Quiz Outer Planets
... The surface of which of these reveals grooved regions with occasional fault cutting across the grooves, suggesting the upwelling of molten material through a frozen surface early in the history of the solar system? a. Titan. b. Venus. c. Ganymede. d. Europa. answer: c ...
... The surface of which of these reveals grooved regions with occasional fault cutting across the grooves, suggesting the upwelling of molten material through a frozen surface early in the history of the solar system? a. Titan. b. Venus. c. Ganymede. d. Europa. answer: c ...
the outer planets, their satellites and the plutoids
... 37. __________ is a satellite of Saturn with one light and one dark side. 38. Saturn’s satellite __________ is a small black-surfaced object in retrograde orbit. 39. __________ __________ can help confine rings to a narrow zone. 40. The planet __________ was discovered by its gravitational effec ...
... 37. __________ is a satellite of Saturn with one light and one dark side. 38. Saturn’s satellite __________ is a small black-surfaced object in retrograde orbit. 39. __________ __________ can help confine rings to a narrow zone. 40. The planet __________ was discovered by its gravitational effec ...
Why are the Jovian Planets so Different?
... Why are the Jovian Planets so Different? • They formed beyond the frost line to form large, icy planetesimals which were massive enough to… – Capture H/He far from Sun to form gaseous planets. – Each Jovian planet formed its own “miniature” solar nebula. – Moons formed out of these disks. ...
... Why are the Jovian Planets so Different? • They formed beyond the frost line to form large, icy planetesimals which were massive enough to… – Capture H/He far from Sun to form gaseous planets. – Each Jovian planet formed its own “miniature” solar nebula. – Moons formed out of these disks. ...
Jupiter`s ring
... All are much larger than the terrestrial planets, have thick atmospheres, but are very inhospitable: ...
... All are much larger than the terrestrial planets, have thick atmospheres, but are very inhospitable: ...
PPT
... Why are the Jovian Planets so Different? • They formed beyond the frost line to form large, icy planetesimals which were massive enough to… – Capture H/He far from Sun to form gaseous planets. – Each Jovian planet formed its own “miniature” solar nebula. – Moons formed out of these disks. ...
... Why are the Jovian Planets so Different? • They formed beyond the frost line to form large, icy planetesimals which were massive enough to… – Capture H/He far from Sun to form gaseous planets. – Each Jovian planet formed its own “miniature” solar nebula. – Moons formed out of these disks. ...
Planetary Puzzle - Espace pour la vie
... ★ Which planet did the Russian pilot’s spacecraft take off from? Important Before starting your mission, research the following: ...
... ★ Which planet did the Russian pilot’s spacecraft take off from? Important Before starting your mission, research the following: ...
The Revolution of the Moons of Jupiter
... Therefore, the perpendicular distance of the moon should be a sinusoidal curve if you plot it versus time (see Figure 2). By taking enough measurements of the position of a moon, you can fit a sine curve to the data and determine the radius of the orbit (the amplitude of the sine curve) and the peri ...
... Therefore, the perpendicular distance of the moon should be a sinusoidal curve if you plot it versus time (see Figure 2). By taking enough measurements of the position of a moon, you can fit a sine curve to the data and determine the radius of the orbit (the amplitude of the sine curve) and the peri ...
Lecture18
... • Tidal friction on the Moon (caused by Earth) has slowed its rotation down to a period of one month. • The Moon now rotates synchronously. – We always see the same side of the Moon. • Tidal friction on the Moon has ceased since its tidal bulges are always aligned with Earth. ...
... • Tidal friction on the Moon (caused by Earth) has slowed its rotation down to a period of one month. • The Moon now rotates synchronously. – We always see the same side of the Moon. • Tidal friction on the Moon has ceased since its tidal bulges are always aligned with Earth. ...
HOW PLANETARY MAGNETOSPHERES HAVE AND CAN
... future exploration of the solar system and our understanding of solar systems beyond our own. In the next decade NASA and ESA have planned detailed exploration of the Jovian magnetosphere, specifically its moons Europa and Ganymede. Currently the Juno mission is undergoing detailed mapping of Jupite ...
... future exploration of the solar system and our understanding of solar systems beyond our own. In the next decade NASA and ESA have planned detailed exploration of the Jovian magnetosphere, specifically its moons Europa and Ganymede. Currently the Juno mission is undergoing detailed mapping of Jupite ...
Lecture 1
... D. Jupiter's rotation is slowing down dramatically, and this slowdown releases energy E. All of the above are the energy sources ...
... D. Jupiter's rotation is slowing down dramatically, and this slowdown releases energy E. All of the above are the energy sources ...
Jupiter, Saturn, Uranus, and Neptune
... about 30,000 km above its atmosphere to about twice Saturn’s radius (136,000 km) – Faint rings can be seen closer to Saturn as well as farther ...
... about 30,000 km above its atmosphere to about twice Saturn’s radius (136,000 km) – Faint rings can be seen closer to Saturn as well as farther ...
Explain why the jovian planets are so much different
... accretion rates went much faster for Jupiter and decreased outward toward the more spreadout regions. By the time the solar wind blew the gas away, Jupiter had had more time to accrete so it grew the largest. Compare the atmospheres of the jovian planets including defining charac ...
