Astro 3 Midterm 2 Study Guide PDF
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This document is a study guide for a midterm exam in an introductory astronomy course. It covers various topics relating to planetary science, including the interiors, surfaces, atmospheres, and characteristics of various celestial bodies within the solar system. It also touches upon extrasolar planets, the Sun, and other stellar phenomena.
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Astro 3: Study Guide for Midterm #2 Reading: Chapters 7, 8, 9, 10, 11, 12, 13 Topics: Terrestrial planets Jovian planets Pluto Asteroids/Comets Extrasolar planets The Sun Measurements of the stars Stellar life cycles 1. Terrestrial Planets...
Astro 3: Study Guide for Midterm #2 Reading: Chapters 7, 8, 9, 10, 11, 12, 13 Topics: Terrestrial planets Jovian planets Pluto Asteroids/Comets Extrasolar planets The Sun Measurements of the stars Stellar life cycles 1. Terrestrial Planets o What are the different layers of a terrestrial planet interior? o What does the size of the lithosphere determine? o What factors determine geological activity? o What are sources of internal heat in terrestrial planets? o How do the geological activity on the Earth and the Moon compare? o What about Venus vs. Mercury? o What does heat travel from the interior of a terrestrial planet to its surface? o Why are larger terrestrial planets hotter? o How are surface area and volume related for a sphere? o Which terrestrial planet has the strongest magnetic field? o What are the processes that shape terrestrial planet surfaces? o How can cratering be used to gauge the age of a terrestrial planet's surface? o How are volcanism and erosion related? o What is an atmosphere? o What impact does an atmosphere have on a terrestrial planet's surface temperature? o Which terrestrial planet has the thickest atmosphere (in terms of atmospheric pressure)? The thinnest atmosphere? o What is the composition of Earth's atmosphere? o What is the greenhouse effect? o What are greenhouse gases? 2. Jovian planets o What is the composition of Jupiter and Saturn? o What is the composition of Uranus and Neptune? o How do the densities of Jupiter and Saturn compare? o Why is Jupiter denser than Saturn? o Why are Uranus and Neptune denser than Saturn? o Why do Uranus and Neptune have a different composition from that of Jupiter and Saturn? o What are the interior structures of the Jovian planets? o Why do Uranus and Neptune have a bluish atmosphere? o What gives rise to the banded atmospheres on Jupiter and Saturn? o What is the origin of the large Jovian moons? o What evidence supports the picture of the large moon origin? o What is one exception to this scenario? o What is the origin of the small Jovian moons? o What evidence supports the picture of the small moon origin? o What are the Galilean moons and the important characteristics of each? o What is a tidal force? o What is special about Saturn's moon Titan? o What is special about Saturn's moon Enceladus? o Do Jovian moons show evidence for geological activity? o Which jovian planets have ring systems? o What is the thickness of Saturn's ring system? o What is the likely origin of Saturn's ring system? 3. Pluto o How is Pluto’s orbit distinct from that of the 8 planets of the solar system? o How do Pluto’s properties make it an exception to the rules of terrestrial vs. jovian planets? o Which satellite mission made the closest approach to Pluto? o Does Pluto’s surface show evidence of geological activity? 4. Asteroids/Comets o Where is the asteroid belt located? o What is a meteor? A meteorite? A meteoroid? o What are the two main repositories of comets? Which one is at smaller/larger heliocentric radius? o Do comets always have tails? o How many tails does a comet have? o What is the composition of the nucleus of a comet? 5. Extrasolar Planets o What are the challenges associate with detecting extrasolar planets? o When was the first extrasolar planet discovered around a main-sequence star? o What are the key techniques we discussed for finding extrasolar planets? o Where is the center of mass in the Sun/Jupiter system (neglecting effects of other planets)? o How fast does the Sun move around the center of mass of the Sun/Jupiter system? o What about the Sun/Earth system? Where is the center of mass, and how fast does the Sun orbit around this center of mass? o Why does the orientation of the extrasolar planetary system matter for radial velocity measurements of extrasolar planets? o What would a multiple planet system look like in a plot of stellar radial velocity vs. time? o What type of planetary system is most easily detected with the radial velocity technique? o What are the types of planetary systems most easily discovered with direct imaging? Why look in the infrared? o Has the planetary transit phenomenon been observed in our own solar system? o Can we observe Jupiter transiting the Sun? o What are some of the highlights from the Kepler mission? o What is the "habitable zone"? o What does the overall distribution of planet masses look like? 6. The Sun o What are the layers of the solar interior? The solar atmosphere? o What are the net inputs and outputs of the proton-proton chain nuclear reaction? o What is the cause of solar activity? What are some of the key phenomena observed as solar activity? 7. Measurements of stars o How are luminosity and apparent brightness related? o Example: 2 stars, A and B, with the same luminosity. B has an apparent o brightness 16 times fainter than that of A. What do you conclude? o What is the relationship between stellar parallax and distance? o Example: A star has a measured parallax of 2 arcsec. What is its distance? (Note: no stars have measured parallaxes this large -- this is an imaginary thought question). o Example: A star has a measured parallax of 0.01 arcsec. What is its distance? o Example: What is the parallax of a star at d=10 pc? o What two key properties does a star's luminosity depend on? o Which law of thermal radiation is contained in the expression for a star's luminosity? o Example: The Sun will turn into a red giant with RRG=300 Rsun and surface temperature TRG=3100 K. How will the luminosity of the Red Giant compare with that of the current Sun? o What are the different spectral types? o On the main sequence the spectral types not only indicate a sequence of temperature, but also a sequence of....? o What is the H-R diagram? o Where is the Main Sequence on the H-R diagram? o What is the defining characteristic of stars on the Main Sequence? o Where are white dwarfs in the H-R diagram? o Where are Red Giants in the H-R diagram? o Example: Let's consider 4 types of stars, O, F, G, M. o Which has the hottest surface temperature? o Which has the same spectral type as the Sun? o Which has the longest Main Sequence lifetime? o Which has the smallest mass? o How do we estimate Main Sequence lifetime? o Which stars have the shortest main sequence lifetimes? o How do we measure the masses of stars? o How do star clusters work as clocks? 8. Stellar life cycles o What happens when a star leaves the main sequence? o What is a giant star? o What is the helium flash? o What do stars do on the horizontal branch, and how long do they spend there? o How many times will the Sun be a red giant? o How do low-mass stars end their life? o What is a planetary nebula? o What happens in the evolution of a high mass star? o What type of hydrogen fusion occurs in high mass stars? o What happens when a high mass star leaves the main sequence? o What happens as a high-mass star uses up the available fuel? o Why does nuclear fusion in high-mass stars stop at iron? o What happens when a high-mass star explodes?