A Cepheid variable or Cepheid is a member of a particular class of variable stars, notable for a fairly tight correlation between their period of variability and absolute luminosity.
Since the period-luminosity relation can be calibrated with great precision using the nearest Cepheid stars, the distances found with this method are among the most accurate available.
For more information about the topic Cepheid variable, read the full article at Wikipedia.org, or see the following related articles:
Supergiant Supergiants are the most massive stars. Supergiants can have masses from 10 to 70 solar masses and brightness from 30,000 up to hundreds of thousands ... >
read more
Red giant A red giant is a large non-main sequence star of stellar classification K or M; so-named because of the reddish appearance of the cooler giant stars. ... >
read more
Luminosity In general physics, luminosity (more properly called luminance) is the density of luminous intensity in a given ... >
read more
Star cluster Star clusters are groups of stars which are gravitationally bound. Two distinct types of star cluster can be distinguished: globular clusters are ... >
read more
Open cluster An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud, and are still loosely gravitationally ... >
read more
Red supergiant star Red supergiants are supergiant stars of spectral type K-M and a luminosity class of I. They are the largest stars in the universe in terms of ... >
read more
Stellar classification In astronomy, stellar classification is a classification of stars based initially on photospheric temperature and its associated spectral ... >
read more
Space observatory A space observatory is any instrument in outer space which is used for observation of distant planets, galaxies, and other outer space objects. A ... >
read more
Blue supergiant star Blue supergiants are supergiant stars (class I) of spectral type O. They are extremely hot and bright, with surface temperatures of between 20,000 - ... >
read more
Andromeda Galaxy TThe Andromeda Galaxy (also known as Messier 31, M31, or NGC 224; older texts often called it the Andromeda Nebula) is a spiral galaxy approximately ... >
read more
Note: This page refers to an article that is licensed under the GNU Free Documentation License. It uses material from the article Cepheid variable at Wikipedia.org. See the Wikipedia copyright page for more details.
Recommend this page on Facebook, Twitter,
and Google +1:
Other bookmarking and sharing tools: