Because of its retrograde orbit and relative proximity to Neptune (closer than the Moon is to Earth), Triton is grouped with the planet's irregular moons (see below). However, we do not guarantee individual replies due to the high volume of messages. Neso This distance exceeds Mercury's aphelion, which is Neso is about 60km (37mi) in diameter based on an assumed albedo, and assuming a mean density of 1.5 g/cm3,[6] its mass is estimated at 21017 kg. This distance is great enough that it exceeds Mercury's aphelion, which is approximately 70 Gm from the Sun. Neso also known as Neptune XIII, is the farthest non-spherical moon of Neptune. From an average distance of 2.8 billion miles (4.5 billion kilometers), Neptune is 30 astronomical units away from the Sun. From an average distance of 2.8 billion miles (4.5 billion kilometers), Neptune is 30 astronomical units away from the Sun. Distance from Neptune It was found by Matthew J. Holman, Brett J. Gladman, et al. WebNeso is one of Neptune's fourteen moons. Triton is also one of the coldest moons in the Solar System, with surface temperature of about 38 K (235.2 C). Before the announcement of its name on February 3, 2007 (IAUC 8802), Neso was known by its designation S/2002 N 4. https://wiki.kidzsearch.com/w/index.php?title=Neso_(moon)&oldid=4300503, the Creative Commons Attribution-ShareAlike License; additional terms may apply. Thank you for taking time to provide your feedback to the editors. Neso WebIt is a retrograde irregular moon discovered by Matthew J. Holman, Brett J. Gladman, et al. Neptune Use this form if you have come across a typo, inaccuracy or would like to send an edit request for the content on this page. The moon's orbit is among the most distant from its planet than any other known moon in Given the lopsided distribution of mass in its moons, it is widely believed that Triton was captured after the formation of Neptune's original satellite system much of which would have been destroyed in the process of capture. Neso was discovered on 14th August 2002 by teams of astronomers led by Matthew Holman and John Kavelaars. Triton, being the largest and most massive of Neptune's moons, was the first to be discovered. WebA small irregular moon of Neptune, notable for its immense distance from its primary planet. or, by Matt Williams, Universe Today. The information you enter will appear in your e-mail message and is not retained by Phys.org in any form. This disambiguation page lists articles associated with the title Neso. Neso comes as close as 28.93 million km to Neptune and recedes as far as 71.58 million km, its maximum distance from Neptune, making it the most distant known moon of any planet. Triton itself is almost an order of magnitude larger than all other known irregular moons and comprises more than 99.5% of all the mass known to orbit Neptune (including the planet's rings and thirteen other known moons). One astronomical unit (abbreviated as AU), is the distance from the Sun to Earth. For a listing of all moons, see Moons of the Planets. Moons of Neptune Neso orbits Neptune at a distance of more than 48 million km , making it the farthest known moon of any planet. In Greek mythology, Neso is one of the Nereids, one of the 50 daughters of Nereus and Doris. Neso At its apoapsis - the farthest point in its orbit from Neptune - it approaches a distance greater than that of Mercury from the Sun. It has the longest known orbit for a moon - over 26 years. Thirdly, they both have unusual orbital eccentricities: Nereid has one of the most eccentric orbits of any known irregular satellite, and Triton's orbit is a nearly perfect circle. The discovery of this moon was purely fortuitous, and occurred as a result of the ongoing search for rings similar to those discovered around Uranus four years earlier. Its mass is estimated at 1.61017 kg. Get weekly and/or daily updates delivered to your inbox. Neso is classed as an irregular retrograde moon. All but the outer two are within Neptune-synchronous orbit (meaning that orbit Neptune slower than it's orbital period (0.6713 days) and thus are being tidally decelerated. Neso (moon With a mean diameter of around 2700 km and a mass of 214080 520 x 1017 kg, Triton is the largest of Neptune's moons, and the only one large enough to achieve hydrostatic equilibrium (i.e. Water ice has been spectroscopically detected on its surface. Many theories have been offered regarding the mechanisms of its capture over the years. Neso orbits Neptune at a mean distance of 50.26 million km. WebNeso is the furthest moon in the solar system of any, orbiting Neptune. Neso googletag.cmd.push(function() { googletag.display('div-gpt-ad-1449240174198-2'); }); Initially, only Triton Neptune's largest moon could be observed. Its mass is estimated at 1.61017 kg. If rings were in fact present, the star's luminosity would decrease slightly just before the planet's closest approach. It has the longest known orbit for a moon - over 26 years. At some points in its orbit it is farther from Neptune than Mercury is from the Sun. Neso It follows a retrograde, highly inclined, and highly eccentric orbit illustrated on the diagram in relation to other irregular satellites of Neptune. It follows a very inclined and very eccentric orbit illustrated on the diagram in relation to other irregular satellites of Neptune. WebNeso is the outermost of the 14 known moons of Neptune. The third moon, later named Larissa, was first observed by Harold J. Reitsema, William B. Hubbard, Larry A. Lebofsky and David J. Tholen on May 24th, 1981. Your