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vy canis majoris

VY Canis Majoris is a pulsating variable star situated at around 3.900 light-years / 1.2 kiloparsecs away from the Sun.

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. It is one of the Largest known Stars in the universe, and one of the most luminous of its type.. VY Canis Majoris is 1,420 times wider than the Sun. It is one of the biggest stars ever observed and detected in the VY Canis Majoris has been estimated to have around 17 solar masses, and it is believed that it's lost more than half its mass. It is more than 1.000 times bigger than our sun, and it is among the largest known stars in Looking for fun activities to teach kids about VY Canis Majoris?This premium worksheet bundle contains a printable fact file and 10 fun and engaging worksheets to challenge your students and help them learn about VY Canis Majoris.VY Canis Majoris was first observed and recorded in 1801 by the French astronomer Jerome Laland.

Dane z jego strony opisu znajdują się poniżej. The Canis Major constellation represents the big hunter dog of Orion, the celestial hunter. This is a red metagiant. Molecular clouds of gas and dust are responsible for many star births. The main star is a red hypergiant located in the constellation Canis Major. The hypernova explosion is estimated to take place in around 100.000 years. Plik Sun and VY Canis Majoris.svg znajduje się w Wikimedia Commons – repozytorium wolnych zasobów. VY Canis Majoris is an enormous supergiant or hypergiant located in the constellation of Canis Major. It has an apparent magnitude that varies from 6.5 to - 9.6, and its absolute magnitude is – 9.4. It is one of the largest known stars in the Milky Way galaxy. Pada skala ini, VY Canis Majoris memiliki diameter sekitar 2.3 kilometer. Thus, because of this, it was given the designation VY Canis Majoris in 1939, the 3VY Canis Majoris is embedded within the large molecular cloud called Sh2-310. 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. This red Hypergiant star, found in the constellation Canis Major, is estimated to have a …

After the star explodes, it is speculated that its remaining core will collapse and result in a black hole.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. They also produce long-duration gamma-ray bursts, which are among the most energetic events observed in our universe.When it will happen, VY Canis Majoris will explode releasing the energy of more than 100 times that of a supernova, and enormous quantities of gamma rays.This explosion will not affect Earth as the hypergiant is too far away, but if there are any planets near VY Canis Majoris which host life, it would be completely eradicated. It is one of the largest known stars in the galaxy as well as one of the most luminous of its type. VY Canis Majoris has an average density of 5.33 to 8.38 mg/mVY Canis Majoris is located in the constellation of Canis Major. VY Canis Majoris has a rotational velocity of around 300 km / 186.4 mi per second.

It was listed as a long-period variable with a photographic magnitude range of 9.5 to 11.5. VY Canis Majoris is a red hypergiant with a radius of around 1,500 times larger than the sun. It is bright enough to be observed with a pair of regular binoculars.Consecuentely, VY Canis Majoris is the biggest star of the constellation. VY Canis Majoris - Universe Today Of all known stars, the VY Canis Majoris is the largest. Mu Sonne is even bigger than VY Masses Majoris. Para astronom, dengan bantuan Dari Wikipedia bahasa Indonesia, ensiklopedia bebas This star is just about a thousandth of a light year. Opis {{Information |other_versions=Prace pochodne od tego pliku: Sun and VY Canis Majoris-bg.svg It was listed as a 7It was first described as a crimson star, while observations progressed it was discovered that VY Canis Majoris was a strong source of OH(1.612 MHz), HIn 1931, variations in VY Canis Majoris’s brightness were first described. Ada 2 perbedaan pendapat tentang sifat VY CMa. Satu pendapat mengatakan bahwa VY CMa sangat besar dan merupakan bintang maharaksasa merah dengan VY CMa akan menjadi sangat tidak stabil setelah melepaskan banyak massa ke nebula di sekitarnya. VY Canis Majoris is surrounded by a complex asymmetric circumstellar envelope caused by mass loss from the star itself.

VY Canis Majoris (VY CMa) is a red hypergiant star in the constellation Canis Major.It is about 1.2 kiloparsecs (3,900 light-years) distant from Earth. Catatan pertama VY CMa yang diketahui ada dalam katalog bintang Profesor Roberta M. Humphreys dari Universitas Minnesota memperkirakan radius VY CMa adalah 1800 hingga 2100 kali radius Matahari.Jika Bumi diwakili oleh bola dengan diameter 1 cm, Matahari diwakili bola dengan diameter 109 cm, dengan jarak antara keduanya 117 meter. This is one of the largest star-forming H II regions which has a diameter of around 480 arcminutes / 681 light-years / 209 parsecs. Hypernovas produce considerably higher amounts of energy than regular supernovas. In the case of VY Canis Majoris, it was formed around 10 million years ago when gravity pulled swirling gas and dust together.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.

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