Cosmic Perspective Fundamentals
Cosmic Perspective Fundamentals
3rd Edition
ISBN: 9780134988504
Author: Bennett, Jeffrey O., Donahue, M. (megan), SCHNEIDER, Nicholas, Voit, Mark
Publisher: Pearson,
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Chapter 12, Problem 3QQ
To determine

The change in parallax shifts of nearby stars if the orbital radius of the Earth is doubled.

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Using Kepler's 3rd law solve the following problem.  Show your work and  highlight your answer.     In a distant star system there are many inhabitable planets.  One of these planets is named Qomar.  Qomar is 3.2 AU's from its star and takes 6.5 Earth years to go around its  star once.    There is another planet in the same star system called Ferenginar.   Ferenginar is 0.9 AUs from the star.  What is the length of a Ferengi year (on Ferenginar) in terms of Earth years?
Kindly provide the solution to the following question using the GRASS  method. Gravitational Fields - Orbital Speed question, (Unit: Gravitational, Electric, and Magnetic Fields).   The images attached are the formulas for this unit and the question. Please make sure to show all your work using the GRASS (given, required, analysis, solution, and statement) method and using formulas from this unit (Gravitational, Electric, and Magnetic Fields).
Using MBH = 6.6 × 10 Mo, calculate the below. a. Find radius of the Schwarzschild sphere (Schwarzschild radius Rs). You can calculated from the appropriate formula or just use the fact that for an object of 1 solar mass Rs = 3 km. b. Express Rs in km, in AU, in parsecs. c. Using the distance to M87 and your result above, find angular radius of the SMBH (Schwarzschild radius). Express it in arcseconds (") and micro- arcseconds (pas) d. Take the radius of Pluto's orbit equal to 40 AU and find its angular size (in micro-arcseconds, pas) at the distance of M87.
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