Because of its blue color, Neptune was named for the Roman god of the sea. This statue of Neptune is at the Trevi Fountain in Rome.
Neptune, shown in Figure below, is the only major planet that can’t be seen from Earth without a telescope. Scientists predicted the existence of Neptune before it was discovered because Uranus did not always appear exactly where it should appear. They knew that the gravitational pull of another planet beyond Uranus must be affecting Uranus’ orbit.
Neptune was discovered in 1846, in the position that had been predicted, and it was named Neptune for the Roman god of the sea because of its bluish color.
In many respects, Neptune is similar to Uranus (Figure below). Neptune has slightly more mass than Uranus, but it is slightly smaller in size. Neptune is much farther from the Sun, at nearly 4.5 billion km (2.8 billion mi). The planet’s slow orbit means that it takes 165 Earth years to go once around the Sun.
Neptune’s blue color is mostly because of frozen methane (CH4). When Voyager 2 visited Neptune in 1986, there was a large dark-blue spot, which scientists named the Great Dark Spot, south of the equator. When the Hubble Space Telescope took pictures of Neptune in 1994, the Great Dark Spot had disappeared, but another dark spot had appeared north of the equator. Astronomers think that both of these spots represent gaps in the methane clouds on Neptune.
The changing appearance of Neptune is caused by its turbulent atmosphere. The winds on Neptune are stronger than on any other planet in the solar system, reaching speeds of 1,100 km/h (700 mi/h), close to the speed of sound. This extreme weather surprised astronomers, since the planet receives little energy from the Sun to power weather systems. Neptune's core is 7000°C (12,632°F) which means that it produces more energy than it receives from the Sun. Neptune is also one of the coldest places in the solar system. Temperatures at the top of the clouds are about -218°C (-360°F).
Neptune has faint rings of ice and dust that may change or disappear in fairly short time frames.
Neptune has 14 known moons. Triton, shown in Figure below, is the only one of them that has enough mass to be spherical in shape. Triton orbits in the direction opposite to the orbit of Neptune. Scientists think Triton did not form around Neptune, but instead was captured by Neptune’s gravity as it passed by.
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| Credit: Courtesy of NASA/JPL-Caltech;By NASA/JPL - http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2194 (file), Public Domain, https://commons.wikimedia.org/w/index.php?curid=126674;By Lookang many thanks to author of original simulation = Todd K. Timberlake author of Easy Java Simulation = Francisco Esquembre - Own work, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=15761788 Source: http://commons.wikimedia.org/wiki/File:Neptune.jpg;By NASA/JPL - http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2194(file), Public Domain, https://commons.wikimedia.org/w/index.php?curid=126674;By Lookang many thanks to author of original simulation = Todd K. Timberlake author of Easy Java Simulation = Francisco Esquembre - Own work, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=15761788 License: Public Domain | ||
| Credit: Courtesy of Lunar and Planetary Institute/NASA;By NASA/JPL - http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2194 (file), Public Domain, https://commons.wikimedia.org/w/index.php?curid=126674;By NASA; Pbroks13 (redraw) - http://solarsystem.nasa.gov/multimedia/gallery/Neptune_Int-browse.jpg, which is in the public domain, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=4948181 Source: http://solarsystem.nasa.gov/multimedia/display.cfm?Category=Planets&IM_ID=283;By NASA/JPL - http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2194(file), Public Domain, https://commons.wikimedia.org/w/index.php?curid=126674;By NASA; Pbroks13 (redraw) - http://solarsystem.nasa.gov/multimedia/gallery/Neptune_Int-browse.jpg,which is in the public domain, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=4948181 License: Public Domain | ||
| Credit: Courtesy of NASA/Jet Propulsion Lab-Caltech/US Geological Survey;By NASA/JPL - http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2194 (file), Public Domain, https://commons.wikimedia.org/w/index.php?curid=126674;By NASA / Jet Propulsion Lab / U.S. Geological Survey - http://photojournal.jpl.nasa.gov/catalog/PIA00317, Public Domain, https://commons.wikimedia.org/w/index.php?curid=96172 Source: http://commons.wikimedia.org/wiki/File:Triton_moon_mosaic_Voyager_2_%2528large%2529.jpg;By NASA/JPL - http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2194(file), Public Domain, https://commons.wikimedia.org/w/index.php?curid=126674;By NASA / Jet Propulsion Lab / U.S. Geological Survey - http://photojournal.jpl.nasa.gov/catalog/PIA00317,Public Domain, https://commons.wikimedia.org/w/index.php?curid=96172 License: Public Domain |
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