Vy Canis Majoris Star Dictionary Vy canis majoris (abbreviated to vy cma) is an extreme oxygen rich red hypergiant or red supergiant (o rich rhg or rsg) and pulsating variable star 1.2 kiloparsecs (3,900 light years) from the solar system in the slightly southern constellation of canis major. Vy cma is a collection of several star like nuclei within a dense nebula. it appears as an oxygen rich red star of spectral class m3 4ii. (1) it is known for its unpredictable behavior and for its strong infrared and microwave signals.
Vy Canis Majoris Wikiwand Vy canis majoris is classified as a variable star. the hypergiant shines at magnitude 6.5 at maximum brightness and at magnitude 9.6 at minimum. its brightness varies due to pulsations. the estimated period of the pulsations is 956 days. other periods of 1,600 and 2,200 have also been reported. Vy canis majoris (abbreviated to vy cma) is an extreme oxygen rich red hypergiant or red supergiant (o rich rhg or rsg) and pulsating variable star 1.2 kiloparsecs (3,900 light years) from the solar system in the slightly southern constellation of canis major. This hubble space telescope image shows the huge nebula of material cast off by the hypergiant star vy canis majoris. this nebula is approximately 186 billion miles across. Vy canis majoris (vy cma) is one of the largest, most luminous red supergiant (rsg) stars in the galaxy. this huge oxygen rich rsg may be on the verge of becoming a bright core collapse type ii supernova. over the 20th century, vy cma has been undergoing episodic large quasi periodic light variations.
Download Vy Canis Majoris Star Space Royalty Free Vector Graphic This hubble space telescope image shows the huge nebula of material cast off by the hypergiant star vy canis majoris. this nebula is approximately 186 billion miles across. Vy canis majoris (vy cma) is one of the largest, most luminous red supergiant (rsg) stars in the galaxy. this huge oxygen rich rsg may be on the verge of becoming a bright core collapse type ii supernova. over the 20th century, vy cma has been undergoing episodic large quasi periodic light variations. Vy canis majoris is a red hypergiant star that is one of the largest and most luminous known stars in the milky way galaxy. it is an irregular pulsating variable and lies about 5,000 light years away in the constellation canis major. 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 β 9.4. Vy canis majoris (abbreivated as vy cma) is an enormous, extremely oxygen rich red hypergiant (or red supergiant) star and pulsating variable star, located approximately 3,820 light years (1,170 parsecs) away from earth in the constellation canis major. The companions may be details of the nebula; some of them are probably variable [02159, 03287]. surrounded by an envelope of gas and dust or a disk of 0.45" (lambda = 5 mkm) angular size.
Vy Canis Majoris Alchetron The Free Social Encyclopedia Vy canis majoris is a red hypergiant star that is one of the largest and most luminous known stars in the milky way galaxy. it is an irregular pulsating variable and lies about 5,000 light years away in the constellation canis major. 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 β 9.4. Vy canis majoris (abbreivated as vy cma) is an enormous, extremely oxygen rich red hypergiant (or red supergiant) star and pulsating variable star, located approximately 3,820 light years (1,170 parsecs) away from earth in the constellation canis major. The companions may be details of the nebula; some of them are probably variable [02159, 03287]. surrounded by an envelope of gas and dust or a disk of 0.45" (lambda = 5 mkm) angular size.
Vy Canis Majoris Star Type Size Location Constellation Star Facts Vy canis majoris (abbreivated as vy cma) is an enormous, extremely oxygen rich red hypergiant (or red supergiant) star and pulsating variable star, located approximately 3,820 light years (1,170 parsecs) away from earth in the constellation canis major. The companions may be details of the nebula; some of them are probably variable [02159, 03287]. surrounded by an envelope of gas and dust or a disk of 0.45" (lambda = 5 mkm) angular size.
Vy Canis Majoris Star Type Size Location Constellation Star Facts
Comments are closed.