Chapter 17: Problem 1
Explain the difference between a star's apparent brightness and its luminosity.
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Chapter 17: Problem 1
Explain the difference between a star's apparent brightness and its luminosity.
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From its orbit around the Earth, the Hipparcos satellite could measure stellar parallax angles with acceptable accuracy only if the angles were larger than about \(0.002\) arcsec. Discuss the advantages or disadvantages of making parallax measurements from a satellite in a large solar orbit, say at the distance of Jupiter from the Sun. If this satellite can also measure parallax angles of \(0.002 \mathrm{arcsec}\), what is the distance of the most remote stars that can be accurately determined? How much bigger a volume of space would be covered compared to the Earth-based observations? How many more stars would you expect to be contained in that volume?
Search the World Wide Web for information about Gaia, a European Space Agency (ESA) spacecraft planned to extend the work carried out by Hipparcos. When is the spacecraft planned to be launched? How will Gaia compare to Hippar\(\cos\) ? For how many more stars will it be able to measure parallaxes? What other types of research will it carry out?
. Sketch the radial velocity curves of a binary consisting of two identical stars moving in circular orbits that are (a) perpendicular to and (b) parallel to our line of sight.
Some giant and supergiant stars are of the same spectral type (G2) as the Sun. What aspects of the spectrum of a G2 star would you concentrate on to determine the star's luminosity class? Explain what you would look for.
Would it be possible for a star to appear bright when viewed through a \(\mathrm{U}\) filter or a \(\mathrm{V}\) filter, but dim when viewed through a B filter? Explain.
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