An Introduction to Physical Science
14th Edition
ISBN: 9781305079137
Author: James Shipman, Jerry D. Wilson, Charles A. Higgins, Omar Torres
Publisher: Cengage Learning
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Textbook Question
Chapter 16, Problem 18MC
Which of the following is not a very useful method for detecting an exoplanet? (16.8)
- (a) the observation of a star’s motion
- (b) the observation of Doppler shifts in the spectrum of a star
- (c) the detection of alien
electromagnetic signals
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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)?
What are the four main challenges that need to be overcome as scientists come together to try to get a probe to an exoplanet
Which of these views cannot be used when trying to
detect exoplanets using the radial velocity method? XYZ
all of these can be observed using the radial velocity
method none of these can be observed using the radial
velocity method?
X
Y
Z
all of these can be observed using the radial velocity
method
none of these can be observed using the radial velocity
method
Figure X
to Earth
Figure Y
to Earth
Figure Z
to Earth
Which of the systems above could not be detected using the transit
method?
Chapter 16 Solutions
An Introduction to Physical Science
Ch. 16.1 - What is the difference between the geocentric...Ch. 16.1 - Prob. 2PQCh. 16.1 - Calculate the period of a planet whose orbit has a...Ch. 16.2 - Prob. 1PQCh. 16.2 - Prob. 2PQCh. 16.3 - Which has the greater albedo, the Earth or the...Ch. 16.3 - Prob. 2PQCh. 16.4 - What makes a planet terrestrial, or pertaining to...Ch. 16.4 - What is the most abundant molecule in the...Ch. 16.5 - Prob. 1PQ
Ch. 16.5 - Prob. 2PQCh. 16.6 - Prob. 1PQCh. 16.6 - Prob. 2PQCh. 16.7 - Prob. 1PQCh. 16.7 - Prob. 2PQCh. 16.8 - Prob. 1PQCh. 16.8 - Prob. 2PQCh. 16 - Prob. AMCh. 16 - Prob. BMCh. 16 - Prob. CMCh. 16 - Prob. DMCh. 16 - Prob. EMCh. 16 - Prob. FMCh. 16 - Prob. GMCh. 16 - Prob. HMCh. 16 - Prob. IMCh. 16 - Prob. JMCh. 16 - Prob. KMCh. 16 - Prob. LMCh. 16 - Prob. MMCh. 16 - Prob. NMCh. 16 - Prob. OMCh. 16 - Prob. PMCh. 16 - Prob. QMCh. 16 - Prob. RMCh. 16 - Prob. SMCh. 16 - Prob. TMCh. 16 - Prob. UMCh. 16 - Prob. VMCh. 16 - Prob. WMCh. 16 - Prob. XMCh. 16 - Prob. 1MCCh. 16 - Which of Keplers laws gives the most direct...Ch. 16 - Which of Keplers laws gives an indication of the...Ch. 16 - Prob. 4MCCh. 16 - Which of the following is abundant on the Earth...Ch. 16 - Prob. 6MCCh. 16 - Prob. 7MCCh. 16 - Which of the following statements concerning the...Ch. 16 - Which of the following is not a physical...Ch. 16 - What are the primary constituents of the Jovian...Ch. 16 - Which of the following is not a physical...Ch. 16 - Which planet has a ring system made of mostly...Ch. 16 - Which Jovian planet revolves on its side and has...Ch. 16 - Which one of the following criteria disqualifies...Ch. 16 - Which statement about the dwarf planet Ceres is...Ch. 16 - Prob. 16MCCh. 16 - Prob. 17MCCh. 16 - Which of the following is not a very useful method...Ch. 16 - ___ is the study of the universe. (Intro)Ch. 16 - Prob. 2FIBCh. 16 - Prob. 3FIBCh. 16 - Prob. 4FIBCh. 16 - Prob. 5FIBCh. 16 - Prob. 6FIBCh. 16 - Prob. 7FIBCh. 16 - The albedo of the Earth is about ___. (16.3)Ch. 16 - Prob. 9FIBCh. 16 - Prob. 10FIBCh. 16 - Prob. 11FIBCh. 16 - Prob. 12FIBCh. 16 - The Jovian planet with retrograde rotation is ___....Ch. 16 - Prob. 14FIBCh. 16 - Prob. 15FIBCh. 16 - Prob. 16FIBCh. 16 - Prob. 17FIBCh. 