3_CraterChain/URL = https://upload.wikimedia.org/wikipedia/commons/d/dd/Chain_of_impact_craters_on_Ganymede.jpg
150_Jupiter/80_Moons_Io_1/License = https://en.wikipedia.org/wiki/File:Io_highest_resolution_true_color.jpg
150_Jupiter/80_Moons_Io_1/Title = Io is the innermost and third-largest of the four Galilean moons of the planet Jupiter. It is the fourth-largest moon in the Solar System, has the highest density of all of them, and has the lowest amount of water (by atomic ratio) of any known astronomical object in the Solar System. It was discovered in 1610 by Galileo Galilei and was named after the mythological character Io, a priestess of Hera who became one of Zeus's lovers. With over 400 active volcanoes, Io is the most geologically active object in the Solar System. This extreme geologic activity is the result of tidal heating from friction generated within Io's interior as it is pulled between Jupiter and the other Galilean moons0x2014Europa, Ganymede and Callisto.
150_Jupiter/80_Moons_Io_1/URL = https://upload.wikimedia.org/wikipedia/commons/7/7b/Io_highest_resolution_true_color.jpg
150_Jupiter/80_Moons_Io_2_CompareEarthMoon/License = https://en.wikipedia.org/wiki/File:Io,_Earth_&_Moon_size_comparison.jpg
150_Jupiter/80_Moons_Io_2_CompareEarthMoon/Title = Diameter comparison of Io, Moon, and Earth.
150_Jupiter/80_Moons_Io_2_CompareEarthMoon/URL = https://upload.wikimedia.org/wikipedia/commons/c/cc/Io,_Earth_&_Moon_size_comparison.jpg
150_Jupiter/80_Moons_Io_3_Vulcan/License = https://en.wikipedia.org/wiki/File:Tvastarpic2.jpg
150_Jupiter/80_Moons_Io_3_Vulcan/Title = The detection of very-high-temperature volcanism0x2014hotter than any terrestrial lavas currently erupting0x2014is one of the most spectacular discoveries by the Galileo mission at Io. The images are of an area called Tvashtar and show curtains of lava fountains erupting on the surface. They were taken by the Galileo spacecraft on November 26, 1999. The active region is approximately 25 km (15.5 miles) long and 1 km (0.6 mile) high. The radiant energy emitted from the lava curtain was so intense that it overpowered the camera's detector and it is registered only in white.
150_Jupiter/80_Moons_Io_3_Vulcan/URL = https://upload.wikimedia.org/wikipedia/commons/f/f0/Tvastarpic2.jpg
150_Jupiter/80_Moons_Io_4_VulcanAnimation/License = https://en.wikipedia.org/wiki/File:Tvashtarvideo.gif
150_Jupiter/80_Moons_Io_4_VulcanAnimation/Title = Five-image sequence of New Horizons images showing Io's volcano Tvashtar spewing material 330 km above its surface
150_Jupiter/80_Moons_Io_4_VulcanAnimation/URL = https://upload.wikimedia.org/wikipedia/commons/1/12/Tvashtarvideo.gif
150_Jupiter/90_Explore_40_Galileo/License = https://en.wikipedia.org/wiki/File:Galileo_Preparations_-_GPN-2000-000672.jpg
150_Jupiter/90_Explore_40_Galileo/Title = In the Vertical Processing Facility (VPF), Galileo is prepared for mating with the Inertial Upper Stage booster.
150_Jupiter/90_Explore_40_Galileo/URL = https://upload.wikimedia.org/wikipedia/commons/1/1d/Galileo_Preparations_-_GPN-2000-000672.jpg
150_Jupiter/90_Explore_50_Juno/License = https://en.wikipedia.org/wiki/File:Juno's_high-gain_antenna_just_before_installation.jpg
150_Jupiter/90_Explore_50_Juno/Title = Juno's high-gain antenna dish being installed
150_Jupiter/90_Explore_50_Juno/URL = https://upload.wikimedia.org/wikipedia/commons/c/c2/Juno's_high-gain_antenna_just_before_installation.jpg
160_Saturn/License = https://en.wikipedia.org/wiki/File:Saturn_during_Equinox.jpg
160_Saturn/Title = This captivating natural color view of the planet Saturn was created from images collected shortly after Cassini began its extended Equinox Mission in July 2008. Six moons complete this constructed panorama: Titan (5,150 kilometers across), Janus (179 kilometers across), Mimas (396 kilometers across), Pandora (81 kilometers across), Epimetheus (113 kilometers across) and Enceladus (504 kilometers across).
160_Saturn/URL = https://upload.wikimedia.org/wikipedia/commons/c/c7/Saturn_during_Equinox.jpg
160_Saturn/02_CompareEarth/License = https://en.wikipedia.org/wiki/File:Saturn,_Earth_size_comparison2.jpg
160_Saturn/02_CompareEarth/Title = Rough comparison of sizes of Saturn and Earth.
160_Saturn/02_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/e/e0/Saturn,_Earth_size_comparison2.jpg
160_Saturn/03_Rings/License = https://en.wikipedia.org/wiki/File:Saturn_from_Cassini_Orbiter_(2007-01-19).jpg
160_Saturn/03_Rings/Title = The rings of Saturn (imaged here by Cassini in 2007) are the most massive and conspicuous in the Solar System.
160_Saturn/03_Rings/URL = https://upload.wikimedia.org/wikipedia/commons/4/47/Saturn_from_Cassini_Orbiter_(2007-01-19).jpg
160_Saturn/04_Eclipse/License = https://en.wikipedia.org/wiki/File:Saturn_eclipse.jpg
160_Saturn/04_Eclipse/Title = Eclipse of the Sun by Saturn. The distant Earth is visible as a dot above the left extremity of the main set of rings.
160_Saturn/04_Eclipse/URL = https://upload.wikimedia.org/wikipedia/commons/b/ba/Saturn_eclipse.jpg
160_Saturn/80_Moon_Enceladus/License = https://en.wikipedia.org/wiki/File:PIA17202_-_Approaching_Enceladus.jpg
160_Saturn/80_Moon_Enceladus/Title = Enceladus is the sixth-largest moon of Saturn. It is about 500 kilometers (310 mi) in diameter, about a tenth of that of Saturn's largest moon, Titan. Enceladus is mostly covered by fresh, clean ice, making it one of the most reflective bodies of the Solar System. Consequently, its surface temperature at noon only reaches 0x2212198 0x00B0C (0x2212324 0x00B0F), far colder than a light-absorbing body would be. Despite its small size, Enceladus has a wide range of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrains. Several robotic missions have been proposed to further explore Enceladus and assess its habitability
160_Saturn/80_Moon_Enceladus/URL = https://upload.wikimedia.org/wikipedia/commons/8/83/PIA17202_-_Approaching_Enceladus.jpg
160_Saturn/80_Moon_Pan_1/License = https://en.wikipedia.org/wiki/File:PIA21436.jpg
160_Saturn/80_Moon_Pan_1/Title = Pan is the innermost named moon of Saturn. It is a small, walnut-shaped moon approximately 35 kilometres across and 23 km wide that orbits within the Encke Gap in Saturn's A Ring. Pan is a ring shepherd and is responsible for keeping the Encke Gap free of ring particles. It is sometimes described as having the appearance of a raviolo.