feedback is important to us. Overview. Very little is known about Neso, another of Neptune's extremely distant irregular moons. [2] [8] Neso orbits Neptune at a distance of more than 48 Gm (billion m ), making it (as WebIn order of distance from Neptune, the regular moons are Naiad, Thalassa, Despina, Galatea, Larissa, Hippocamp, and Proteus. Neso also known as Neptune XIII, is the farthest non-spherical moon of Neptune. Learn about it here! Neso In addition, all the inner moons dark objects, with geometric albedo ranging from 7 to 10%. You can unsubscribe at any time and we'll never share your details to third parties. Neso (moon All but the outer two are within Neptune- synchronous orbit (Neptune's rotational period is 0.6713 day or 16 hours Neso WebIn order of distance from Neptune, the regular moons are Naiad, Thalassa, Despina, Galatea, Larissa, Hippocamp, and Proteus. They generally follow inclined eccentric and often retrograde orbits far from Neptune; the only exception is Triton, which orbits close to the planet following a circular orbit, though retrograde and inclined. At apocenter, the satellite is more than 72 Gm from Neptune. Their spectra also indicated that they are made from water ice contaminated by some very dark material, probably organic compounds. Before the announcement of its name on February 3, 2007 (IAUC 8802), Neso was known by its designation S/2002 N 4. An irregular moon usually refers to a moon that has been captured by a planet's gravity rather than one which formed around it. WebNeso can refer to: Neso, one of the Nereids. Neso Neso (moon Five of those six new moons were seen again, including the moon that is now known as Neso. A retrograde moon is one that orbits in the opposite direction of its host planet's rotation. Neso Neither your address nor the recipient's address will be used for any other purpose. WebNeso is the outermost moon of planet Neptune and has a similar orbit with Psamathe, indicating that they might originally have been part of a larger moon that broke apart. Neso is about 60 km in diameter, and assuming the mean density of 1.5 g/cm 3. Neso The as yet unnamed fourteenth moon, currently identified as S/2004 N 1, is thought to measure no more than 1620 km in diameter. WebNeso also known as Neptune XIII, is the farthest non-spherical moon of Neptune. Discovery of new ornithopod solves mystery of unidentified large dinosaur tracks, Hydrogen peroxide found on Jupiter's moon Ganymede in higher latitudes, Magnetic Quincke rollers: Forces and torques of magnetism that guide complex dynamics of active particles, Observers investigate a short-period X-ray binary system, Using GPS as a possible earthquake predictor, Science X Daily and the Weekly Email Newsletter are free features that allow you to receive your favorite sci-tech news updates in your email inbox. Finally, Nereid also has the lowest inclination of any known irregular satellite. How distant you may ask, well, check out the video to find out. For general feedback, use the public comments section below (please adhere to guidelines). How distant you may ask, well, check out the video to find out. Neso on August 14, 2002, though it went unnoticed until 2003. moons of Neptune WebIn order of distance from Neptune, the regular moons are Naiad, Thalassa, Despina, Galatea, Larissa, Hippocamp, and Proteus. The moon's orbit is among the most distant from its planet than any other known moon in on August 14, 2002, though it went unnoticed until 2003. It follows a very inclined and very eccentric orbit illustrated on the diagram in relation to other irregular satellites of Neptune. Neso (moon WebNeso is the outermost of the 14 known moons of Neptune. At its apoapsis - the farthest point in its orbit from Neptune - it approaches a distance greater than that of Mercury from the Sun. Neso is about 60 km in diameter, and assuming the mean density of 1.5 g/cm 3. Moons of Neptune The most widely-accepted is that Triton is a surviving member of a binary Kuiper Belt Object that was disrupted with an encounter with Neptune. At a distance of 354,759 km from Neptune, it also sits between the planet's inner and outer moons. From an average distance of 2.8 billion miles (4.5 billion kilometers), Neptune is 30 astronomical units away from the Sun. For a listing of all moons, see Moons of the Planets. Neso (moon), the outermost moon of Neptune, and the moon with the greatest known orbital distance from its planet. Neso WebShortest mean distance between Neptune and Neso is about 48.387 million kilometer or about 0.3234 AU (astronomical unit) Neptune is 8 th planet in our solar system This disambiguation page lists articles associated with the title Neso. Overview. Neso is the goddess of islands. It orbits Neptune at a distance of more than 48 million km, making it the most distant known moon of any planet. By using our site, you acknowledge that you have read and understand our Privacy Policy It has a diameter of 60 kilometres (37 miles). The inner moons are closely associated with Neptune's narrow ring system. Consider supporting ScienceX's mission by getting a premium account. Its mass is estimated at 1.61017 kg. Overview. Given the similarity of the orbit's parameters with Psamathe (S/2003 N 1), it was suggested that both irregular satellites could have a common origin in the break-up of a larger moon.