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Inti didn`t form in the X wind (and neither did most CAIs)
Inti didn`t form in the X wind (and neither did most CAIs)

... within lifetime of disk, while H and He gas are available to accrete (Lissauer & Stewart 1993). Underlying assumption of MMSN - that planets’ current orbits reflect where mass was in the solar nebula - is wrong! Planets migrated! (Fernandez & Ip 1984; Malhotra 1993). Turns out, planets migrated a lo ...
The Planets
The Planets

... Jovian planets.  The diameter of the largest terrestrial planet, Earth, is only onequarter the diameter of the smallest Jovian planet, Neptune.  The Jovian planets are often called giants. (also called the outer planets).  The terrestrial planets are closer to the sun and are called the inner pla ...
The Jovian Planets
The Jovian Planets

... At a depth of 80–100 km, predictions indicate the temperature is Earth-like and the pressure is 10 times greater than that at the Earth’s surface. As one goes deeper in Jupiter’s atmosphere, gaseous hydrogen becomes liquid hydrogen (~7,000 km). The pressure here is 500,000 times that of the Earth su ...
In Roman mythology Neptune was the god of the Sea. He is known
In Roman mythology Neptune was the god of the Sea. He is known

... Neptune's rings are very dark and very faint. Scientists still haven't figured out what they are made of yet. Look for Neptune! Neptune can be seen with binoculars (if you know exactly where to look) but a large telescope is needed to see anything other than a tiny disk. ~ Neptune is a giant gas pla ...
PSRD: Dynamics and Chemistry of Planet Construction
PSRD: Dynamics and Chemistry of Planet Construction

... Planetary dynamicists knew that overcoming these problems would require including more planetesimals in the simulations. They reasoned that more planetesimals interacting with planetary embryos would cause more rapid accretion and less elliptical and inclined orbits. The underlying cause is that the ...
Document
Document

... Overview of the Solar System ...
Neptune - Super Teacher Worksheets
Neptune - Super Teacher Worksheets

... the farthest away. (Pluto is even farther, but it doesn’t count since most astronomers no longer consider it a planet.) Neptune is a cold, dark place that’s the smallest of the gas giants. It was named after the Roman god of water and the sea. Neptune is a ball of gas and ice, with a rocky core. Thi ...
- La Salle Elementary School
- La Salle Elementary School

... • Jupiter’s atmosphere is about 90 percent hydrogen and 10 percent helium. • The planet itself is about 80 percent hydrogen and 20 percent helium. • Jupiter is a ball of gas swirling around a thick liquid layer that conceals a solid core. Scientists are not certain what makes up the core. ...
Solar System PPT
Solar System PPT

... • Jupiter’s atmosphere is about 90 percent hydrogen and 10 percent helium. • The planet itself is about 80 percent hydrogen and 20 percent helium. • Jupiter is a ball of gas swirling around a thick liquid layer that conceals a solid core. Scientists are not certain what makes up the core. ...
Lesson 2 - Verona Public Schools
Lesson 2 - Verona Public Schools

... • Jupiter’s atmosphere is about 90 percent hydrogen and 10 percent helium. • The planet itself is about 80 percent hydrogen and 20 percent helium. • Jupiter is a ball of gas swirling around a thick liquid layer that conceals a solid core. Scientists are not certain what makes up the core. ...
CS3_Ch 2 - Leon County Schools
CS3_Ch 2 - Leon County Schools

... • Jupiter’s atmosphere is about 90 percent hydrogen and 10 percent helium. • The planet itself is about 80 percent hydrogen and 20 percent helium. • Jupiter is a ball of gas swirling around a thick liquid layer that conceals a solid core. Scientists are not certain what makes up the core. ...
The Asteroid Belt
The Asteroid Belt

... Asteroid-like objects are believed to have filled the early Solar System. Computer simulations provide evidence that Jupiter’s strong gravity and tidal effects disrupted the orbits of these planetesimals within the asteroid belt. As a result much of this material was ejected from the Solar System.Th ...
Rapid planet formation
Rapid planet formation

... large ‘gas giants’ in our own solar system. Alan Boss is one well-known specialist in extrasolar planet research who has proposed a new theory of gas giant formation.3,4 ...
Voyager
Voyager

... turn up new, small moons, most of which are too small to be spherical. Saturn has at least for 60 moons.)  The smallest of the four larger moons – the Galilean moons – is 5000 times larger than the largest of the smaller moons. The Galilean moons are spherical, while the others are irregular in sha ...
Where in the Solar System Are Smaller Objects Found?
Where in the Solar System Are Smaller Objects Found?

