Our Evolving Universe
Self Test 1
In discussing stars, parallax refers to
the apparent motion of a star through the night, caused by the Earth's rotation
the difficulty in seeing stellar colours with the naked eye, because of the eye's physiology
the apparent motion of a star through the year, caused by the Earth's orbit
the distortions in telescopic images of the stars, caused by imperfect telescope optics
Compared to the 30 or so
nearest
stars, the Sun is
brighter than most
fainter than most
about average
impossible to compare, because we have no way of knowing how bright these stars really are
Sirius has
apparent
magnitude -1.5 and
absolute
magnitude 1.4, while Rigel has
apparent
magnitude 0.1 and
absolute
magnitude -7. Therefore
Sirius appears brighter but is really fainter (and closer)
Sirius appears fainter but is really brighter (and further away)
Sirius appears brighter and really is brighter
Sirius appears fainter and really is fainter
The mass of a star can be measured
only if its distance is known
only if its size (radius) is known
only indirectly, by estimating from other properties - there is no direct way to do it
only if it has a suitable binary companion
The Earth's distance from the Sun (one
astronomical unit
) is about eight light minutes. The nearest stars are
hundreds of astronomical units away
thousands of astronomical units away
hundreds of thousands of astronomical units away
hundreds of millions of astronomical units away
out of 5.
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Summary of Lecture 1
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Summary of Lecture 2
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