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| physical object > natural object > celestial body > star > variable > periodic variable > long-period variable |
| long-period variable (red variable, Mira variable) | ||||
| subject | fact | |||
| long-period variable | has amplitude 9 magnitudes in the visible, but only 2 or 3 magnitudes in the integrated spectrum | ![]() |
| has period 100 to 1000 days | ![]() | |
| has prototype Mira | ![]() | |
| has spectral type M star, R star, or N star | ![]() | |
| has synonym red variable | ![]() | |
| has synonym Mira variable | ![]() | |
| has definition Cyclic variable with cycles 100-500 days, and of spectral types K, M, S and C. | ![]() | |
| has definition Pulsating red giant or supergiant. Population I typically have periods greater than 200 days; Population II, periods less than 200 days. Long-period variables emit most of their radiation in the infrared. | ![]() | |
| is a kind of periodic variable | ![]() | |
| is a part of disk | ![]() | |
| variable | has name designated with
| ![]() |
| has observational problem some difficulty in distinguishing between various kinds | ![]() | |
| has observable variation time scale within a period of decades | ![]() | |
| has light curve | ![]() | |
| has optical brightness variation 0.2 magnitudes or greater | ![]() | |
| star | has star surface temperature | ![]() |
| has V magnitude | ![]() | |
| has B magnitude | ![]() | |
| has U magnitude | ![]() | |
| has position on celestial sphere from the point of view of Earth | ![]() | |
| has parallax from the point of view of Earth's orbit | ![]() | |
| has proper motion | ![]() | |
| has radiation at surface which is diffused out from the hotter core | ![]() | |
| has energy source gravitational contraction and or fusion | ![]() | |
| has energy production which takes place primarily within the core | ![]() | |
| has surface density which depends on luminosity class | ![]() | |
| has surface temperature greater than 1000 Kelvin | ![]() | |
| has apparent magnitude | ![]() | |
| has absolute magnitude | ![]() | |
| has age | ![]() | |
| has catalog star catalog | ![]() | |
| has material hydrogen, helium | ![]() | |
| has velocity determined from proper motion and radial velocity | ![]() | |
| has mass greater than 0.08 the sun's mass | ![]() | |
| celestial body | has spectra | ![]() |
| physical object | has location or center of gravity | ![]() |
| has angular momentum | ![]() | |
| has momentum | ![]() | |
| has temperature | ![]() | |
| has volume | ![]() | |
| has extent | ![]() |
Kinds of long-period variable :
(15 facts) (omicron Cet) - A red giant that varies in brightness as it pulsates. When brightest, Mira is visible to the naked eye; when dimmest, Mira can be viewed only with optical aid. Mira is the prototype of all pulsating red giants, which are called Miras in its honor., A irregular long-period intrinsic variable. It was named Mira ("wonderful") in 1596 by Fabricius, who made the first recorded observations of its brightness fluctuations. Mira is a double star with a faint B companion which is itself variable.
Next periodic variable: RR Lyrae star Up: periodic variable Previous periodic variable: eclipsing binary