160_Saturn/80_Moon_Pan_1/URL = https://upload.wikimedia.org/wikipedia/commons/b/b5/PIA21436.jpg
160_Saturn/80_Moon_Pan_3_Highway/License = https://en.wikipedia.org/wiki/File:Pans_highway_3-05-07.jpg
160_Saturn/80_Moon_Pan_3_Highway/Title = Cassini image showing Pan orbiting in the Encke Gap.
160_Saturn/80_Moon_Pan_3_Highway/URL = https://upload.wikimedia.org/wikipedia/commons/5/57/Pans_highway_3-05-07.jpg
160_Saturn/80_Moon_Phoebe/License = https://en.wikipedia.org/wiki/File:Phoebe_cassini.jpg
160_Saturn/80_Moon_Phoebe/Title = Phoebe is roughly spherical and has a differentiated interior. It was spherical and hot early in its history and was battered out of roundness by repeated impacts. It is believed to be a captured centaur that originated in the Kuiper belt. Phoebe is the second largest retrograde satellite in the solar system after Triton.
160_Saturn/80_Moon_Phoebe/URL = https://upload.wikimedia.org/wikipedia/commons/3/32/Phoebe_cassini.jpg
160_Saturn/80_Moon_Titan_1/License = https://en.wikipedia.org/wiki/File:Titan_in_true_color.jpg
160_Saturn/80_Moon_Titan_1/Title = Titan is the largest moon of Saturn and the second-largest natural satellite in the Solar System. It is the only moon known to have a dense atmosphere, and the only known body in space, other than Earth, where clear evidence of stable bodies of surface liquid has been found. Titan is 50% larger (in diameter) than Earth's moon and 80% more massive. It is the second-largest moon in the Solar System after Jupiter's moon Ganymede, and is larger than the planet Mercury, but only 40% as massive.
160_Saturn/80_Moon_Titan_1/URL = https://upload.wikimedia.org/wikipedia/commons/4/45/Titan_in_true_color.jpg
160_Saturn/80_Moon_Titan_2_Surface/License = https://en.wikipedia.org/wiki/File:Huygens_surface_color_sr.jpg
160_Saturn/80_Moon_Titan_2_Surface/Title = The color x2 super-resolution image of the Titan's surface as seen by the Huygens probe.
160_Saturn/80_Moon_Titan_2_Surface/URL = https://upload.wikimedia.org/wikipedia/commons/7/70/Huygens_surface_color_sr.jpg
160_Saturn/90_Explore_3_CassiniHuygens_1/License = https://en.wikipedia.org/wiki/File:Cassini_Saturn_Orbit_Insertion.jpg
160_Saturn/90_Explore_3_CassiniHuygens_1/Title = This is an artists concept of Cassini during the Saturn Orbit Insertion (SOI) maneuver, just after the main engine has begun firing. Cassini's close proximity to the planet after the maneuver offers a unique opportunity to observe Saturn and its rings at extremely high resolution.
160_Saturn/90_Explore_3_CassiniHuygens_1/URL = https://upload.wikimedia.org/wikipedia/commons/b/b2/Cassini_Saturn_Orbit_Insertion.jpg
160_Saturn/90_Explore_3_CassiniHuygens_2_Huygens/License = https://en.wikipedia.org/wiki/File:Huygens_probe_dsc03686.jpg
160_Saturn/90_Explore_3_CassiniHuygens_2_Huygens/Title = The Huygens probe0x003B scale 1 facsimile. A full-size replica of the probe, 1.3 metres (4.3 feet) across
160_Saturn/90_Explore_3_CassiniHuygens_2_Huygens/URL = https://upload.wikimedia.org/wikipedia/commons/c/ca/Huygens_probe_dsc03686.jpg
160_Saturn/90_Explore_3_CassiniHuygens_3_Assembly/License = https://en.wikipedia.org/wiki/File:Cassini-Huygens_is_installed_to_the_payload_adapter.jpg
160_Saturn/90_Explore_3_CassiniHuygens_3_Assembly/Title = Flight mechanics from NASA0x2019s Jet Propulsion Laboratory (JPL) in Pasadena, Calif., lower the Cassini spacecraft onto its launch vehicle adapter in KSC0x2019s Payload Hazardous Servicing Facility. The adapter will later be mated to a Titan IV/Centaur expendable launch vehicle that will lift Cassini into space.
160_Saturn/90_Explore_3_CassiniHuygens_3_Assembly/URL = https://upload.wikimedia.org/wikipedia/commons/6/68/Cassini-Huygens_is_installed_to_the_payload_adapter.jpg
160_Saturn/90_Explore_3_CassiniHuygens_4_LaunchPad/License = https://en.wikipedia.org/wiki/File:Titan4B_on_Launch_Complex_40.jpg
160_Saturn/90_Explore_3_CassiniHuygens_4_LaunchPad/Title = The second Titan IVB/Centaur (Model 401), with Cassini/Huygens on board. At Launch Complex 40 on Cape Canaveral Air Station, the Mobile Service Tower has been retracted away from the Titan IVB/Centaur carrying the Cassini spacecraft.
160_Saturn/90_Explore_3_CassiniHuygens_4_LaunchPad/URL = https://upload.wikimedia.org/wikipedia/commons/8/82/Titan4B_on_Launch_Complex_40.jpg
170_Uranus/License = https://en.wikipedia.org/wiki/File:Uranus_clouds.jpg
170_Uranus/Title = Uranus is the seventh planet from the Sun. Its name is a reference to the Greek god of the sky, Uranus, who, according to Greek mythology, was the grandfather of Zeus (Jupiter) and father of Cronus (Saturn). It has the third-largest planetary radius and fourth-largest planetary mass in the Solar System. Uranus is similar in composition to Neptune, and both have bulk chemical compositions which differ from that of the larger gas giants Jupiter and Saturn. For this reason, scientists often classify Uranus and Neptune as "ice giants" to distinguish them from the other gas giants. The Uranian axis of rotation is approximately parallel with the plane of the Solar System, with an axial tilt of 97.770x00B0 (as defined by prograde rotation). This gives it seasonal changes completely unlike those of the other planets. Near the solstice, one pole faces the Sun continuously and the other faces away. Only a narrow strip around the equator experiences a rapid day0x2013night cycle, but with the Sun low over the horizon. At the other side of Uranus's orbit the orientation of the poles towards the Sun is reversed. Each pole gets around 42 years of continuous sunlight, followed by 42 years of darkness. Image of Uranus obtained in 2005 by ACS on HST. Rings, southern collar and a bright cloud in the northern hemisphere are visible.
