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... Jupiter has more than 60 moons. Its ...
Saturn`s Wildest Weather
Saturn`s Wildest Weather

... The Cassini spacecraft zooms above Saturn’s clouds. It’s cold here. Little sunlight reaches the craft. Launched in 1997, Cassini reached Saturn in 2004. Since then, it has made many fantastic finds. Cassini discovered many moons. It found chemical lakes and dunes on Saturn’s largest moon, Titan. It s ...
21trans-neptunian2s
21trans-neptunian2s

... Features of Pluto ...
Introduction - Beck-Shop
Introduction - Beck-Shop

... a wonderful surprise that the ringed planets are just as beautiful and scientifically compelling seen close up! Furthermore, the ringed planets are not just objects of beauty, but complicated physical systems that provide a local laboratory and analogy for other cosmic systems like galaxies and plan ...
Name: ____ Date: __________ Period: ________ Pluto Files (PBS
Name: ____ Date: __________ Period: ________ Pluto Files (PBS

... of a planet? Why does Pluto not fit this description? How long was Pluto considered a planet and what year did it all change and why?  International Astronomical Union (IAU)---they are in charge of naming celestial (space) objects  Current definition: o A planet needs to be round and orbit the Sun ...
Planetary Rings - Astronomy Cast
Planetary Rings - Astronomy Cast

... Pamela: In the case of all three of these bodies... Jupiter, Uranus, and Neptune... we think that the formation process is probably very similar to what is sustaining the rings of Saturn. You start whacking the moons orbiting these planets, and we know that things collide, and the material that get ...
The Potato Radius: a Lower Minimum Size for Dwarf Planets
The Potato Radius: a Lower Minimum Size for Dwarf Planets

... on the yield strength of these bodies during their formative years when their shapes were determined. Our proposed ~200 km potato radius for icy moons would substantially increase the number of trans-Neptunian objects classified as “dwarf planets”. Keywords: planetary science, gravity, accretion, an ...
Jupiter
Jupiter

... • Distinctly larger equatorial than polar diameter – ~ 6.5 % difference for Jupiter – ~ 0.34% difference for Earth ...
Jupiter
Jupiter

... • Distinctly larger equatorial than polar diameter – ~ 6.5 % difference for Jupiter – ~ 0.34% difference for Earth ...
A Theory of the Origin of the Solar System There have been
A Theory of the Origin of the Solar System There have been

... arises in its boundary layer. A t this stage the gravitational force on unit mass of the boundary layer becomes comparable to its centrifugal force. Prior to this stage the gravitational contraction of the solar nebula proceeds without any appreciable viscous loss and the solar nebula spins more or ...
Document
Document

... Pluto – From its discovery in 1930 until 2006, Pluto was classified as a planet. – In the late 1970s, following the discovery of minor planet 2060 Chiron in the outer Solar System and the recognition of Pluto's relatively low mass, its status as a major planet began to be questioned. ...
Asteroids in retrograde resonance with Jupiter
Asteroids in retrograde resonance with Jupiter

... to ep+q . This reflects the fact that a p/−q retrograde resonance is weaker than its p/q prograde counterpart (whose force is proportional to e|p−q| ) as an encounter of an asteroid and a planet orbiting in opposite directions around the Sun occurs at a higher relative velocity during a shorter time ...
Origin of the orbital architecture of the giant planets of the Solar
Origin of the orbital architecture of the giant planets of the Solar

... Other compact planetary configurations could lead to the crossing of different MMRs. For reasons of completeness, we studied the crossing of the 2:3 and 1:2 MMRs between (1) Saturn and the inner ice giant, and (2) the two ice giants, by placing Saturn exterior to the 1:2 MMR with Jupiter, and varyin ...
Eris is Pluto`s Twin This diagram shows the path of a faint star during
Eris is Pluto`s Twin This diagram shows the path of a faint star during

... “Observing occultations by the tiny bodies beyond Neptune in the Solar System requires great precision and very careful planning. This is the best way to measure Eris’s size, short of actually going there,” explains Bruno Sicardy, the lead author. Observations of the occultation were attempted from ...
Lecture 22 Giant Planets Rings
Lecture 22 Giant Planets Rings

... Christiaan Huygens was the first person to explain the rings (and their disappearance) when in 1659 he worked out that Saturn must be surrounded by a thin flat ring that does not touch the planet. The appearance and disappearance of the rings was due the different viewing geometries as seen from Ear ...
Pluto: Dwarf Planet - ASTR101
Pluto: Dwarf Planet - ASTR101