16 - Prob. 1SACh. 16 - What is the main difference between the...Ch. 16 - Prob. 3SACh. 16 - Prob. 4SACh. 16 - Describe the orientation and the shape of the...Ch. 16 - Prob. 6SACh. 16 - Prob. 7SACh. 16 - Prob. 8SACh. 16 - Prob. 9SACh. 16 - Prob. 10SACh. 16 - Prob. 11SACh. 16 - Prob. 12SACh. 16 - Explain the differences between the Grand Canyon...Ch. 16 - Prob. 14SACh. 16 - Prob. 15SACh. 16 - Which planets axis of rotation is a peculiarity,...Ch. 16 - Prob. 17SACh. 16 - Prob. 18SACh. 16 - Why is Pluto not considered a major planet, and...Ch. 16 - Prob. 20SACh. 16 - Prob. 21SACh. 16 - What was the major influence in the formation of...Ch. 16 - What is astrometry?Ch. 16 - Prob. 24SACh. 16 - Prob. 1VCCh. 16 - Give some reasons our knowledge of the solar...Ch. 16 - A Foucault pendulum suspended from the ceiling of...Ch. 16 - Prob. 3AYKCh. 16 - Explain how the scientific method was used to...Ch. 16 - How does the solar nebula theory explain the...Ch. 16 - Calculate the period T of a planet whose orbit has...Ch. 16 - Calculate the period T of a dwarf planet whose...Ch. 16 - Calculate the length R of the semimajor axis of a...Ch. 16 - Calculate the length R of the semimajor axis of a...Ch. 16 - Determine what the period of revolution of the...Ch. 16 - Determine what the period of revolution of the...Ch. 16 - Asteroids are believed to be material that never...Ch. 16 - Show that the asteroid belt lies between Mars and...Ch. 16 - Use Keplers third law to show that the closer a...Ch. 16 - Prob. 10ECh. 16 - Prob. 11ECh. 16 - List the Jovian planets in order of increasing...
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- Describe the solar nebula, and outline the sequence of events within the nebula that gave rise to the planetesimals.arrow_forwardThe graph below shows how the brightness of a star changes over time due to the fact that it is orbited by an exoplanet. How does the exoplanet’s orbital period around its star compare to the orbital period of the Earth around the Sun?arrow_forwardUse this light curve of a star with a transiting exoplanet to answer the following. If the exoplanet is orbiting a star identical to our own Sun, what is its average orbital distance, in AU? What is the period in years of the transiting exoplanet? Use this light curve of a star with a transiting exoplanet to answer the following questions. Brightness 0 V V V B 5 10 15 20 Time (months) 25 30 35arrow_forward
- Describe the Doppler Method of searching for exoplanets.arrow_forwardWhich is these facts is NOT explained by the nebular theory? There are two main types of planets: terrestrial and jovian Existance of comets and asteroids Planets orbit in the same direction and plane Number of planets of each type (4 terrestrial and 4 jovian)arrow_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
- List three ways in which the exoplanets we have detected have been found to be different from planets in our solar system.arrow_forwardList any similarities between discovered exoplanets and planets in our solar system.arrow_forwardIf a star must remain on the main sequence for at least 4 billion years for life to evolve to intelligence, what is the most massive a star that can form and still possibly harbor intelligent life on one of its exoplanets? (Hints: Use the formula for stellar life expectancies, Eq. 121, and data in Appendix Table A-7.)arrow_forward
- The certain forest moon travels in an approximately circular orbit of radius 14,733,533 m with a period of 11 days 13 hr, around its gas giant exoplanet host. Calculate the mass of the exoplanet from this information. (Units: kilograms) (Note: if 'numerical answers only' appears, type your answer in the form '12.67e7' or '12.67e+7' with a lower case e instead of 'x10^7')arrow_forwardIs there an exoplanet detection method that works better with detecting exoplanets that are at a large distance from their host star? a) none b) radial velocity method c) direct detection d) transit methodarrow_forward9) 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_forward
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