outer planets
... objects are called trans-Neptunian objects (TNOs) and exist in the Kuiper Belt. • Kuiper Belt a region of the solar system that is just beyond the orbit of Neptune and that contains dwarf planets and other small bodies made mostly of ice • Eris, Makemake, and Haumea are trans-neptunian dwarf planets ...
... objects are called trans-Neptunian objects (TNOs) and exist in the Kuiper Belt. • Kuiper Belt a region of the solar system that is just beyond the orbit of Neptune and that contains dwarf planets and other small bodies made mostly of ice • Eris, Makemake, and Haumea are trans-neptunian dwarf planets ...
It`s time for the human race to enter the solar system
... Asteroids are small rocky bodies that orbit the Sun between the orbits of Mars and Jupiter, primarily in the asteroid belt. Their orbits generally lie close to the plane of the planetary orbits, although they are usually tilted a bit more. Some have quite large eccentricities. Some 500,000 asteroids ...
... Asteroids are small rocky bodies that orbit the Sun between the orbits of Mars and Jupiter, primarily in the asteroid belt. Their orbits generally lie close to the plane of the planetary orbits, although they are usually tilted a bit more. Some have quite large eccentricities. Some 500,000 asteroids ...
Dwarf Planets - Cloudfront.net
... One Dwarf planet does have a composition similar to Earth…Ceres It was once considered an asteroid it orbits in the asteroid belt between Mars and Jupiter at 2.77 AU It is between 909 & 975km in diameter. ...
... One Dwarf planet does have a composition similar to Earth…Ceres It was once considered an asteroid it orbits in the asteroid belt between Mars and Jupiter at 2.77 AU It is between 909 & 975km in diameter. ...
Bianca
... dark spots but there is one really big one. It is also the darkest and it is called the Great Dark Spot. ...
... dark spots but there is one really big one. It is also the darkest and it is called the Great Dark Spot. ...
Solar System Bodies PPT
... gas to somewhat liquid materials on what would be the “surface” Possible that the center is solid if differentiation is happening just as it did on Earth. ...
... gas to somewhat liquid materials on what would be the “surface” Possible that the center is solid if differentiation is happening just as it did on Earth. ...
Dwarf Planets - cloudfront.net
... • Has enough mass so that gravity makes them roughly spherical • But have not cleared their orbit of other objects ...
... • Has enough mass so that gravity makes them roughly spherical • But have not cleared their orbit of other objects ...
Comets…
... Small objects in the Solar System Meteors, Comets, : we see them without a telescope Asteroids: small rocky objects mostly between Mars and Jupiter – too faint to see without a telescope Kuiper belt objects: even fainter objects beyond Pluto, debris left over from solar system formation Image of co ...
... Small objects in the Solar System Meteors, Comets, : we see them without a telescope Asteroids: small rocky objects mostly between Mars and Jupiter – too faint to see without a telescope Kuiper belt objects: even fainter objects beyond Pluto, debris left over from solar system formation Image of co ...
Powerpoint - BU Imaging Science
... Pluto makes three orbits for every two orbits by Neptune So do lots of other Kuiper Belt objects Many Kuiper Belt Objects are in stable orbital resonances with Neptune, whereas unstable orbital resonances with Jupiter cause gaps in Asteroid Belt ...
... Pluto makes three orbits for every two orbits by Neptune So do lots of other Kuiper Belt objects Many Kuiper Belt Objects are in stable orbital resonances with Neptune, whereas unstable orbital resonances with Jupiter cause gaps in Asteroid Belt ...
Remnants of Rock and Ice (Chapter 12)
... Pluto makes three orbits for every two orbits by Neptune So do lots of other Kuiper Belt objects Many Kuiper Belt Objects are in stable orbital resonances with Neptune, whereas unstable orbital resonances with Jupiter cause gaps in Asteroid Belt ...
... Pluto makes three orbits for every two orbits by Neptune So do lots of other Kuiper Belt objects Many Kuiper Belt Objects are in stable orbital resonances with Neptune, whereas unstable orbital resonances with Jupiter cause gaps in Asteroid Belt ...
Goal: To understand what the Kuiper Belt is, and why it is
... Classical Region Ranges from 42-47 AUs. Quaoar and Varuna are the most famous objects from this region. ...
... Classical Region Ranges from 42-47 AUs. Quaoar and Varuna are the most famous objects from this region. ...
