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...uminosity stars (red and white dwarfs) from the Gliese Catalogue of Nearby Stars.]] ...ll]]. Stars on this band are known as '''main-sequence stars''' or "dwarf" stars. ...

The primary (IK Pegasi A) is a [[main sequence]], [[spectral class|A-class]] star that displays minor pulsations in [[lumi ...gasi B) is a massive [[white dwarf]]—a star that has evolved past the main sequence and is no longer generating energy through [[nuclear fusion]]. They orbit e ...

| title=Are beryllium abundances anomalous in stars with giant planets? | title=Magnetic Field and Rotation in Lower Main-Sequence Stars: an Empirical Time-dependent Magnetic Bode's Relation? ...

...trait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars | title=First radius measurements of very low mass stars with the VLTI ...

...en-Institut Heidelberg | date=March 4, 1998 | work=ARI Database for Nearby Stars |url=http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c01453.h ...wo-Tenths catalogue|LTT]] 15309, Munich 15040, [[List of nearest stars|Proxima Ophiuchi]], [[Variable star designation|V2500 Ophiuchi]], ''[[Latin ...

...ght|300px|The [[Pleiades (star cluster)|Pleiades]], an [[open cluster]] of stars in the [[constellation]] of [[Taurus (constellation)|Taurus]]. ''[[NASA]] p ...ghtest stars gained proper names. Extensive [[star catalogue|catalogues of stars]] have been assembled by astronomers, which provide standardized [[star des ...

...s to smaller denser clumps within, which then proceed to collapse and form stars. Star formation is a complex process, which always produces a gaseous [[pro {{main article|History of Solar System formation and evolution hypotheses}} ...

| title=The Stars: Their Structure and Evolution | title=The Stars: Their Structure and Evolution ...

| title=The Stars: Their Structure and Evolution | title=The determination of T_eff for metal-poor A-type stars using V and 2MASS J, H and K magnitudes ...

...nergy]].<ref name="osln" /> White dwarfs comprise roughly 6% of all known stars in the [[Local Interstellar Cloud|solar neighborhood]].<ref>[http://www.cha ...hys230/lectures/planneb/planneb.html Late stages of evolution for low-mass stars], Michael Richmond, lecture notes, Physics 230, [[Rochester Institute of Te ...

...wn as a [[white dwarf]]. In the far distant future, the gravity of passing stars gradually will whittle away at the Sun's retinue of planets. Some planets w {{main|History of Solar System formation and evolution hypotheses}} ...

The Solar System is also home to two main belts of [[small solar system body|small bodies]]. The [[asteroid belt]], w {{main|Discovery and exploration of the Solar System}} ...

The extreme [[age of the universe]] and its vast number of stars suggest that if the Earth is typical, extraterrestrial life should be commo ...olved: there are an estimated 250 billion (2.5 x [[1 E9|10¹¹]]) stars in the [[Milky Way]] and 70 sextillion (7 x 10²²) in the [[visib ...

{{main|History of the Big Bang theory}} ...of general relativity|tests]] on the scale of the solar system and binary stars while extrapolation to cosmological scales has been validated by the empiri ...

...et Propulsion Laboratory |publisher=NASA}}</ref> Its surface comprises two main types of terrain. Dark regions, saturated with [[impact crater]]s and dated ...ede, on January 13. By January 15, Galileo came to the conclusion that the stars were actually bodies orbiting Jupiter.<ref name="Discovery">{{cite web | ur ...

{{main|Light}} {{Main|Bose gas|Bose–Einstein statistics|Spin-statistics theorem}} ...