... Most asteroids are found in the asteroid belt. However, asteroids can be found throughout the solar system. Some of these other asteroids may have formed in the asteroid belt and then their orbits changed because they passed too close to Jupiter. A million asteroids in one area seems like a lot. It ...
PHYS178 Planets
PHYS178 Planets

... • Much more cloud activity is seen on Neptune than on Uranus. This is because Uranus lacks a substantial internal heat source. • Interiors and Magnetic Fields of Uranus and Neptune: Both Uranus and Neptune may have a rocky core surrounded by a mantle of water and ammonia. Electric currents in these ...
The Kuiper Belt - UCLA - Earth, Planetary, and Space Sciences
The Kuiper Belt - UCLA - Earth, Planetary, and Space Sciences

... such questioning began to fade when we found a second body in March 1993. This object is as far from the sun as QB 1 but is located on the opposite side of the solar system. During the past three years, several other research groups have joined the effort, and a steady stream of discoveries has ensu ...
Size of the Solar System Quiz Please Do Not Write on This Paper
Size of the Solar System Quiz Please Do Not Write on This Paper

... 2. Mary looked in her science book at a picture of the solar system. The planets were large and colorful but she knew it was NOT an accurate model. Why? a. The planets should have been much FARTHER apart. b. The planets are NOT colorful. They are white. c. We DON’T know exactly what the planets look ...
pdf format
pdf format

... – probably formed by processes similar to those that formed the planets • Object in irregular orbits – probably formed far away and were captured later ...
NEPTUNE*!
NEPTUNE*!

... close to Neptune that they orbit within its ring system ...
Saturn
Saturn

... harvest  Father of Ceres, Jupiter, Pluto, and Neptune  Ruled during the Golden Age of Men  Saturn represents limits of control as it was thought to be the limit of the Solar System ...
Week 5 Lecture
Week 5 Lecture

... their mass locked in a small rocky core. For Jupiter this is 11,000 km in diameter, 8 times Earth’s mass with pressures of 70 million bars. • Saturn’s larger core can be inferred from its higher degree of oblateness (due to lesser gravity). However it would be even more oblate were it not for its he ...
ment, but minimal basin formation between crustal - SwRI
ment, but minimal basin formation between crustal - SwRI

...  How widespread was this lunar LHB? ...
Jupiter and Saturn
Jupiter and Saturn

... of Jupiter and Saturn? 2. What is going on in Jupiter’s Great Red Spot? 3. What is the nature of the multicolored clouds of Jupiter and Saturn? 4. What does the chemical composition of Jupiter’s atmosphere imply about the planet’s origin? 5. How do astronomers know about the deep interiors of Jupite ...
DTU_9e_ch08 - University of San Diego Home Pages
DTU_9e_ch08 - University of San Diego Home Pages

... Jupiter is by far the largest and most massive planet in the solar system. Jupiter and Saturn probably have rocky cores surrounded by a thick layer of liquid metallic hydrogen and an outer layer of ordinary liquid hydrogen and helium. Both planets have an overall chemical composition very similar to ...
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Jumping-Jupiter scenario

The jumping-Jupiter scenario specifies an evolution of giant-planet migration described by the Nice model, in which an ice giant (Uranus, Neptune, or an additional Neptune-mass planet) encounters first Saturn and then Jupiter, causing the step-wise separation of their orbits. The jumping-Jupiter scenario was proposed by Ramon Brasser, Alessandro Morbidelli, Rodney Gomes, Kleomenis Tsiganis, and Harold Levison after their studies revealed that the smooth divergent migration of Jupiter and Saturn resulted in an inner Solar System significantly different from the current Solar System. The sweeping of secular resonances through the inner Solar System during the migration excited the eccentricities of the terrestrial planets beyond current values and left an asteroid belt with an excessive ratio of high- to low-inclination objects. The step-wise separation of Jupiter and Saturn described in the jumping-Jupiter scenario allows these resonances to quickly cross the inner Solar System without altering orbits excessively. The jumping-Jupiter scenario also results in a number of other differences with the original Nice model. The fraction of lunar impactors from asteroid belt during the Late Heavy Bombardment is significantly reduced, most of the Jupiter trojans are captured via an alternative mechanism, and Jupiter acquires its population of irregular satellites via the same process as the other planets. The frequent ejection of an ice giant during simulations of the jumping-Jupiter scenario has led some to propose an additional giant planet in the early Solar System.
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