Pluto was discovered on February 18th 1930 by Clyde
... There are 8 planets in our Solar System, but lots of smaller bodies that are now being called dwarf planets. Examples of dwarf planets are Pluto, Ceres and Eris. Astronomers used to think that the Solar System ended at Pluto but in 1992 the Kuiper Belt was discovered beyond Neptune. Many dwarf plane ...
... There are 8 planets in our Solar System, but lots of smaller bodies that are now being called dwarf planets. Examples of dwarf planets are Pluto, Ceres and Eris. Astronomers used to think that the Solar System ended at Pluto but in 1992 the Kuiper Belt was discovered beyond Neptune. Many dwarf plane ...
Summary of Chapter 8
... planetesimals that formed beyond Neptune’s orbit remain there today as the Kuiper Belt. Icy planetesimals that formed between Jupiter and Neptune were scattered in all directions by Jupiter’s gravity, forming the Oort Cloud. Comets come from the Kuiper Belt and Oort Cloud. Solar system formation end ...
... planetesimals that formed beyond Neptune’s orbit remain there today as the Kuiper Belt. Icy planetesimals that formed between Jupiter and Neptune were scattered in all directions by Jupiter’s gravity, forming the Oort Cloud. Comets come from the Kuiper Belt and Oort Cloud. Solar system formation end ...
Orbital excitation of the Giant planets & its relation to the Late Heavy
... increased chaotic scattering of U,N and S (~2 My) inclinations are increased • Rapid migration phase: 5-30 My for 90% Δa ...
... increased chaotic scattering of U,N and S (~2 My) inclinations are increased • Rapid migration phase: 5-30 My for 90% Δa ...
Life in the Universe lab1
... +asteroid+belt,+a+region+between+Mars+and+Jupiter.+The+images+are+helping+astronomers+plan+f or+the+Dawn+spacecraft's+tour+of+these+hefty+asteroids.+Credit:+NASA,+ESA,+J.+Parker+(Southwest +Research+Institute),+L.+McFadden+(University+of+Maryland) Pallas- is the second largest asteroid Vesta- the th ...
... +asteroid+belt,+a+region+between+Mars+and+Jupiter.+The+images+are+helping+astronomers+plan+f or+the+Dawn+spacecraft's+tour+of+these+hefty+asteroids.+Credit:+NASA,+ESA,+J.+Parker+(Southwest +Research+Institute),+L.+McFadden+(University+of+Maryland) Pallas- is the second largest asteroid Vesta- the th ...
Four Great Satellite Observatories Hubble Space Telescope
... extending to about 50,000 AU Kuiper belt: On orderly orbits from 30-100 AU in disk of solar system ...
... extending to about 50,000 AU Kuiper belt: On orderly orbits from 30-100 AU in disk of solar system ...
Boardworks Space Physics W8
... orbits the Sun, has enough mass to be spherical, and has cleared the area around its orbit of objects.” This photograph shows Pluto and its moon, Charon. Pluto’s orbit is surrounded by smaller objects that have not been cleared by its gravitational field. Pluto and the other ‘smaller’ planet-like ob ...
... orbits the Sun, has enough mass to be spherical, and has cleared the area around its orbit of objects.” This photograph shows Pluto and its moon, Charon. Pluto’s orbit is surrounded by smaller objects that have not been cleared by its gravitational field. Pluto and the other ‘smaller’ planet-like ob ...
Kuiper belt objects - Rosemary`s ePortfolio
... objects beyond the orbit of Neptune. Found by Gerard Kuiper It contains debris from the early creation of the solar system. It contains short-period comets. ...
... objects beyond the orbit of Neptune. Found by Gerard Kuiper It contains debris from the early creation of the solar system. It contains short-period comets. ...
Primordial Matter in the Solar System
... • Keplerian orbits, e.g. P2 = a3 • Gaps, such as the Kirkwood Gap, due to orbital resonance with Jupiter and other asteroids (like the Cassini Division in Saturn’s rings) • Jupiter maintains the asteroid belt, although may have prevented planet formation • Families of asteroids: Floras, Trojans, and ...
... • Keplerian orbits, e.g. P2 = a3 • Gaps, such as the Kirkwood Gap, due to orbital resonance with Jupiter and other asteroids (like the Cassini Division in Saturn’s rings) • Jupiter maintains the asteroid belt, although may have prevented planet formation • Families of asteroids: Floras, Trojans, and ...