[4]. WebNeso also known as Neptune XIII, is the farthest non-spherical moon of Neptune. The yellow segments extend from the pericentre to the apocentre, showing the eccentricity. and Terms of Use. WebNeso is the outermost moon of planet Neptune and has a similar orbit with Psamathe, indicating that they might originally have been part of a larger moon that broke apart. Neptune Neso, daughter of King Teucer. WebNeso is the outermost moon of Neptune and the most distant orbiting moon in our solar system. The moon measures approximately 20 miles (34 kilometers) across, making it the smallest known moon of Neptune. It has a diameter of 60 kilometres (37 miles). At a distance of 354,759 km from Neptune, it also sits between the planet's inner and outer moons. It was found by Matthew J. Holman, Brett J. Gladman, et al. Neso Only the two largest regular moons have been imaged with a resolution sufficient to discern their shapes and surface features. Neso This disambiguation page lists articles associated with the title Neso. on August 14, 2002, though it went unnoticed until 2003. WebNeso is the outermost of the 14 known moons of Neptune. First of all, they are the largest two known irregular moons in the Solar System. on August 14, 2002, though it went unnoticed until 2003. No further moons were found until Voyager 2 flew by Neptune in 1989. Nereid is the third-largest moon of Neptune. WebNeso orbits Neptune at a distance of more than 48 million km, making it the farthest known moon of any planet. It was found by Matthew J. Holman, Brett J. Gladman, et al. [2] [8] Neso orbits Neptune at a distance of more than 48 Gm (billion m ), making it (as It may also be referred to as Neptune XIII. The next moon, Galatea, orbits just inside the most prominent Adams ring and its gravity helps maintaining the ring by containing its particles. WebA small irregular moon of Neptune, notable for its immense distance from its primary planet. Neso is about 60 km in diameter, and assuming the mean density of 1.5 g/cm3. Very little is known about Neso, another of Neptune's extremely distant irregular moons. This page was last changed on 12 March 2013, at 22:46. It was found by Matthew J. Holman, Brett J. Gladman, et al. [2] [8] Neso orbits Neptune at a distance of more than 48 Gm (billion m ), making it (as For general inquiries, please use our contact form. The first was Nereid, Neptune's second largest and most massive moon, which was discovered on May 1st, 1949, by Gerard P. Kuiper (for whom the Kuiper Belt is named) using photographic plates from the McDonald Observatory in Fort Davis, Texas. WebNeso is one of Neptune's fourteen moons. 0.33 AU (~49,500,000 km), 3,220 Neptune radii, 49.285 Gm. WebNeso is a dwarf moon, that has unbelievable distance from Neptune while orbiting it. Neso, daughter of King Teucer. At apocenter, the satellite is more than 72 Gm from Neptune. WebNeso orbits Neptune at a distance of more than 48 Gm (billion m), making it (as of 2015) the most distant known moon of any planet. part may be reproduced without the written permission. Neso orbits Neptune at a mean distance of 50.26 million km. on August 14, 2002, though it went unnoticed until 2003. Neptune Neso It was found by Matthew J. Holman, Brett J. Gladman, et al. Neso All but the outer two are within Neptune- synchronous orbit (Neptune's rotational period is 0.6713 day or 16 hours Neso comes as close as 28.93 million km to Neptune and recedes as far as 71.58 million km, its maximum distance from Neptune, making it the most distant known moon of any planet. However, the orbit of Neso is fairly elongated. Distance from Neptune Neso /niso/, also known as Neptune XIII, is the outermost known natural satellite of Neptune. WebNeso is the furthest moon in the solar system of any, orbiting Neptune. Neso WebNon-spherical moons of Neptune. Neso's eccentric orbit takes it millions of miles from the ice giant. At some points in its orbit it is farther from Neptune than Mercury is from the Sun. Neso is about 60 km in diameter, and assuming the mean density of 1.5 g/cm3. WebNeso can refer to: Neso, one of the Nereids. Your email address is used only to let the recipient know who sent the email. Before it was officially named on February 3, 2007 (IAUC 8802), Neso was known by its provisional designation, S/2002 N 4. And just seventeen days after it was discovered, astronomers began to notice that it too had a system of moons. Neso However, owing to the moon being geologically active (which results in cryovolcanism) and surface temperature variations that cause sublimation, Triton is one of only two moons in the Solar System that has a substantial atmosphere. The moon measures approximately 20 miles (34 kilometers) across, making it the smallest known moon of Neptune. Neso Neso is one of Neptune's fourteen moons. Secondly, they both have atypically small semi-major axes, with Triton's being over an order of magnitude smaller than those of all other known irregular moons. Neptune's Regular Moons are those located closest to the planet and which follow circular prograde orbits that lie in the planet's equatorial plane. It follows a very inclined and very eccentric orbit illustrated on the diagram in relation to other irregular satellites of Neptune. It was observed by William Lassell on October 10th, 1846, just seventeen days after Neptune was discovered. Given its distance from the Sun, the only mission to ever study Neptune and its moons up close was the Voyager 2 mission. This indicated the presence of a moon rather than a ring. But by the mid-20th century and after, thanks to improvements in ground-based telescopes and the development of robotic space probes, many more moons would be discovered. Neso Neso

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