Classes as extreme as M2.5 and M5 have been given.A very large and luminous star, VY CMa is among the Most of the output of VY CMa is emitted as infrared radiation, with a maximum emission at 5–10 μm, which is in part caused by reprocessing of the radiation by the circumstellar nebula.Since VY CMa has no companion star, its mass cannot be measured directly through gravitational interactions. This galaxy is situated at around 42,000 light-years away from the Galactic Center.The Nine Planets has been online since 1994 and was one of the first multimedia websites that appeared on the World Wide Web.Take an interactive tour of the solar system, or browse the site to find fascinating information, facts, and data about our planets, the solar system, and beyond.

The cluster is in relation with the giant nebula Sh2-310.NGC 2354 is a relatively fain open cluster that contains around 15 stars which are visible through binoculars. Parallax is … This is one of the largest star-forming H II regions which has a diameter of around 480 arcminutes / 681 light-years / 209 parsecs. VY Canis Majori’s radius has been estimated to be around 1.420 times greater than the sun’s radius.VY Canis Majoris’s diameter is around 1.750 times greater than the VY Canis Majoris is a red supergiant/hypergiant star of spectral type M3-M4.5. VY Canis Majoris has a rotational velocity of around 300 km / 186.4 mi per second. Aludra is located at around 2,000 light-years away.Tau Canis Majoris is a multiple star system located at around 5,000 light-years away. It has an apparent magnitude that varies from 6.5 to –  9.6, and its absolute magnitude is – 9.4.This hypergiant is losing its mass to a rate of around 30 times the mass of VY Canis Majoris is cooler than our sun, with an estimated surface temperature of around 3.490 K. Our Sun has around 5.778 K surface temperatures for comparison.

Hypernovas produce considerably higher amounts of energy than regular supernovas. VY Canis Majoris a.k.a. This disputed dwarf irregular galaxy is situated at around 25,000 light-years away from us.The Canis Major Dwarf Galaxy is estimated to contain 1 billion stars, many of which are red giants. VY Canis Majoris is around 4,000 light years from Earth in the constellation of Canis Major. WR 7 lies at the center of a complex bubble of gas which is shocked and partially ionized by the star’s radiation and winds.WR 7 is also exciting the ring nebula NGC 2359, also known as Thor’s Helmet. VY Canis Majoris is an enormous supergiant or hypergiant located in the constellation of Canis Major. Comparison of the effective temperature and bolometric luminosity of VY CMa compared to evolutionary tracks for massive stars suggest an initial mass of The effective temperature of VY CMa is uncertain but as the spectrum of VY CMa varies, then also the temperature may vary. This Wolf-Rayet star has a bolometric luminosity 620,000 times greater than that of our Sun.It is also several times hotter, having temperatures of around 89,100 K. EZ Canis Majoris has 2,300% of our Sun’s mass and 325% of its radius.HD 56925, also designated as WR 7, is also a Wolf-Rayet star, located at around 17,000 light-years away from us.

Scientists eventually realized that the said discrete components were actually bright areas of the surrounding nebula.You can read more about the VY Canis Majoris here in Universe Today. The most massive known star is R136a1. Formation Edit. The brightest star here is Tau Canis Majoris, and thus the whole cluster is sometimes referred to as the Tau Canis Majoris Cluster.

It is among the largest known stars ever discovered. Furud has surface temperatures of around 18,700 K, it is located at 362 light-years.Muliphein, designated as Gamma Canis Majoris, is a blue-white B-type bright giant star located at around 440 light-years away. VY Canis Majoris is a pulsating variable star situated at around 3.900 light-years / 1.2 kiloparsecs away from the Sun. VY Canis Majoris is a very young star, and it is believed that it evolved from an VY Canis Majoris is situated at around 3.900 light-years / 1.2 kiloparsecs away from the Sun.

It is said to lay inside of a dormant volcano, using very many smaller dragons as its drone-like subjects. It is more than 1.000 times bigger than our sun, and it is among the largest known stars in the Milky Way galaxy.VY Canis Majoris was first observed and recorded in 1801 by the French astronomer Jerome Laland. Muliphein has an apparent magnitude of +4.10.This star is a chemically peculiar Hg-Mg star having abnormal lines of magnesium and mercury in its spectrum.

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