170_Uranus/URL = https://upload.wikimedia.org/wikipedia/commons/0/0e/Uranus_clouds.jpg
170_Uranus/02_CompareEarth/License = https://en.wikipedia.org/wiki/File:Uranus,_Earth_size_comparison_2.jpg
170_Uranus/02_CompareEarth/Title = Diameter comparison of Uranus and Earth
170_Uranus/02_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/9/95/Uranus,_Earth_size_comparison_2.jpg
170_Uranus/04_Aurorae/License = https://en.wikipedia.org/wiki/File:Alien_aurorae_on_Uranus.jpg
170_Uranus/04_Aurorae/Title = Ever since Voyager 2 beamed home spectacular images of the planets in the 1980s, planet-lovers have been hooked on extra-terrestrial aurorae. In 2011, the NASA/ESA Hubble Space Telescope became the first Earth-based telescope to snap an image of the aurorae on Uranus. These pictures are form 2017.
170_Uranus/04_Aurorae/URL = https://upload.wikimedia.org/wikipedia/commons/8/86/Alien_aurorae_on_Uranus.jpg
170_Uranus/05_Aurorae/License = https://en.wikipedia.org/wiki/File:Uranuslight.jpg
170_Uranus/05_Aurorae/Title = Uranus's aurorae against its equatorial rings, imaged by the Hubble telescope. Unlike the aurorae of Earth and Jupiter, those of Uranus are not in line with its poles, due to its lopsided magnetic field.
170_Uranus/05_Aurorae/URL = https://upload.wikimedia.org/wikipedia/commons/2/2e/Uranuslight.jpg
170_Uranus/80_Moons_Miranda_1/License = https://en.wikipedia.org/wiki/File:PIA18185_Miranda's_Icy_Face.jpg
170_Uranus/80_Moons_Miranda_1/Title = Miranda, also designated Uranus V, is the smallest and innermost of Uranus's five round satellites. It is named after Miranda from William Shakespeare's play The Tempest. Like the other large moons of Uranus, Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus' extreme seasonal cycle. At just 470 km in diameter, Miranda is one of the smallest closely observed objects in the Solar System that might be in hydrostatic equilibrium (spherical under its own gravity).
170_Uranus/80_Moons_Miranda_1/URL = https://upload.wikimedia.org/wikipedia/commons/e/e1/PIA18185_Miranda's_Icy_Face.jpg
170_Uranus/80_Moons_Miranda_2_Close/License = https://en.wikipedia.org/wiki/File:Miranda_elsinorinverness.jpg
170_Uranus/80_Moons_Miranda_2_Close/Title = The fault scarps around Elsinore (top right) and the chevrons of Inverness Corona (bottom left). Miranda has one of the most extreme and varied topographies of any object in the Solar System, including Verona Rupes, a 20-kilometer-high scarp that is the highest cliff in the Solar System.
170_Uranus/80_Moons_Miranda_2_Close/URL = https://upload.wikimedia.org/wikipedia/en/3/33/Miranda_elsinorinverness.jpg
180_Neptun/License = https://en.wikipedia.org/wiki/File:Neptune_-_Voyager_2_(29347980845)_flatten_crop.jpg
180_Neptun/Title = Neptune is the eighth and farthest-known Solar planet from the Sun. In the Solar System, it is the fourth-largest planet by diameter, the third-most-massive planet, and the densest giant planet. It is 17 times the mass of Earth, slightly more massive than its near-twin Uranus.
180_Neptun/URL = https://upload.wikimedia.org/wikipedia/commons/6/63/Neptune_-_Voyager_2_(29347980845)_flatten_crop.jpg
180_Neptun/02_CompareEarth/License = https://en.wikipedia.org/wiki/File:Neptune,_Earth_size_comparison_2b.jpg
180_Neptun/02_CompareEarth/Title = Diameter comparison of Neptune and Earth.
180_Neptun/02_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/7/78/Neptune,_Earth_size_comparison_2b.jpg
180_Neptun/03_Clouds/License = https://en.wikipedia.org/wiki/File:Neptune_clouds.jpg
180_Neptun/03_Clouds/Title = Bands of high-altitude clouds cast shadows on Neptune's lower cloud deck. The bright sides of the clouds which face the Sun are brighter than the surrounding cloud deck because they are more directly exposed to the sun. Shadows can be seen on the side opposite the sun.
180_Neptun/03_Clouds/URL = https://upload.wikimedia.org/wikipedia/commons/c/c8/Neptune_clouds.jpg
180_Neptun/04_Storms/License = https://en.wikipedia.org/wiki/File:Neptune_storms.jpg
180_Neptun/04_Storms/Title = The Great Dark Spot (top), Scooter (middle white cloud),0x005B800x005D and the Small Dark Spot (bottom), with contrast exaggerated.
180_Neptun/04_Storms/URL = https://upload.wikimedia.org/wikipedia/commons/8/8c/Neptune_storms.jpg
180_Neptun/80_Moons_Triton/License = https://en.wikipedia.org/wiki/File:Triton_moon_mosaic_Voyager_2_(large).jpg
180_Neptun/80_Moons_Triton/Title = Global color mosaic of Triton, taken in 1989 by Voyager 2 during its flyby of the Neptune system. Color was synthesized by combining high-resolution images taken through orange, violet, and ultraviolet filters0x003B these images were displayed as red, green, and blue images and combined to create this color version. With a radius of 1,350 km (839 mi), about 22% smaller than Earth's moon, Triton is by far the largest satellite of Neptune. It is one of only three objects in the Solar System known to have a nitrogen-dominated atmosphere (the others are Earth and Saturn's giant moon, Titan).
180_Neptun/80_Moons_Triton/URL = https://upload.wikimedia.org/wikipedia/commons/a/a6/Triton_moon_mosaic_Voyager_2_(large).jpg
180_Neptun/80_Moons_Triton_2_CompareEarthMoon/License = https://en.wikipedia.org/wiki/File:Triton,_Earth_&_Moon_size_comparison.jpg
180_Neptun/80_Moons_Triton_2_CompareEarthMoon/Title = Diameter comparison of Triton, Moon, and Earth.
