Download problems

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

X-ray astronomy detector wikipedia , lookup

Hubble Space Telescope wikipedia , lookup

XMM-Newton wikipedia , lookup

Leibniz Institute for Astrophysics Potsdam wikipedia , lookup

Arecibo Observatory wikipedia , lookup

Allen Telescope Array wikipedia , lookup

Lovell Telescope wikipedia , lookup

Optical telescope wikipedia , lookup

James Webb Space Telescope wikipedia , lookup

Jodrell Bank Observatory wikipedia , lookup

Spitzer Space Telescope wikipedia , lookup

Reflecting telescope wikipedia , lookup

International Ultraviolet Explorer wikipedia , lookup

Very Large Telescope wikipedia , lookup

CfA 1.2 m Millimeter-Wave Telescope wikipedia , lookup

Transcript
AST 101 Spring 2008
Chapter 3 Weekly Problems
from Astronomy: A Beginner’s Guide to the Universe 5/E
NOT TO BE TURNED IN!
Complete and understand the Review and Discussion questions and the Problems to
prepare for the quizzes.
Review and Discussion:
Q1. List three advantages of reflecting telescopes over refracting telescopes.
Q3. How does Earth’s atmosphere affect what is seen through an optical telescope?
Q9. What is interferometry, and what problem in radio astronomy does it address?
Q14. What are the main advantages of studying objects at many different wavelengths of
radiation?
Problems:
P3. A 2-m telescope can collect a given amount of light in one hour. Under the same
observing conditions, how much time would be required for a 6-m telescope to perform
the same task? A 12-m telescope?
P4. A certain space-based telescope can achieve (diffraction-limited) angular resolution
of 0.05″ for red light (wavelength 700 nm). What would its resolution be (a) in the
infrared, at wavelength 3.5 μm, and (b) in the ultraviolet, at wavelength 140 nm?