MidtermReview - Review Questions for the Midterm: 1....

Info iconThis preview shows pages 1–3. Sign up to view the full content.

View Full Document Right Arrow Icon
Review Questions for the Midterm: 1. Overview the details of Jupiter beginning to migrate inwards, including possible causes and effects. Describe the final state of our Solar System in this case. If, as we believe may have happened in some exosolar systems, Jupiter were to migrate inwards, it could be due to a number of possible causes: gravitational interaction with other stars, gravitational interaction with other planets, and gravitational drag (where an in-spiraling body drags another along in its wake). The question then is what becomes of Jupiter in this scenario. Possible results are: a. It keeps going until it falls into the sun, or b. It stops somewhere in a closer orbit. Several mechanisms for the latter have been suggested, including (1) Running out of disk with which to interact, possibly due to solar wind activity, (2) Magnetic fields from the disk interacting with and braking the planet’s sun- ward fall until it goes into close orbit, or (3) Tidal locking with the sun acting to park the planet in close orbit. Whether Jupiter kept falling in or slowed into near orbit, it would have huge effect upon other planets on the way, clearing out other planets including our own as it goes, either Colliding with them; Tearing them apart with its gravitational field; Capturing them and turning them into satellites; Flinging them to larger orbits or even out of the solar system altogether. 1 2. What is the difference between proper motion and radial velocity of a star? Proper motion is motion that can be traced on the sky; radial velocity is motion in the same plane as the observer, i.e., towards and away from your p.o.v. 3. Describe the three most important properties for measuring a radial velocity curve used for planet detection. This is done by measuring the radial velocity of the star, that is, by examining the minute fluctuations in its movement towards and away from us. Since the star’s motion would be regular unless acted upon by some other body, any fluctuations that exhibit periodicity are presumed to be caused by the gravitational pull of a body orbiting that star. To do this we need a number of observations, with a high degree of sensitivity, over a period of time long enough to detect periodicity. Through this we can look at the signal (the actual mo- tion curve of the star including any fluctuations), noise (inaccuracies due to sampling er- ror, lack of sensitivity in instruments, interference from other sources, e.g. ., our own at- mosphere), and sampling (the number of samples over time). 1 Note that this is the only option discussed in the course. The others are my own suggestions.
Background image of page 1

Info iconThis preview has intentionally blurred sections. Sign up to view the full version.

View Full DocumentRight Arrow Icon
4. Where is most of the light coming from in a black hole and why? The jets, which are projected upon the axis of the black hole’s (presumed) rotation. As
Background image of page 2
Image of page 3
This is the end of the preview. Sign up to access the rest of the document.

This note was uploaded on 09/24/2008 for the course AST 309 taught by Professor Johnlacy during the Spring '08 term at University of Texas at Austin.

Page1 / 5

MidtermReview - Review Questions for the Midterm: 1....

This preview shows document pages 1 - 3. Sign up to view the full document.

View Full Document Right Arrow Icon
Ask a homework question - tutors are online