180_Neptun/80_Moons_Triton_2_CompareEarthMoon/URL = https://upload.wikimedia.org/wikipedia/commons/2/2b/Triton,_Earth_&_Moon_size_comparison.jpg
180_Neptun/80_Moons_Triton_3_Rotation/License = https://en.wikipedia.org/wiki/File:Triton_Rotation_Movie.gif
180_Neptun/80_Moons_Triton_3_Rotation/Title = This movie of rotating Triton from Voyager 2 spacecraft.
180_Neptun/80_Moons_Triton_3_Rotation/URL = https://upload.wikimedia.org/wikipedia/commons/f/f3/Triton_Rotation_Movie.gif
180_Neptun/80_Moons_Triton_4_South/License = https://en.wikipedia.org/wiki/File:Triton_(moon).jpg
180_Neptun/80_Moons_Triton_4_South/Title = Voyager 2 image showing the southern hemisphere of Triton. This image was made using about a dozen Voyager 2 frames. The large, pinkish colored south polar cap is at the top of the image. North of the cap the surface is generally darker and redder in color. This area exhibits a plethora of unusual morphologic features, including the long lineations at the center of the frame.
180_Neptun/80_Moons_Triton_4_South/URL = https://upload.wikimedia.org/wikipedia/commons/9/91/Triton_(moon).jpg
180_Neptun/90_Explore_1_Voyager2_1/License = https://en.wikipedia.org/wiki/File:Voyager_spacecraft_model.png
180_Neptun/90_Explore_1_Voyager2_1/Title = Artist's rendering, from NASA, of the design employed by the twin Voyager 1 and Voyager 2 spacecraft, in mission configuration. Sent into the outer solar system for the purpose of embarking on the "grand tour" of the Gas giants, Voyager 1 made successful reconnaissance flybys of the planet Jupiter and Saturn in 1979 and 1980. Voyager 2 also performed flybys of Jupiter and Saturn in 1979 and 1981, along with the very first, and so far only, visits of the planets Uranus and Neptune in 1986 and 1989.
180_Neptun/90_Explore_1_Voyager2_1/URL = https://upload.wikimedia.org/wikipedia/commons/6/60/Voyager_spacecraft_model.png
180_Neptun/90_Explore_1_Voyager2_2_Testing/License = https://en.wikipedia.org/wiki/File:Voyager_Testing_1976_PIA21732.jpg
180_Neptun/90_Explore_1_Voyager2_2_Testing/Title = Voyager in transport to a solar thermal test chamber.
180_Neptun/90_Explore_1_Voyager2_2_Testing/URL = https://upload.wikimedia.org/wikipedia/commons/thumb/2/21/Voyager_Testing_1976_PIA21732.jpg/1007px-Voyager_Testing_1976_PIA21732.jpg
180_Neptun/90_Explore_1_Voyager2_3_Launch/License = https://en.wikipedia.org/wiki/File:Titan_3E_Centaur_launches_Voyager_2.jpg
180_Neptun/90_Explore_1_Voyager2_3_Launch/Title = The Voyager 2 aboard Titan III-Centaur launch vehicle lifted off on August 20, 1977.
180_Neptun/90_Explore_1_Voyager2_3_Launch/URL = https://upload.wikimedia.org/wikipedia/commons/a/a4/Titan_3E_Centaur_launches_Voyager_2.jpg
200_Pluto/License = https://en.wikipedia.org/wiki/File:Pluto_in_True_Color_-_High-Res.jpg
200_Pluto/Title = Pluto is a dwarf planet in the Kuiper belt, a ring of bodies beyond the orbit of Neptune. It was the first and the largest Kuiper belt object to be discovered. After Pluto was discovered in 1930 it was declared to be the ninth planet from the Sun. Beginning in the 1990s, its status as a planet was questioned following the discovery of several objects of similar size in the Kuiper belt, including the dwarf planet Eris. This led the International Astronomical Union (IAU) in 2006 to formally define the term "planet" 0x2014 excluding Pluto and reclassifying it as a dwarf planet.
200_Pluto/URL = https://upload.wikimedia.org/wikipedia/commons/e/ef/Pluto_in_True_Color_-_High-Res.jpg
200_Pluto/02_CompareToLots/License = https://en.wikipedia.org/wiki/File:Pluto_compared2.jpg
200_Pluto/02_CompareToLots/Title = Pluto (bottom right) compared in size to the largest satellites in the solar system (from left to right and top to bottom): Ganymede, Titan, Callisto, Io, the Moon, Europa, and Triton
200_Pluto/02_CompareToLots/URL = https://upload.wikimedia.org/wikipedia/commons/2/23/Pluto_compared2.jpg
200_Pluto/03_RotationWithCharon/License = https://en.wikipedia.org/wiki/File:Pluto-Charon_system-new.gif
200_Pluto/03_RotationWithCharon/Title = An oblique view of the Pluto0x2013Charon system showing that Pluto orbits a point outside itself. The two bodies are mutually tidally locked. 6.387 day revolution shown 1 second/day.
200_Pluto/03_RotationWithCharon/URL = https://upload.wikimedia.org/wikipedia/commons/2/2f/Pluto-Charon_system-new.gif
200_Pluto/04_Snakeskin/License = https://en.wikipedia.org/wiki/File:Snakeskin_terrain_on_Pluto_(PIA19957).png
200_Pluto/04_Snakeskin/Title = Patterns of blue-gray ridges and reddish material observed in the Tartarus Dorsa region on July 14, 2015
200_Pluto/04_Snakeskin/URL = https://upload.wikimedia.org/wikipedia/commons/7/79/Snakeskin_terrain_on_Pluto_(PIA19957).png
200_Pluto/05_ByeBye/License = https://en.wikipedia.org/wiki/File:Blue_hazes_over_backlit_Pluto.jpg
200_Pluto/05_ByeBye/Title = View of Pluto as New Horizons left the system, catching the Sun's rays passing through Pluto's atmosphere, forming a ring.
200_Pluto/05_ByeBye/URL = https://upload.wikimedia.org/wikipedia/commons/0/02/Blue_hazes_over_backlit_Pluto.jpg
200_Pluto/80_Moons_Charon/License = https://en.wikipedia.org/wiki/File:Charon_in_True_Color_-_High-Res.jpg
200_Pluto/80_Moons_Charon/Title = Charon is the largest of the five known natural satellites of the dwarf planet Pluto. It has a mean radius of 606 km (377 mi). Charon is the sixth-largest trans-Neptunian object after Pluto, Eris, Haumea, Makemake and Gonggong. With half the diameter and one eighth the mass of Pluto, Charon is a very large moon in comparison to its parent body. Its gravitational influence is such that the barycenter of the Plutonian system lies outside Pluto.
