Loose Leaf For Explorations: Introduction To Astronomy
9th Edition
ISBN: 9781260432145
Author: Thomas T Arny, Stephen E Schneider Professor
Publisher: McGraw-Hill Education
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Chapter 10, Problem 2TY
To determine
The composition of the inner core of Jupiter.
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According to the chart below, how do the gas giants differ from the terrestrial planets?
THE TERRESTRIAL PLANETS
THE GAS GIANTS
MERCURY
MARS
JUPITER
SATURN
URANUS
NEPTUNE
VENUS
EARTH
ROCK
ROCK
ROCK
ROCK
INNER
CORE
INNER
CORE
CORE
SIren/
Nickel
CORE
Iron/
WATER
WATER
WATER
Nickel
OUTER
CORE
OUTER
CORE
METALLIC
U HYDROGEN
METALLIC
WATER
MANTLE
Reck
HYDROGEN
MANTLE
Rock
MANTLE
Reck
CORE
SIren/
Silicates
Silicates
Silicates
Nickel
HYDROGEN
GAS
HYDROGEN
GAS
HYDROGEN
HYDROGEN
GAS
GAS
SURFACE
SURFACE
SURFACE
SURFACE
O The gas giants do not have solid surfaces.
O The gas giants have an iron core.
O The gas giants lack hydrogen gas.
O The gas giants do not contain water.
Which of these things did the Voyager spacecraft discover about Enceladus in the early 1980s, indicating that it is somewhat unusual among planetary bodies in our solar system? Check the TWO items that apply.
a It has a thick atmosphere, made mostly of nitrogen.
b It has the darkest, least reflective surface of all the known planetary bodies.
c It is the brightest (i.e. most reflective) object in the solar system.
d The entire surface is more heavily-cratered than any other body in our solar system.
e Its surface is very smooth in some places.
The narrowness of the rings of Uranus and Neptune is believed to be caused by
a.
gravitational interactions between ring particles.
b.
a spiral density wave which confines them.
c.
the magnetic field which holds them in place.
d.
the smaller mass of Uranus and Neptune as compared to that of Saturn.
e.
small shepherd moons that orbit near the rings.
Chapter 10 Solutions
Loose Leaf For Explorations: Introduction To Astronomy
Ch. 10 - Prob. 1QFRCh. 10 - What does Jupiter look like?Ch. 10 - How do astronomers know what lies inside the outer...Ch. 10 - What are the major gaseous substances that make up...Ch. 10 - What is the interior structure of Jupiter and...Ch. 10 - Do Jupiter and Saturn have solid surfaces?Ch. 10 - Prob. 7QFRCh. 10 - Prob. 8QFRCh. 10 - What sort of activity has been seen on Io? What is...Ch. 10 - What are the rings of Saturn made of? How do...
Ch. 10 - Prob. 11QFRCh. 10 - Prob. 12QFRCh. 10 - Prob. 13QFRCh. 10 - What is unusual about Uranuss rotation axis? What...Ch. 10 - Prob. 15QFRCh. 10 - Why are Uranus and Neptune so blue?Ch. 10 - Why are the outer planets so large?Ch. 10 - Prob. 18QFRCh. 10 - Prob. 1TQCh. 10 - Prob. 2TQCh. 10 - Ganymede and Callisto orbiting Jupiter and Tethys...Ch. 10 - Approximate the Roche limit as 2.44 times a...Ch. 10 - Prob. 5TQCh. 10 - (10.3) Is Uranuss sky blue for the same reason our...Ch. 10 - Prob. 7TQCh. 10 - Prob. 8TQCh. 10 - Prob. 9TQCh. 10 - Prob. 10TQCh. 10 - Prob. 1PCh. 10 - Prob. 2PCh. 10 - Prob. 3PCh. 10 - Prob. 4PCh. 10 - Prob. 5PCh. 10 - Prob. 6PCh. 10 - Prob. 7PCh. 10 - Prob. 8PCh. 10 - (10.1) The low average densities of Jupiter and...Ch. 10 - Prob. 2TYCh. 10 - Prob. 3TYCh. 10 - Prob. 4TYCh. 10 - Prob. 5TYCh. 10 - Prob. 6TYCh. 10 - Prob. 7TY
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- Jupiter is denser than water, yet composed for the most part of two light gases, hydrogen and helium. What makes Jupiter as dense as it is?arrow_forwardJupiter is slightly larger than Saturn but its density is about 2 times the density of Saturn. The reason for this density difference is a. Jupiter's higher mass and gravity compress its interior more b. Jupiter is more compressed by Sun's gravity c. Jupiter has larger volume d. Jupiter has larger proportions of rocks and metalarrow_forwardWhich of these is an example of an energy source that could exist on Europa (or beneath its surface) and help enable life in a Europan ocean? a Volcanoes and/or hydrothermal vents on the seafloor b Solar flares from the Sun that penetrate Europa's ice and send radiation into the liquid-water ocean c Europa's rapid motion as it orbits Jupiter d The combustion of fossils fuels beneath the surface, similar to burning coal in the Earth's crustarrow_forward
- How many times more pressure exists in the interior of Jupiter compared to that of Earth?arrow_forwardGM What is the orbital velocity and period of a ring particle at the outer edge of Saturn's A ring? (Note: The radius of the edge of the A ring is 136,500 km. Hint: Use the formula for orbital velocity, V. = v orbital velocity km/s period hrarrow_forwardThe Great Red Patch is the term given to the enormous red area on Jupiter's surface. Are there any predictions on how long it will take the planet to complete its rotation?arrow_forward
- Imagine that astronomers have just discovered a planet orbiting another star (other than the Sun), and they have reported the mass of the planet as 4.2 Jupiter-masses. Explain in a few words what this means.arrow_forwardcalculate the density of jupiterarrow_forwardEarth-based telescopic observations of Neptune reveal a. a bluish-green disk with no visible surface detail. b. white clouds and a dark blue spot. c. belt-zone circulation as seen on Jupiter and Saturn. d. rapidly rising and sinking convection currents of different shades of blue. e. cyclonic storms near the planet’s equator.arrow_forward
- Describe the process through which the terrestrial planets and the planets of Jupiter diverged so drastically.arrow_forwardWhat is the range of density for the outer planets (in g/cm3)? 1.2 to 5.5 2.2 to 5.5 2.2 to 6.5 3.3 to 7.2 none of thesearrow_forwardWhich one of the mechanism below can NOT be responsible for providing intrinsic luminosity for planets? Gravitational settling of the hydrogen molecules. Gravitational settling of the helium atoms. Residual heat dating from the formation epoch of the planets. Decay of radio-active isotopes like uranium.arrow_forward
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