Notable features Stars Horologium does not have any bright stars.

Notable features Stars There are no stars brighter than 4th magnitude in this constellation.

It is a semiregular variable star with a minimum magnitude of 5.1 and a maximum magnitude of 3.4.

Notable features Stars There are four bright stars in Chamaeleon.

The three brightest stars, Alpha, Beta and Gamma, make up the triangle.

The brightest stars, on either scale, have negative magnitude numbers.

Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names.

Within the constellation's borders, there are 49 stars brighter than or equal to apparent magnitude 6.5.

Its name is Latin for triangle , derived from its three brightest stars, which form a long and narrow triangle.

The relative brightness of the two stars is also an important factor, as glare from a bright star may make it difficult to detect the presence of a fainter component.

The arrangement of the brightest stars is somewhat similar to Ursa Major and Ursa Minor.

The bright stars correspond to little daggers on the rete.

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Brightest stars The nine brightest stars of the Pleiades are named for the Seven Sisters of Greek mythology Sterope, Merope, Electra, Maia, Taygeta, Celaeno, and Alcyone, along with their parents Atlas and Pleione.

Along with Aldebaran, Regulus, and Fomalhaut, Antares comprises the group known as the 'Royal stars of Persia'.

The brighter stars, however, are not true members of the cluster, as they are closer to the Earth than the dimmer ones.

The brightest stars, usually the stars that make up the constellation's eponymous asterism, also retain proper names, often from Arabic.

The arms are visible because the high density facilitates star formation, and therefore they harbor many bright and young stars.

The French explorer and astronomer Nicolas Louis de Lacaille charted and gave the brighter stars their Bayer designations in 1756.

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Several of the brightest stars in the 'Plough' of Ursa Major are former members of an open cluster which now form such an association, in this case, the Ursa Major Moving Group.

For example, the asterism known as the Big Dipper comprises the seven brightest stars in the IAU constellation (area) Ursa Major.

During the 20th century, observations showed that H II regions often contained hot, bright stars.

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The youngest and brightest stars we now see in the Orion Nebula are thought to be less than 300,000 years old, and the brightest may be only 10,000 years in age.

Bright stars were important to the ancient Polynesians for navigation between the many islands and atolls of the Pacific Ocean.

Because of this, its main stars have no particular pattern and it is devoid of bright deep sky objects.

The primary has a luminosity of and the secondary has a luminosity of the primary is an A type star with an absolute magnitude of 0.2 and the secondary is a B9 type star with an absolute magnitude of 0.4.

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Ultraviolet astronomy is best suited to the study of thermal radiation and spectral emission lines from hot blue stars (OB stars) that are very bright in this wave band.

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The absolute magnitudes of galaxies can be much lower (brighter).

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Observations A few of the brightest H II regions are visible to the naked eye.

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Higher potentials, spaced at 19 volt intervals, will result in additional glowing regions in the tube.

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Among nearby stars, it has been found that younger population I stars have generally lower velocities than older, population II stars.

Some open clusters contain hot blue stars which seem to be much younger than the rest of the cluster.

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Symbiotic stars are binary star systems composed of a late type giant star and a hotter companion object.

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