200_Pluto/80_Moons_Charon/URL = https://upload.wikimedia.org/wikipedia/commons/2/2e/Charon_in_True_Color_-_High-Res.jpg
200_Pluto/90_Explore_1_NewHorizons/License = https://en.wikipedia.org/wiki/File:New_Horizons_spacecraft_model_1.png
200_Pluto/90_Explore_1_NewHorizons/Title = New Horizons is an interplanetary space probe that was launched as a part of NASA's New Frontiers program. Engineered by the Johns Hopkins University Applied Physics Laboratory (APL) and the Southwest Research Institute (SwRI), with a team led by S. Alan Stern, the spacecraft was launched in 2006 with the primary mission to perform a flyby study of the Pluto system in 2015, and a secondary mission to fly by and study one or more other Kuiper belt objects (KBOs) in the decade to follow, which became a mission to 486958 Arrokoth. It is the fifth space probe to achieve the escape velocity needed to leave the Solar System.
200_Pluto/90_Explore_1_NewHorizons/URL = https://upload.wikimedia.org/wikipedia/commons/e/ee/New_Horizons_spacecraft_model_1.png
200_Pluto/90_Explore_1_NewHorizons_2_InFactory/License = https://en.wikipedia.org/wiki/File:New_Horizons_1.jpg
200_Pluto/90_Explore_1_NewHorizons_2_InFactory/Title = New Horizons in a factory at Kennedy Space Center in 2005
200_Pluto/90_Explore_1_NewHorizons_2_InFactory/URL = https://upload.wikimedia.org/wikipedia/commons/4/46/New_Horizons_1.jpg
200_Pluto/90_Explore_1_NewHorizons_3_Launch/License = https://en.wikipedia.org/wiki/File:Atlas_V_551_roars_into_blue_sky.jpg
200_Pluto/90_Explore_1_NewHorizons_3_Launch/Title = NASA0x2019s New Horizons spacecraft roars into the blue sky aboard an Atlas V rocket spewing flames and smoke.
200_Pluto/90_Explore_1_NewHorizons_3_Launch/URL = https://upload.wikimedia.org/wikipedia/commons/3/32/Atlas_V_551_roars_into_blue_sky.jpg
210_Arrokoth/License = https://en.wikipedia.org/wiki/File:UltimaThule_CA06_color_vertical_(rotated).png
210_Arrokoth/Title = 486958 Arrokoth is a trans-Neptunian object located in the Kuiper belt. It is a contact binary 36 km (22 mi) long, composed of two planetesimals 21 km (13 mi) and 15 km (9 mi) across, that are joined along their major axes. The larger lobe, which is flatter than smaller lobe, appears to be an aggregate of 8 or so smaller units, each approximately 5 km (3 mi) across, that fused together before they came into contact. Because there have been few to no disruptive impacts on Arrokoth since it formed, the details of its formation have been preserved. With the New Horizons space probe's flyby at 05:33 on 1 January 2019 (UTC time), Arrokoth became the farthest and most primitive object in the Solar System visited by a spacecraft. At the time of the New Horizons flyby, the object had been nicknamed Ultima Thule.
210_Arrokoth/URL = https://upload.wikimedia.org/wikipedia/commons/0/09/UltimaThule_CA06_color_vertical_(rotated).png
210_Arrokoth/02_Stereoscopic/License = https://en.wikipedia.org/wiki/File:MU69_simulated_3D.gif
210_Arrokoth/02_Stereoscopic/Title = A 3-D animation created by blending two images
210_Arrokoth/02_Stereoscopic/URL = https://upload.wikimedia.org/wikipedia/en/3/3d/MU69_simulated_3D.gif
210_Arrokoth/03_Flyby/License = https://en.wikipedia.org/wiki/File:Ultima_Thule_Departure_movie.gif
210_Arrokoth/03_Flyby/Title = Mission scientists created this "departure movie" from 14 different images taken by the New Horizons Long Range Reconnaissance Imager (LORRI) shortly after the spacecraft flew past the Kuiper Belt object nicknamed Ultima Thule (officially named 2014 MU69) on Jan. 1, 2019.  This is the farthest movie of any object in our Solar System ever made by any spacecraft. 
210_Arrokoth/03_Flyby/URL = https://upload.wikimedia.org/wikipedia/commons/1/15/Ultima_Thule_Departure_movie.gif
300_ChuryumovGerasimenko/License = https://en.wikipedia.org/wiki/File:Comet_67P_on_19_September_2014_NavCam_mosaic.jpg
300_ChuryumovGerasimenko/Title = 7P/Churyumov0x2013Gerasimenko is a Jupiter-family comet, originally from the Kuiper belt, with a current orbital period of 6.45 years, a rotation period of approximately 12.4 hours and a maximum velocity of 135,000 km/h (38 km/s0x003B 84,000 mph). Churyumov0x2013Gerasimenko is approximately 4.3 by 4.1 km at its longest and widest dimensions. It was first observed on photographic plates in 1969 by Soviet astronomers Klim Ivanovych Churyumov and Svetlana Ivanovna Gerasimenko, after whom it is named. 
300_ChuryumovGerasimenko/URL = https://upload.wikimedia.org/wikipedia/commons/8/81/Comet_67P_on_19_September_2014_NavCam_mosaic.jpg
300_ChuryumovGerasimenko/02_WeatherAnimation/License = https://en.wikipedia.org/wiki/File:67P_Churyumov-Gerasimenko_surface.gif
300_ChuryumovGerasimenko/02_WeatherAnimation/Title = Dust and cosmic rays on the surface of the comet in 2016, with stars moving in the background. Filmed by Rosetta's OSIRIS instrument.
300_ChuryumovGerasimenko/02_WeatherAnimation/URL = https://upload.wikimedia.org/wikipedia/commons/0/01/67P_Churyumov-Gerasimenko_surface.gif
300_ChuryumovGerasimenko/03_ApproachAnimation/License = https://en.wikipedia.org/wiki/File:NavCam_Comet_67P_animation_20140806_(cropped).gif
300_ChuryumovGerasimenko/03_ApproachAnimation/Title = This animation consists of 86 images acquired by Rosetta's NavCam as it approached 67P in August 2014.