... accretion rates went much faster for Jupiter and decreased outward toward the more spreadout regions. By the time the solar wind blew the gas away, Jupiter had had more time to accrete so it grew the largest. Compare the atmospheres of the jovian planets including defining charac ...
The Jovian Planets
... The top of the deepest cloud layer, which is not visible to us, lies 80 km below the troposphere. In 1995, Galileo probe arrived at Jupiter. Galileo survived in the atmosphere for about an hour before being crushed by atmospheric pressure at an altitude of 150 km below the troposphere. Galileo’s fin ...
... The top of the deepest cloud layer, which is not visible to us, lies 80 km below the troposphere. In 1995, Galileo probe arrived at Jupiter. Galileo survived in the atmosphere for about an hour before being crushed by atmospheric pressure at an altitude of 150 km below the troposphere. Galileo’s fin ...
Lecture13: Jovian Planets
... rotation (pulling mass outward) against gravity (pulling mass inward). dense core => strong gravity => small oblateness. o Complicated models of mass distribution are built to fit the observed oblateness. o Saturn’s internal structure is similar to that of Jupiter, but with a larger rocky core (by ...
... rotation (pulling mass outward) against gravity (pulling mass inward). dense core => strong gravity => small oblateness. o Complicated models of mass distribution are built to fit the observed oblateness. o Saturn’s internal structure is similar to that of Jupiter, but with a larger rocky core (by ...
Earth 110 – Exploration of the Solar System Assignment 5
... atmospheres prevent spacecraft from reaching any kind of surface, if they have one, and can generate storms 2-3 times the size of Earth. They have many moons ranging in size from terrestrial planets (one of which has a thick atmosphere!) to small asteroids. Their rings, while appearing delicate or f ...
... atmospheres prevent spacecraft from reaching any kind of surface, if they have one, and can generate storms 2-3 times the size of Earth. They have many moons ranging in size from terrestrial planets (one of which has a thick atmosphere!) to small asteroids. Their rings, while appearing delicate or f ...
Earth 110 – Exploration of the Solar System Assignment 4
... expensive, and more risky (not to mention the amount of time it takes to travel out there), but necessary in order to study them. Missions to the outer solar system mostly consist of flybys. However, Jupiter has had one orbiter (Galileo), with another on the way (Juno), and Saturn has had one orbite ...
... expensive, and more risky (not to mention the amount of time it takes to travel out there), but necessary in order to study them. Missions to the outer solar system mostly consist of flybys. However, Jupiter has had one orbiter (Galileo), with another on the way (Juno), and Saturn has had one orbite ...
The Outer Planets - Duplin County Schools
... However, its atmosphere, composition, and internal structure are thought to be remarkably similar to Jupiter’s The most prominent feature of Saturn is its system of rings ...
... However, its atmosphere, composition, and internal structure are thought to be remarkably similar to Jupiter’s The most prominent feature of Saturn is its system of rings ...
Chapter 9
... 30,000 km above its atmosphere to about twice Saturn’s radius (136,000 km) – Faint rings can be seen closer to Saturn as well as farther away – Thickness of rings: a few ...
... 30,000 km above its atmosphere to about twice Saturn’s radius (136,000 km) – Faint rings can be seen closer to Saturn as well as farther away – Thickness of rings: a few ...
Chapter 9
... • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge supports the idea that the ...
... • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge supports the idea that the ...
jupiter 1
... lifts them out of the ring plane. As a result, dust is continuously swept away, but is replenished by new particles eroded from the small satellites. ...
... lifts them out of the ring plane. As a result, dust is continuously swept away, but is replenished by new particles eroded from the small satellites. ...
Ch10_Lecture
... • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge supports the idea that the ...
... • With a density of 1.2 g/cm3 and smaller size, Uranus must contain proportionally fewer light elements than Jupiter/Saturn • Density is too low for it to contain much rock or iron • Uranus’s interior probably contains water, methane, and ammonia • Size of equatorial bulge supports the idea that the ...
Chapter 10 The Outer Worlds… Jupiter Jupiter Jupiter`s Interior
... • Triton’s orbit is “backwards” and is highly tilted with respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at ...
... • Triton’s orbit is “backwards” and is highly tilted with respect to Neptune’s equator – Triton is perhaps a captured planetesimal from the Kuiper belt • Triton is large enough and far enough from the planet to retain an atmosphere • Triton has some craters with dark steaks extending from them – at ...
Juno (spacecraft)
Juno is a NASA New Frontiers mission to the planet Jupiter. Juno was launched from Cape Canaveral Air Force Station on 5 August 2011 and will arrive on 4 July 2016. The spacecraft is to be placed in a polar orbit to study Jupiter's composition, gravity field, magnetic field, and polar magnetosphere. Juno will also search for clues about how the planet formed, including whether it has a rocky core, the amount of water present within the deep atmosphere, how its mass is distributed, and its deep winds, which can reach speeds of 618 kilometers per hour (384 mph).The spacecraft's name comes from Greco-Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief, but his wife, the goddess Juno, was able to peer through the clouds and see Jupiter's true nature.