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 8, Problem 3TY
To determine
The Doppler shift method is used to detect which one of the following option.
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Which of these views cannot be used when trying to
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none of these can be observed using the radial velocity
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Which of the systems above could not be detected using the transit
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If you could visit another planetary system while the planets are forming, would you expect to see the condensation sequence at work, or do you think that process was most likely unique to our Solar System? How do the properties of the extrasolar planets discovered so far affect your answer?
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If the solar nebula hypothesis is correct, do you think there are more planets in the Universe than stars? Why or why not?
H5.
A star with mass 1.05 M has a luminosity of 4.49 × 1026 W and effective temperature of 5700 K. It dims to 4.42 × 1026 W every 1.39 Earth days due to a transiting exoplanet. The duration of the transit reveals that the exoplanet orbits at a distance of 0.0617 AU. Based on this information, calculate the radius of the planet (expressed in Jupiter radii) and the minimum inclination of its orbit to our line of sight.
Follow up observations of the star in part reveal that a spectral feature with a rest wavelength of 656 nm is redshifted by 1.41×10−3 nm with the same period as the observed transit. Assuming a circular orbit what can be inferred about the planet’s mass (expressed in Jupiter masses)?
Chapter 8 Solutions
Loose Leaf For Explorations: Introduction To Astronomy
Ch. 8 - Name the eight planets in order of increasing...Ch. 8 - (8.1) What is Pluto, and why isnt it a planet?Ch. 8 - Where are the asteroid belt, the Kuiper belt, and...Ch. 8 - Prob. 4QFRCh. 8 - Prob. 5QFRCh. 8 - Prob. 6QFRCh. 8 - What properties, apart from position, distinguish...Ch. 8 - How old is the Solar System? How do we know?Ch. 8 - Prob. 9QFRCh. 8 - Prob. 10QFR
Ch. 8 - Prob. 11QFRCh. 8 - Prob. 12QFRCh. 8 - Prob. 13QFRCh. 8 - Prob. 14QFRCh. 8 - Prob. 15QFRCh. 8 - Prob. 16QFRCh. 8 - Prob. 17QFRCh. 8 - Prob. 18QFRCh. 8 - Prob. 19QFRCh. 8 - Prob. 20QFRCh. 8 - Prob. 21QFRCh. 8 - Prob. 22QFRCh. 8 - Prob. 1TQCh. 8 - Prob. 2TQCh. 8 - Prob. 3TQCh. 8 - Prob. 4TQCh. 8 - By what factor would the Sun be shrunk to be the...Ch. 8 - (8.1) Calculate the densities of Venus and Jupiter...Ch. 8 - Look up the masses and radii of Mercury and...Ch. 8 - Prob. 4PCh. 8 - Prob. 5PCh. 8 - Prob. 6PCh. 8 - Prob. 7PCh. 8 - Prob. 8PCh. 8 - Prob. 1TYCh. 8 - Prob. 2TYCh. 8 - Prob. 3TYCh. 8 - Prob. 4TYCh. 8 - Prob. 5TYCh. 8 - The numerous craters we see on the solid surfaces...Ch. 8 - Prob. 7TY
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- When astronomers found the first giant planets with orbits of only a few days, they did not know whether those planets were gaseous and liquid like Jupiter or rocky like Mercury. The observations of HD 209458 settled this question because observations of the transit of the star by this planet made it possible to determine the radius of the planet. Use the data given in the text to estimate the density of this planet, and then use that information to explain why it must be a gas giant.arrow_forwardList three ways in which the exoplanets we have detected have been found to be different from planets in our solar system.arrow_forwardWhere would you look for some “original” planetesimals left over from the formation of our solar system?arrow_forward
- Describe the solar nebula, and outline the sequence of events within the nebula that gave rise to the planetesimals.arrow_forwardWhat is an exoplanet? Group of answer choices A planet in our solar system beyond Pluto. Any planet with extra-terrestrial life. A planet in an extra-solar star system outside of our solar system. Objects in the solar system such as Pluto that were once considered planets but no longer are.arrow_forwardDescribe the Doppler Method of searching for exoplanets.arrow_forward
- 9) An interstellar cloud fragment 0.2 light-year in diameter is rotating at a rate of one revolution per million years. It now begins to collapse. Assuming that the mass remains constant, estimate the cloud's rotation period when it has shrunk to (a) the size of the solar nebula, 100 AU across, and (b) the size of Earth's orbit, 2 AU across. (answers: 0.016 revolutions per year, and an orbital period of 62.5 years, This is 40 revolutions per year, and an orbital period of 0.025 years, or just a little over 9 days)arrow_forwardPlanetary migration is a new process that has been added to the nebular theory of solar system formation. What type of planet, that does not exist in our solar system, made this change to the theory necessary? super-Earths Jovian planets beyond the "frost line" mini-Neptunes O hot Jupiters terrestrial planets in the habitable zonearrow_forwardThe search for extrasolar planets fall broadly into two categories, what are they? Lensing and transits Astrometry and Doppler shifts Speckle imaging and interferometry Dust emission and radio bursts Direct and indirect detectionarrow_forward
- If Exoplanets A and B are orbiting their host stars at similar distances and we know that the host star for exoplanet A emits peak radiation at 400 nm, while the radiation at exoplanet B’s star peaks at 1920 nm, in the absence of other information, which exoplanet would be warmer, and why?arrow_forwardPlease help me with this question. A=.2arrow_forwardWhat is the exoplanet doing when the light we detect from the star begins to increase from the least amount of light to the greatest amount of light?arrow_forward
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