300_ChuryumovGerasimenko/03_ApproachAnimation/URL = https://upload.wikimedia.org/wikipedia/commons/d/da/NavCam_Comet_67P_animation_20140806_(cropped).gif
300_ChuryumovGerasimenko/04/License = https://en.wikipedia.org/wiki/File:67P-C-G_-_May_2_2015_(32730086746).jpg
300_ChuryumovGerasimenko/04/Title = As seen by Rosetta on 2 May 2015
300_ChuryumovGerasimenko/04/URL = https://upload.wikimedia.org/wikipedia/commons/5/59/67P-C-G_-_May_2_2015_(32730086746).jpg
300_ChuryumovGerasimenko/05/License = https://en.wikipedia.org/wiki/File:67P-C-G_-_March_28_2015_(32370930490).jpg
300_ChuryumovGerasimenko/05/Title = Assembled using two version of the same image. One with minimal lightening for the comet nucleus, the other heavily lightened for the jets. Image taken using the OSIRIS instrument aboard the ESA's Rosetta spacecraft.
300_ChuryumovGerasimenko/05/URL = https://upload.wikimedia.org/wikipedia/commons/1/12/67P-C-G_-_March_28_2015_(32370930490).jpg
300_ChuryumovGerasimenko/06_CloseUp/License = https://en.wikipedia.org/wiki/File:Cliffs_of_Comet_67P.jpg
300_ChuryumovGerasimenko/06_CloseUp/Title = Image showing ragged cliffs, 10 December 2014
300_ChuryumovGerasimenko/06_CloseUp/URL = https://upload.wikimedia.org/wikipedia/commons/4/46/Cliffs_of_Comet_67P.jpg
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_1/License = https://en.wikipedia.org/wiki/File:Rosetta_spacecraft_model.png
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_1/Title = Churyumov0x2013Gerasimenko was the destination of the European Space Agency's Rosetta mission, launched on 2 March 2004. Rosetta rendezvoused with Churyumov0x2013Gerasimenko on 6 August 2014 and entered orbit on 10 September 2014. Rosetta's lander, Philae, landed on the comet's surface on 12 November 2014, becoming the first spacecraft to land on a comet nucleus. On 30 September 2016, the Rosetta spacecraft ended its mission by landing on the comet in its Ma'at region.
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_1/URL = https://upload.wikimedia.org/wikipedia/commons/9/9a/Rosetta_spacecraft_model.png
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_2_SelfieAtMars/License = https://en.wikipedia.org/wiki/File:Rosetta0x2019s_self-portrait_at_Mars_(12743274474).jpg
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_2_SelfieAtMars/Title = On 25 February 2007 at 02:15 GMT, Rosetta passed just 250 km from the surface of Mars. Rosetta0x2019s Philae lander took this image 4 minutes before closest approach, at a distance of 1000 km. It captures one of Rosetta0x2019s 14 m-long solar wings, set against the northern hemisphere of Mars, where details in the Mawrth Vallis region can be seen.
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_2_SelfieAtMars/URL = https://upload.wikimedia.org/wikipedia/commons/e/e2/Rosetta0x2019s_self-portrait_at_Mars_(12743274474).jpg
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_3_Philae/License = https://en.wikipedia.org/wiki/File:Philae_lander_(transparent_bg).png
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_3_Philae/Title = Philae is a robotic European Space Agency lander that accompanied the Rosetta spacecraft until it separated to land on comet 67P/Churyumov0x2013Gerasimenko, ten years and eight months after departing Earth. On 12 November 2014, Philae touched down on the comet, but it bounced when its anchoring harpoons failed to deploy and a thruster designed to hold the probe to the surface did not fire. After bouncing off the surface twice, Philae achieved the first-ever "soft" (nondestructive) landing on a comet nucleus, although the lander's final, uncontrolled touchdown left it in a non-optimal location and orientation. Despite the landing problems, the probe's instruments obtained the first images from a comet's surface.
300_ChuryumovGerasimenko/90_Explore_1_Rosetta_3_Philae/URL = https://upload.wikimedia.org/wikipedia/commons/9/95/Philae_lander_(transparent_bg).png
310_Tempel1/License = https://en.wikipedia.org/wiki/File:PIA02142_Tempel_1_bottom_sharped.jpg
310_Tempel1/Title = Tempel 1 is a periodic Jupiter-family comet discovered by Wilhelm Tempel in 1867. It completes an orbit of the Sun every 5.5 years. Tempel 1 was the target of the Deep Impact space mission, which photographed a deliberate high-speed impact upon the comet in 2005. It was re-visited by the Stardust spacecraft on February 14, 2011 and came back to perihelion in August 2016.
310_Tempel1/URL = https://upload.wikimedia.org/wikipedia/commons/5/5d/PIA02142_Tempel_1_bottom_sharped.jpg
310_Tempel1/02_DeepImpact/License = https://en.wikipedia.org/wiki/File:Deep_Impact_HRI.jpeg
310_Tempel1/02_DeepImpact/Title = Comet Tempel 1 67 seconds after it collided with Deep Impact, taken by the high-resolution camera on the flyby spacecraft. The image reveals ridges, scalloped edges and possibly impact craters formed long ago.
310_Tempel1/02_DeepImpact/URL = https://upload.wikimedia.org/wikipedia/commons/3/3e/Deep_Impact_HRI.jpeg
310_Tempel1/03_DeepImpact_Animation/License = https://en.wikipedia.org/wiki/File:HRIV_Impact.gif
310_Tempel1/03_DeepImpact_Animation/Title = Flyby spacecraft Deep Impact shows the flash that occurred when comet Tempel 1 ran over the spacecraft's impactor probe. It was taken by the flyby craft's High Resolution Instrument, Visual CCD camera (HRIV) over a period of about 40 seconds. Black borders are the result of image stabilization.
310_Tempel1/03_DeepImpact_Animation/URL = https://upload.wikimedia.org/wikipedia/commons/4/43/HRIV_Impact.gif
310_Tempel1/04_DeepImpact_Animation/License = https://en.wikipedia.org/wiki/File:ITS_Impact.gif
310_Tempel1/04_DeepImpact_Animation/Title = Image sequence from the Impactor Targeting Sensor, Visual CCD (ITS) during encounter. Images begin at 1024x1024 and drop to 64x64 just before impact. Images resized and stabilized for easier viewing.
310_Tempel1/04_DeepImpact_Animation/URL = https://upload.wikimedia.org/wikipedia/commons/9/99/ITS_Impact.gif
310_Tempel1/90_Explore_1_DeepImpact_1/License = https://en.wikipedia.org/wiki/File:Deep_Impact.jpg
310_Tempel1/90_Explore_1_DeepImpact_1/Title = Computer rendering of the Deep Impact space probe after separation of the impactor.
