Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 12, Problem 36Q
To determine
The reason why the two intervals between the successive edge-on presentations of Saturn's rings are not equal, where one is about 13 years 9 months and the other is about 15 years 9 months..
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Jupiter's moons have angular separations on the order of a dozen arcminutes. Does this correspond to more or less than one degree?
Jupiter's moons have angular separations on the order of a dozen arcminutes. Does this correspond to more or less than one degree?
Group of answer choices
- Less than one degree
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Chapter 12 Solutions
Universe
Ch. 12 - Prob. 1CCCh. 12 - Prob. 2CCCh. 12 - Prob. 3CCCh. 12 - Prob. 4CCCh. 12 - Prob. 5CCCh. 12 - Prob. 6CCCh. 12 - Prob. 7CCCh. 12 - Prob. 8CCCh. 12 - Prob. 9CCCh. 12 - Prob. 10CC
Ch. 12 - Prob. 11CCCh. 12 - Prob. 1QCh. 12 - Prob. 2QCh. 12 - Prob. 3QCh. 12 - Prob. 4QCh. 12 - Prob. 5QCh. 12 - Prob. 6QCh. 12 - Prob. 7QCh. 12 - Prob. 8QCh. 12 - Prob. 9QCh. 12 - Prob. 10QCh. 12 - Prob. 11QCh. 12 - Prob. 12QCh. 12 - Prob. 13QCh. 12 - Prob. 14QCh. 12 - Prob. 15QCh. 12 - Prob. 16QCh. 12 - Prob. 17QCh. 12 - Prob. 18QCh. 12 - Prob. 19QCh. 12 - Prob. 20QCh. 12 - Prob. 21QCh. 12 - Prob. 22QCh. 12 - Prob. 23QCh. 12 - Prob. 24QCh. 12 - Prob. 25QCh. 12 - Prob. 26QCh. 12 - Prob. 27QCh. 12 - Prob. 28QCh. 12 - Prob. 29QCh. 12 - Prob. 30QCh. 12 - Prob. 31QCh. 12 - Prob. 33QCh. 12 - Prob. 34QCh. 12 - Prob. 35QCh. 12 - Prob. 36QCh. 12 - Prob. 37QCh. 12 - Prob. 38QCh. 12 - Prob. 39QCh. 12 - Prob. 40QCh. 12 - Prob. 41QCh. 12 - Prob. 42QCh. 12 - Prob. 43QCh. 12 - Prob. 44QCh. 12 - Prob. 45QCh. 12 - Prob. 46QCh. 12 - Prob. 47QCh. 12 - Prob. 48QCh. 12 - Prob. 49QCh. 12 - Prob. 50QCh. 12 - Prob. 51QCh. 12 - Prob. 52QCh. 12 - Prob. 53QCh. 12 - Prob. 54QCh. 12 - Prob. 55QCh. 12 - Prob. 56QCh. 12 - Prob. 57QCh. 12 - Prob. 58QCh. 12 - Prob. 59Q
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Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.Similar questions
- How deep would be the eclipse caused by Jupiter transiting in front of the Solar disk, as observed from a distant star?arrow_forwardThe value we have just calculated is the combined masses of Jupiter and Callisto! Their mass is in units of the Sun's Mass (MS) - we can convert this to units which are more familiar to us like kilograms by multiplying this answer by the scale factor (1.99x1030 kg/1 MS): (MJupiter + MCallisto) = ( MS) (1.99x1030 kg/1 Solar Mass) = _______x_10___ kg (I have already written the x 10 so you are reminded to write the exponenet of 10 in the scientific notation expression of your answer). Since you know from looking at pictures of Jupiter with its Galilean Satellites (look in your book at a picture if you have not already), that Callisto is much smaller than Jupiter - in fact it is less than 0.001 of Jupiter's size or mass, so the number we have just calculated for (MJupiter + MCallisto) is almost the same as MJupiter . How much more massive is Jupiter than the Earth? (The mass of Earth is about 5.98 x 1024 kg)arrow_forwardExplain the tidal hypothesis.arrow_forward
- Which would have the longer orbital period: a moon 1 million km from the center of Jupiter, or a moon 1 million km from the center of Earth? Why?arrow_forwardWhich is the phase of Venus when it is closest? Which when farthest? How do you know?arrow_forwardThe day on Mars is 1.026 Earth-days long. The martian year lasts 686.98 Earth-days. The two moons of Mars take 0.32 Earth-day (for Phobos) and 1.26 Earth-days (for Deimos) to circle the planet. You are given the task of coming up with a martian calendar for a new Mars colony. Would a solar or lunar calendar be better for tracking the seasons?arrow_forward
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- The diameter of the earth’s moon is 2195 miles. The diameter of Jupiter is 86881 miles. How many of earth’s moons could fit across the diameter of Jupiter? Round your answer to the nearest whole number.arrow_forwardAn asteroid is observed to be on a superior orbit with a synodic period of 466.6 days. What are the sidereal orbital period and semi-major axis of this asteroid? Choose the option below that most closely matches your answers. Select one: O a. Sidereal period = 1683 days and %3D semi-major = 2.7 AU O b. Sidereal period = 1683 days and semi-major axis = 4.8 AU O c. Sidereal period = 865 days and semi- major axis = 1.8 AU O d. Sidereal period = 426 day and semi- %3D major axis = 2.7 AU O e. Sidereal period = 1727 days and е. semi-major axis = 0.8 AUarrow_forward1 of 1 Celestial Profile: SATURN Table A-11 Principal Satellites of the Solar System Distance from Orbital Period Orbital Orbital Primary Satellite Radius (km) Primary (10' km) days Eccentkity Inclination" МOTION Esrth Moon 3614 272 OSS Average distance from the Sun Eccentricity of orbit Inclination of orbit to ecliptic Orbital period Rotation period (sidereal) 14 X 12 x 10 9.58 AU (143 x 10° km) Mars Prebos 94 Lleimos 235 126 Aalh 0.056 lupelet 135 X 1x lo 1820 422 177 2.5° Europe 15NI 29.5 y Grymede 3630 1001 Caleto 2M10 1884 10.57 h 11A Satun Janus 110 x 80 x 100 151.5 0.70 Inclination of equator to orbit 26,7° 196 185.5 15 Enceladus 250 2380 137 Tethys 530 2917 CHARACTERISTICS Dure 550 377 24 Rhea 527 452 Equatorial diameter 1.21 X 10 km (9.45 De 5.68 X 1025 kg (95.2 Ma) 0.69 g/cm 1.1 Earth gravities Tite 1222 Hyperion 203 X 110 X 1o 1454 2128 0.104 Mass Lapetir 20 356 Phocte 106 12.900 0.163 190 Average density Gravity at cloud tops Escape velocity Temperature at cloud tops Uans…arrow_forward
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