Stars & Stellar Evolution Flashcards
luminosity
the rate at which a star or other object emits electromagnetic energy into space; the total power output of an object
apparent brightness
a measure of the amount of light received by Earth from a star or other object—that is, how bright an object appears in the sky, as contrasted with its luminosity
magnitude
an older system of measuring the amount of light we receive from a star or other luminous object; the larger the magnitude, the less radiation we receive from the object
color index
difference between the magnitudes of a star or other object measured in light of two different spectral regions—for example, blue minus visual (B–V) magnitudes
brown dwarf
an object intermediate in size between a planet and a star; the approximate mass range is from about 1/100 of the mass of the Sun up to the lower mass limit for self-sustaining nuclear reactions, which is about 0.075 the mass of the Sun; brown dwarfs are capable of deuterium fusion, but not hydrogen fusion
spectral class
(or spectral type) the classification of stars according to their temperatures using the characteristics of their spectra; the types are O, B, A, F, G, K, and M with L, T, and Y added recently for cooler star-like objects that recent survey have revealed
giant
a star of exaggerated size with a large, extended photosphere
proper motion
the angular change per year in the direction of a star as seen from the Sun
radial velocity
motion toward or away from the observer; the component of relative velocity that lies in the line of sight
space velocity
the total (three-dimensional) speed and direction with which an object is moving through space relative to the Sun
selection effect
the selection of sample data in a nonrandom way, causing the sample data to be unrepresentative of the entire data set
eclipsing binary
a binary star in which the plane of revolution of the two stars is nearly edge-on to our line of sight, so that the light of one star is periodically diminished by the other passing in front of it
distances Light year=KM=CM
1 light-year = 9.5 × 1012 km = 9.5 × 1017 cm
interstellar dust
tiny solid grains in interstellar space thought to consist of a core of rocklike material (silicates) or graphite surrounded by a mantle of ices; water, methane, and ammonia are probably the most abundant ices
interstellar medium (ISM)
or interstellar matter) the gas and dust between the stars in a galaxy