... and is not Jovian or Terrestrial (like earth) •  Since it has almost all of the same characterisUcs of a planet, except does not have a “neighborhood” cleared around its orbit, it is classified as a TransNeptunian Object (TNO) •  To be a planet it must: be in orbit around the sun; be massiv ...
3rd GradeBook Notes for A Feast of Words…Earth and BeyondUnit
3rd GradeBook Notes for A Feast of Words…Earth and BeyondUnit

... equator – an imaginary line around the center of a moon or a planet, halfway between the north and south poles gravity – a force that pulls two objects together; gravity pulls you down onto Earth orbit – to travel around an object such as a sun or planet rotation – the action of spinning on an axis ...
BIRTH OF CHRIST RECALCULATED Preliminary Considerations
BIRTH OF CHRIST RECALCULATED Preliminary Considerations

... It thus seems highly probable that all in the Empire registered an oath of obedience and an approval of the Pater Patrae to Augustus at this time and that Quirinius had been sent to the East to conduct it. It is reasonable that a period of about a year was allowed for complete enrollment, thus begin ...
A coupling of the origin of asteroid belt, planetary ring
A coupling of the origin of asteroid belt, planetary ring

... planet, and planet around the Sun, run across the solar system back and forth, this gives rise to great bombardment on the objects they encounter, advent of comets when close enough to the Sun, and appearance of meteors when close enough to the Earth, some of the fragments occasionally land on the s ...
Solar System - Manhasset Schools
Solar System - Manhasset Schools

... On average, Pluto is more than 3.6 billion miles (5.8 billion kilometers) away from the sun. That is about 40 times as far from the sun as Earth. Pluto orbits the sun in an oval like a racetrack. Because of its oval orbit, Pluto is sometimes closer to the sun than at other times. At its closest poin ...
margarita2007
margarita2007

... • Merged satellites are more massive and have been accreted earlier than surviving one • Surviving satellites are predominantly low-mass systems and have been accreted recently • The building blocks of the stellar halo were on average more massive and were accreted (and disrupted) earlier than de po ...
ASTR 330: The Solar System
ASTR 330: The Solar System

... • First close flyby of an asteroid (Gaspra) and discovery of first asteroidal moon: Ida’s Dactyl. ...
Lecture 10. Roche Limit / Comets
Lecture 10. Roche Limit / Comets

... rocky meteoroids2. In contrast, a half-rock, half-ice mixture (similar to the composition of many of the satellites in the outer Solar System) would generally be expected. Previous ring origin theories invoke the collisional disruption of a small moon3, 4, or the tidal disruption of a comet during a ...
Hubble observations of Ceres and Pluto:
Hubble observations of Ceres and Pluto:

... to be, but like the unscientific Bode’s Law before it, Percival Lowell’s predictions of a trans-Neptunian “Planet X” were based on flawed calculations of perturbations in Neptune’s orbit. So both Ceres and Pluto were discovered for the wrong reasons, and the flawed predictions led them to be unhesit ...
Moon - mrnicholsscience
Moon - mrnicholsscience

... Planets, moons, dwarf planets and comets Comets are ice, rock, and dust in eccentric orbits. They make a tail when they get closer to the Sun. ...
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Naming of moons

The naming of moons has been the responsibility of the International Astronomical Union's committee for Planetary System Nomenclature since 1973. That committee is known today as the Working Group for Planetary System Nomenclature (WGPSN).Prior to its formation, the names of satellites have had varying histories. The choice of names is often determined by a satellite's discoverer; however, historically some satellites were not given names for many years after their discovery; for instance, Titan was discovered by Huygens in 1655, but was not named until 1847, almost two centuries later.Before the IAU assumed responsibility for astronomical nomenclature, only twenty-five satellites had been given names that were in wide use and are still used. Since then, names have been given to 129 additional satellites: 45 satellites of Jupiter, 43 of Saturn, 22 of Uranus, 11 of Neptune, 5 of Pluto, 1 of Eris, and 2 of Haumea. The number will continue to rise as current satellite discoveries are documented and new satellites are discovered.At the IAU General Assembly in July 2004, the WGPSN suggested it may become advisable to not name small satellites, as CCD technology makes it possible to discover satellites as small as 1 km in diameter. To date, however, names have been applied to all moons discovered, regardless of size.
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