X-ray trigonometric parallax/Quiz
X-ray trigonometric parallax is a lecture about the theoretical possibility of using higher resolution X-ray detectors to measure stellar parallaxes. It is also a mini-lecture for a quiz section as part of the department of radiation astronomy course on the principles of radiation astronomy.
You are free to take this quiz based on X-ray trigonometric parallax at any time.
To improve your score, read and study the lecture, the links contained within, listed under See also, External links, and in the {{principles of radiation astronomy}} template. This should give you adequate background to get 100 %.
As a "learning by doing" resource, this quiz helps you to assess your knowledge and understanding of the information, and it is a quiz you may take over and over as a learning resource to improve your knowledge, understanding, test-taking skills, and your score.
Suggestion: Have the lecture available in a separate window.
To master the information and use only your memory while taking the quiz, try rewriting the information from more familiar points of view, or be creative with association.
Enjoy learning by doing!
Quiz
[edit | edit source]
Hypotheses
[edit | edit source]- It is possible using X-ray trigonometric parallax to fix the position of the Sun.
See also
[edit | edit source]External links
[edit | edit source]- International Astronomical Union
- NASA/IPAC Extragalactic Database - NED
- NASA's National Space Science Data Center
- The SAO/NASA Astrophysics Data System
- SDSS Quick Look tool: SkyServer
- SIMBAD Astronomical Database
- SIMBAD Web interface, Harvard alternate
- Spacecraft Query at NASA
- Universal coordinate converter
{{Radiation astronomy resources}}
Learn more about Trigonometric parallax |