310_Tempel1/90_Explore_1_DeepImpact_1/URL = https://upload.wikimedia.org/wikipedia/commons/3/3d/Deep_Impact.jpg
310_Tempel1/90_Explore_1_DeepImpact_2_Launch/License = https://en.wikipedia.org/wiki/File:Delta_II_7925_(2925)_rocket_with_Deep_Impact.jpg
310_Tempel1/90_Explore_1_DeepImpact_2_Launch/Title = The sun rises behind Launch Pad 17-B, Cape Canaveral Air Force Station, Fla., where the Boeing Delta II rocket carrying the Deep Impact spacecraft waits for launch.
310_Tempel1/90_Explore_1_DeepImpact_2_Launch/URL = https://upload.wikimedia.org/wikipedia/commons/9/94/Delta_II_7925_(2925)_rocket_with_Deep_Impact.jpg
320_Hartley/License = https://en.wikipedia.org/wiki/File:Comet_Hartley_2.jpg
320_Hartley/Title = Comet Hartley 2, designated as 103P/Hartley by the Minor Planet Center, is a small periodic comet with an orbital period of 6.46 years. It was discovered by Malcolm Hartley in 1986 at the Schmidt Telescope Unit, Siding Spring Observatory, Australia. Its diameter is estimated to be 1.2 to 1.6 kilometres. Hartley 2 was the target of a flyby of the Deep Impact spacecraft, as part of the EPOXI mission, on 4 November 2010,0x005B70x005D which was able to approach within 700 kilometers (430 mi) of Hartley 2 as part of its extended mission. As of November 2010 Hartley 2 is the smallest comet which has been visited.
320_Hartley/URL = https://upload.wikimedia.org/wikipedia/commons/e/e6/Comet_Hartley_2.jpg
330_ShoemakerLevy/License = https://en.wikipedia.org/wiki/File:Shoemaker-Levy_9_on_1994-05-17.png
330_ShoemakerLevy/Title = Comet Shoemaker0x2013Levy 9 was a comet that broke apart in July 1992 and collided with Jupiter in July 1994, providing the first direct observation of an extraterrestrial collision of Solar System objects. This generated a large amount of coverage in the popular media, and the comet was closely observed by astronomers worldwide. The collision provided new information about Jupiter and highlighted its possible role in reducing space debris in the inner Solar System.
330_ShoemakerLevy/URL = https://upload.wikimedia.org/wikipedia/commons/7/71/Shoemaker-Levy_9_on_1994-05-17.png
330_ShoemakerLevy/02_CrashAnimation/License = https://en.wikipedia.org/wiki/File:Max_Planck_Institute_Shoemaker0x2013Levy_9.gif
330_ShoemakerLevy/02_CrashAnimation/Title = Jupiter in infrared, Shoemaker0x2013Levy 9 collision (left), Io (right).
330_ShoemakerLevy/02_CrashAnimation/URL = https://upload.wikimedia.org/wikipedia/commons/b/b4/Max_Planck_Institute_Shoemaker0x2013Levy_9.gif
330_ShoemakerLevy/02_CrashScars/License = https://en.wikipedia.org/wiki/File:Jupiter_showing_SL9_impact_sites.jpg
330_ShoemakerLevy/02_CrashScars/Title = Brown spots mark impact sites on Jupiter's southern hemisphere.
330_ShoemakerLevy/02_CrashScars/URL = https://upload.wikimedia.org/wikipedia/commons/5/5d/Jupiter_showing_SL9_impact_sites.jpg
330_ShoemakerLevy/03_CrashScars/License = https://en.wikipedia.org/wiki/File:Impact_site_of_fragment_G.png
330_ShoemakerLevy/03_CrashScars/Title = A reddish, asymmetric ejecta pattern.
330_ShoemakerLevy/03_CrashScars/URL = https://upload.wikimedia.org/wikipedia/commons/8/81/Impact_site_of_fragment_G.png
400_Meteorid/License = https://en.wikipedia.org/wiki/File:Cosmic_Fireball_Falling_Over_ALMA.jpg
400_Meteorid/Title = A meteoroid is a small rocky or metallic body in outer space.
400_Meteorid/URL = https://upload.wikimedia.org/wikipedia/commons/9/95/Cosmic_Fireball_Falling_Over_ALMA.jpg
400_Meteorid/02_Fragments/License = https://en.wikipedia.org/wiki/File:323213main_Petersmeteorites_946-710.jpg
400_Meteorid/02_Fragments/Title = 2008 TC3 meteorite fragments found on February 28, 2009, in the Nubian Desert, Sudan
400_Meteorid/02_Fragments/URL = https://upload.wikimedia.org/wikipedia/commons/3/38/323213main_Petersmeteorites_946-710.jpg
400_Meteorid/03_PerseideAnimation/License = https://en.wikipedia.org/wiki/File:P10220XX.01.49.MESZ.14.08.2019.Berlin.Perseiden.x1.0.gif
400_Meteorid/03_PerseideAnimation/Title = A meteoroid of the Perseids with a size of about ten millimetres entering the earth's atmosphere in real time. The meteorid is at the bright head of the trail, and the ionisation of the mesosphere is still visible in the tail.
400_Meteorid/03_PerseideAnimation/URL = https://upload.wikimedia.org/wikipedia/commons/4/4e/P10220XX.01.49.MESZ.14.08.2019.Berlin.Perseiden.x1.0.gif
400_Meteorid/04_Leonid/License = https://en.wikipedia.org/wiki/File:Leonid_Meteor.jpg
400_Meteorid/04_Leonid/Title = A meteor of the Leonid meteor shower0x003B the photograph shows the meteor, afterglow, and wake as distinct components
400_Meteorid/04_Leonid/URL = https://upload.wikimedia.org/wikipedia/commons/a/a7/Leonid_Meteor.jpg
400_Meteorid/05_Chelyabinsk/License = https://en.wikipedia.org/wiki/File:2013_Chelyabinsk_meteor_trace.jpg
400_Meteorid/05_Chelyabinsk/Title = The Chelyabinsk meteor was an extremely bright, exploding fireball, known as superbolide, measuring about 17 to 20 m across, with an estimated initial mass of 11,000 tonnes, as the relatively small asteroid entered Earth's atmosphere. It was the largest known natural object to have entered Earth's atmosphere since the Tunguska event in 1908.
