Brightness of Stars Flashcards
Why can we only see 2000-3000 stars in the sky?
-too far
-cosmic dust can obscure the view
-star is too small
-temp of the star
Why are distances to planets in km, while the distances to stars and galaxies are in ly?
They are so far away
What is the current estimate for the number of galaxies in the universe?
100 billion
What is the estimated volume of our universe?
1x10^30 cubic lightyears
What is a baseline?
-Baseline is an imaginary line from which the distance to an object is measured
-The diameter of Earth’s orbit is the longest baseline possible
-In astronomy, the distances are very large, and a larger baseline increases the accuracy
Why does parallax only work for stars less than 200 ly away?
At distances further than 200 ly, the angles involved are too small, creating too many observational errors
When using triangulation to determine distances indirectly what can you do to improve the accuracy of your measurements?
Use bigger baselines
What is a Cepheid variable star and what makes it a variable?
Cepheid variable stars are unstable, yellow supergiants that pulse, or change in size and brightness
Why is a Cepheid variable star referred to as a standard candle?
They pulsate over regular intervals (this correlates with how bright a star is)
Observations of a pair of Cepheids reveal that Cepheid A is pulsing faster than Cepheid B. Which of the 2 has a greater absolute magnitude?
Cepheid B
What is the difference between absolute and apparent magnitude?
Absolute magnitude is the actual amount of light a star gives off, while apparent magnitude is how bright a star appears in the night sky
What is the connection between a Cepheid variable star’s pulse and its brightness?
the larger Cepheids pulse slower and are brighter
What 2 conclusions can an astronomer make about a galaxy with a slight red shift and a galaxy with a large redshift?
The more red-shifted a galaxy is, the faster it moves, and the farther away it is
How does the brightness of a light source change with distance?
At different distances from the observer, the different light sources appear as the same brightness