Solutions
... Suppose someone claimed to make the discoveries described below. (These are not real discoveries.) Decide whether each discovery should be considered reasonable or surprising. Explain clearly; not all these have definitive answers, so your explanation is more important than your chosen answer. 19. A ...
... Suppose someone claimed to make the discoveries described below. (These are not real discoveries.) Decide whether each discovery should be considered reasonable or surprising. Explain clearly; not all these have definitive answers, so your explanation is more important than your chosen answer. 19. A ...
A Look at Our Solar System: The Sun, the planets and more
... First three are narrow, fourth one is broad and more diffused. Space between them are filled with dust. Made mostly of microscopic particles. ...
... First three are narrow, fourth one is broad and more diffused. Space between them are filled with dust. Made mostly of microscopic particles. ...
The Pluto controversy: What`s a planet, anyway?
... The best question of all: what questions intrigue you? Imagine a Solar System curriculum that begins with the concept of density—a big concept for third graders, but not inaccessible. Rocks and metals have high density. Balloons and beach balls have low density. Divide the inner and outer planets in ...
... The best question of all: what questions intrigue you? Imagine a Solar System curriculum that begins with the concept of density—a big concept for third graders, but not inaccessible. Rocks and metals have high density. Balloons and beach balls have low density. Divide the inner and outer planets in ...
Your 2nd midterm …
... Long-period comets originate in a spherical cloud of icy bodies extending from 10,000 to 100,000 AU away from the sun and called the Oort cloud Some short-period comets can come from the Oort cloud and have their orbits altered by Jupiter, but most of them are thought to belong to the Kuiper belt lo ...
... Long-period comets originate in a spherical cloud of icy bodies extending from 10,000 to 100,000 AU away from the sun and called the Oort cloud Some short-period comets can come from the Oort cloud and have their orbits altered by Jupiter, but most of them are thought to belong to the Kuiper belt lo ...
Kuiper belt
The Kuiper belt /ˈkaɪpər/ or /'køypǝr/ (as in Dutch), sometimes called the Edgeworth–Kuiper belt, is a region of the Solar System beyond the planets, extending from the orbit of Neptune (at 30 AU) to approximately 50 AU from the Sun. It is similar to the asteroid belt, but it is far larger—20 times as wide and 20 to 200 times as massive. Like the asteroid belt, it consists mainly of small bodies, or remnants from the Solar System's formation. Although many asteroids are composed primarily of rock and metal, most Kuiper belt objects are composed largely of frozen volatiles (termed ""ices""), such as methane, ammonia and water. The Kuiper belt is home to three officially recognized dwarf planets: Pluto, Haumea, and Makemake. Some of the Solar System's moons, such as Neptune's Triton and Saturn's Phoebe, are also thought to have originated in the region.The Kuiper belt was named after Dutch-American astronomer Gerard Kuiper, though he did not actually predict its existence. In 1992, 1992 QB1 was discovered, the first Kuiper belt object (KBO) since Pluto. Since its discovery, the number of known KBOs has increased to over a thousand, and more than 100,000 KBOs over 100 km (62 mi) in diameter are thought to exist. The Kuiper belt was initially thought to be the main repository for periodic comets, those with orbits lasting less than 200 years. However, studies since the mid-1990s have shown that the belt is dynamically stable, and that comets' true place of origin is the scattered disc, a dynamically active zone created by the outward motion of Neptune 4.5 billion years ago; scattered disc objects such as Eris have extremely eccentric orbits that take them as far as 100 AU from the Sun.The Kuiper belt should not be confused with the hypothesized Oort cloud, which is a thousand times more distant and is not flat. The objects within the Kuiper belt, together with the members of the scattered disc and any potential Hills cloud or Oort cloud objects, are collectively referred to as trans-Neptunian objects (TNOs).Pluto is likely the largest and most-massive member of the Kuiper belt and the largest and the second-most-massive known TNO, surpassed only by Eris in the scattered disc. Originally considered a planet, Pluto's status as part of the Kuiper belt caused it to be reclassified as a dwarf planet in 2006. It is compositionally similar to many other objects of the Kuiper belt, and its orbital period is characteristic of a class of KBOs, known as ""plutinos"", that share the same 2:3 resonance with Neptune.