400_Meteorid/05_Chelyabinsk/URL = https://upload.wikimedia.org/wikipedia/commons/d/d4/2013_Chelyabinsk_meteor_trace.jpg
400_Meteorid/06_ISS/License = https://en.wikipedia.org/wiki/File:Looking_Down_on_a_Shooting_Star.JPG
400_Meteorid/06_ISS/Title = This astronaut photograph, taken from the International Space Station provides the unusual perspective of looking down on a meteor as it passes through the atmosphere. Green and yellow airglow appears in thin layers above the limb of the Earth, extending from image left to the upper right. Atoms and molecules above 50 kilometers in the atmosphere are excited by sunlight during the day, and then release this energy at night, producing primarily green light that is observable from orbit.
400_Meteorid/06_ISS/URL = https://upload.wikimedia.org/wikipedia/commons/b/b7/Looking_Down_on_a_Shooting_Star.JPG
400_Meteorid/07_Murnpeowie/License = https://en.wikipedia.org/wiki/File:Murnpeowie_meteorite.jpg
400_Meteorid/07_Murnpeowie/Title = Murnpeowie Meteorite - this spectacular, 2520 pound iron meteorite was found in the South Australian Outback in 1909. The mass has a well-preserved, dark-colored, outer surface with nice regmaglypts (surface cavities). Iron meteorites exposed at Earth's surface oxidize & rust relatively quickly. Given the fresh nature of Murnpeowie, it's been estimated that it fell to Earth within five years of it being found.
400_Meteorid/07_Murnpeowie/URL = https://upload.wikimedia.org/wikipedia/commons/7/79/Murnpeowie_meteorite.jpg
400_Meteorid/08_Willamette/License = https://en.wikipedia.org/wiki/File:Willamette_Meteorite_AMNH.jpg
400_Meteorid/08_Willamette/Title = The Willamette Meteorite, officially named Willamette and originally known as Tomanowos by the Clackamas Chinook Native American tribe is an iron-nickel meteorite found in the U.S. state of Oregon. It is the largest meteorite found in North America and the sixth largest in the world. There was no impact crater at the discovery site0x003B researchers believe the meteorite landed in what is now Canada or Montana, and was transported as a glacial erratic to the Willamette Valley during the Missoula Floods at the end of the last Ice Age (~13,000 years ago).
400_Meteorid/08_Willamette/URL = https://upload.wikimedia.org/wikipedia/commons/c/cc/Willamette_Meteorite_AMNH.jpg
400_Meteorid/09_Hoba/License = https://en.wikipedia.org/wiki/File:Hoba_meteorite_(15682150765).jpg
400_Meteorid/09_Hoba/Title = The Hoba meteorite, short for Hoba West, is a meteorite that lies on the farm of the same name, not far from Grootfontein, in the Otjozondjupa Region of Namibia. It has been uncovered but, because of its large mass, has never been moved from where it fell. The main mass is estimated at more than 60 tonnes. It is the largest known intact meteorite (as a single piece). In 1920 the owner of the land, Jacobus Hermanus Brits, encountered the object while ploughing one of his fields with an ox. During this task, he heard a loud metallic scratching sound and the plough came to an abrupt halt.
400_Meteorid/09_Hoba/URL = https://upload.wikimedia.org/wikipedia/commons/a/a7/Hoba_meteorite_(15682150765).jpg
400_Meteorid/10_CapeYork/License = https://en.wikipedia.org/wiki/File:Agpalilik_fragment_of_Cape_York_meteorite.jpg
400_Meteorid/10_CapeYork/Title = The Cape York meteorite, also known as the Innaanganeq meteorite, is one of the largest known iron meteorites, classified as a medium octahedrite in chemical group IIIAB. In addition to many small fragments, at least eight large fragments with a total mass of 58 tons have been recovered. The date of the meteorite fall is debated, but was probably within the last few thousand years. It was known to local Inuit for centuries, who used it as a source of meteoritic iron for tools.
400_Meteorid/10_CapeYork/URL = https://upload.wikimedia.org/wikipedia/commons/a/a4/Agpalilik_fragment_of_Cape_York_meteorite.jpg
400_Meteorid/11_Bendego/License = https://en.wikipedia.org/wiki/File:Museu_Nacional,_UFRJ_-_Quinta_da_Boa_Vista_3.jpg
400_Meteorid/11_Bendego/Title = The Bendeg0x00F3 Meteorite (also known as Pedra do Bendeg0x00F3 or simply Bendeng0x00F3) is a meteorite found in the interior of the state of Bahia, Brazil. It weights 5,360 kilograms. The Bendeg0x00F3 meteorite was found in 1784 by the boy Domingos da Motta Botelho, who grazed cattle on a farm near the present town of Monte Santo, Bahia. News of the finding quickly spread. In 1785, governor D. Rodrigues Menezes arranged for it to be transported to Salvador, however, the meteorite's excessive weight made transportation difficult. The cart it was on ran out of control down a hill and the meteorite fell into a dry stream bed, 180 meters away from the spot where it was originally found. It remained there until 1888, when it was recovered and brought to the National Museum.
400_Meteorid/11_Bendego/URL = https://upload.wikimedia.org/wikipedia/commons/4/41/Museu_Nacional,_UFRJ_-_Quinta_da_Boa_Vista_3.jpg
400_Meteorid/12_Esquel/License = https://en.wikipedia.org/wiki/File:Pallasite-Esquel-RoyalOntarioMuseum-Jan18-09.jpg
400_Meteorid/12_Esquel/Title = Esquel is a meteorite found near Esquel, a Patagonian town in the northwest part of the province of Chubut in Argentina. It is a pallasite, a type of stony0x2013iron meteorite that when cut and polished shows yellowish olivine (peridot) crystals. In 1951 a farmer uncovered a meteorite in an unknown location near Esquel while digging a hole for a water tank. The meteorite was purchased from the finders and taken to the United States in 1992 by meteorite expert Robert Haag. The Esquel pallasite is known worldwide among collectors and the meteoritical scientific community. Esquel is regarded as one of the most beautiful meteorites ever found and is also one of the most desirable pallasites among meteorite collectors. It is a main group pallasite (MGP).
400_Meteorid/12_Esquel/URL = https://upload.wikimedia.org/wikipedia/commons/a/ad/Pallasite-Esquel-RoyalOntarioMuseum-Jan18-09.jpg
400_Meteorid/12_Esquel_02_Polished/License = https://en.wikipedia.org/wiki/File:Esquel.jpg
400_Meteorid/12_Esquel_02_Polished/Title = The slice shows the crystals' transparency.
400_Meteorid/12_Esquel_02_Polished/URL = https://upload.wikimedia.org/wikipedia/commons/0/00/Esquel.jpg

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