An Introduction to Physical Science
14th Edition
ISBN: 9781305079120
Author: James Shipman, Jerry D. Wilson, Charles A. Higgins, Omar Torres
Publisher: Brooks Cole
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Chapter 16, Problem 17FIB
To determine
To fill in the blank: The method used to detect an exoplanet passing in front of its parent star.
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Students have asked these similar questions
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?
While doing a transit study, you find an exoplanet around a nearby Sun-like star. The time between transits is P= 32days. During a transit, the time from first to second contact is t2−t1= 30minutes, and the time from fist to third contact is t3−t1= 5hours. The depth of the transit is δF/F= 0.01. During follow-up radial velocity measurements of the star, you find that its peak radial velocity is vr= 65m s−1. What is the radius of the planet? What is the mass of the planet? What is the semimajor axis of the planet’s orbit?
Use 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
35
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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- 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)?arrow_forwardIf a transit depth of 0.001 (or 0.1% decrease in brightness) is detected for a star with a radius of 0.3 RSun, what would the radius of the exoplanet be in units of RSun?arrow_forwardConsider the attached light curve for a transiting planet observed by the Kepler mission. If the host star is identical to the sun, what is the radius of this planet? Give your answer in terms of the radius of Jupiter. Brightness of Star Residual Flux 0.99 0.98 0.97 0.006 0.002 0.000 -8-881 -0.06 -0.04 -0.02 0.00 Time (days) → 0.02 0.04 0.06arrow_forward
- The 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_forwardWhat are the four main challenges that need to be overcome as scientists come together to try to get a probe to an exoplanetarrow_forwardWhich of the following is not a very useful method for detecting an exoplanet? (16.8) (a) the observation of a stars motion (b) the observation of Doppler shifts in the spectrum of a star (c) the detection of alien electromagnetic signalsarrow_forward
- What appears to be the most common size of exoplanets? Jupiter size Neptune size Mini-Neptune size Earth and super-Earth size.arrow_forwardAs the amount of light observed from the star rises, what is the exoplanet doing in response?arrow_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
- 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_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_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_forward
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