vy canis majoris distance from earth

Its traditional name means "the virgins", having been transferred from the group of stars to Epsilon alone.

It is a blue-white supergiant of spectral type B2Iab, around 404 light-years from Earth. We and our partners will store and/or access information on your device through the use of cookies and similar technologies, to display personalised ads and content, for ad and content measurement, audience insights and product development. [90] NGC 2362 is a small, compact open cluster, 5200 light-years from Earth. [44], Also called Aludra, Eta Canis Majoris is a blue-white supergiant of spectral type B5Ia with a luminosity 176,000 times and diameter around 80 times that of the Sun. [51] Omicron1 is an orange K-type supergiant of spectral type K2.5Iab that is an irregular variable star, varying between apparent magnitudes 3.78 and 3.99. Both stars are emitting jets of material, that of the Herbig Ae/Be star being much larger—11.7 light-years long. EZ Canis Majoris is a Wolf–Rayet star of spectral type WN4 that varies between magnitudes 6.71 and 6.95 over a period of 3.766 days; the cause of its variability is unknown but thought to be related to its stellar wind and rotation. [87] Its most luminous stars have already evolved into giants. Does Jerry Seinfeld have Parkinson's disease? Sirius is also a binary star; its companion Sirius B is a white dwarf with a magnitude of 8.4–10,000 times fainter than Sirius A to observers on Earth. [41] Nearby is Delta Canis Majoris, also called Wezen.

At this distance, ... but I flew out to 8 light minutes, roughly the distance from Sol to Earth, from a random G-type. When did organ music become associated with baseball? I searched up of the radius of VY Majoris and google said it was 987.9 million km and the radius of the earth is 6371.393 km according to google (I converted from miles to km). The brightest is a 6.3-magnitude star of spectral type K3. [95], NGC 2207 and IC 2163 are a pair of face-on interacting spiral galaxies located 125 million light-years from Earth. VY Canis Majoris è una stella ipergigante rossa variabile irregolare situata nella costellazione del Cane Maggiore a 3 840 anni luce dal sole. Its current mass is about 17 ± 8 solar masses, having shed material from an initial mass of 25–32 solar masses. Nu2 Canis Majoris is an ageing orange giant of spectral type K1III of apparent magnitude 3.91 located around 64 light-years distant. About 40 million years ago, the two galaxies had a close encounter and are now moving farther apart; nevertheless, the smaller IC 2163 will eventually be incorporated into NGC 2207. [69] Exceedingly faint, it has an apparent magnitude of 26.6. Oma valikute muutmiseks võite igal ajal külastada oma privaatsuse juhtseadeid. In contrast, the other bright stars of the constellation are stars of great distance and high luminosity. [45] Classified as an Alpha Cygni type variable star, Aludra varies in brightness from magnitude 2.38 to 2.48 over a period of 4.7 days. [31], Sirius is the brightest star in the night sky at apparent magnitude −1.46 and one of the closest stars to Earth at a distance of 8.6 light-years. [1] Covering 380 square degrees or 0.921% of the sky, it ranks 43rd of the 88 currently-recognized constellations in size. As the interaction continues, gas and dust will be perturbed, sparking extensive star formation in both galaxies. [6], At the southern limits of the constellation lie Kappa and Lambda Canis Majoris. A fifth component, a magnitude 10 star, lies at a distance of 13,000 astronomical units (0.21 ly).

These include Sirius (Alpha Canis Majoris), the brightest star in the night sky, as well as three other stars above magnitude 2.0. Sirius was the basis for the ancient Egyptian calendar. The material on this site can not be reproduced, distributed, transmitted, cached or otherwise used, except with prior written permission of Multiply. È una delle stelle più grandi conosciute, con un raggio pari a circa 1 420 volte il raggio solare (696 000 km) e, in virtù delle sue … [28] Flamsteed's listing of Nu1, Nu2, Nu3, Xi1, Xi2, Omicron1 and Omicron2 have all remained in use. [23] The moon (Mityan, "native cat") sought to lure the further wife (Epsilon) away, but Unurgunite assaulted him and he has been wandering the sky ever since. [73] R Canis Majoris is another eclipsing binary that varies from magnitude 5.7 to 6.34 over 1.13 days,[74] with a third star orbiting these two every 93 years. [39] This star is one of the brightest known extreme ultraviolet sources in the sky. VY Canis Majoris is located in the constellation Canis Major. but have no connection with each other. [83] The more massive Herbig Ae/Be star is enveloped in an irregular roughly spherical cocoon of dust that has an inner diameter of 20 AU (3.0×109 km) and outer diameter of 50 AU (7.5×109 km). [6] The star marked the Great Dog's mouth on Bayer's star atlas. [94] On the other hand, a globular cluster in Puppis, NGC 2298—which appears to be part of the Canis Major dwarf system—is extremely metal-poor, suggesting it did not arise from the Milky Way's thick disk, and instead is of extragalactic origin. [49] Only 7 million years old,[49] it has exhausted the supply of hydrogen at its core and is now processing helium. Its name is Latin for "greater dog" in contrast to Canis Minor, the "lesser dog"; both figures are commonly represented as following the constellation of Orion the hunter through the sky. [3] The Ancient Greeks replaced the bow and arrow depiction with that of a dog. Information about your device and internet connection, including your IP address, Browsing and search activity while using Verizon Media websites and apps. [38] Marking the dog's right thigh on Bayer's atlas is Epsilon Canis Majoris,[33] also known as Adhara. [88] NGC 2360, known as Caroline's Cluster after its discoverer Caroline Herschel, is an open cluster located 3.5 degrees west of Muliphein and has a combined apparent magnitude of 7.2. The nature of the changes are unclear, but it is possible they were caused by an event such as the star's absorption of an accretion disc. [71] Its four main component stars are hot O-type stars, with a combined mass 80 times that of the Sun and shining with 500,000 times its luminosity, but little is known of their individual properties. In the second century, it was included in Ptolemy's 48 constellations, and is counted among the 88 modern constellations. [7] In medieval Arab astronomy, the constellation became al-Kalb al-Akbar, "the Greater Dog", transcribed as Alcheleb Alachbar by 17th century writer Edmund Chilmead. [72] UW Canis Majoris is another Beta Lyrae-type star 3000 light-years from Earth; it is an eclipsing binary that ranges in magnitude from a minimum of 5.3 to a maximum of 4.8. [13], Both the Māori people and the people of the Tuamotus recognized the figure of Canis Major as a distinct entity, though it was sometimes absorbed into other constellations. [69], Tau Canis Majoris is a Beta Lyrae-type eclipsing multiple star system that varies from magnitude 4.32 to 4.37 over 1.28 days. [25] The official constellation boundaries, as set by Belgian astronomer Eugène Delporte in 1930, are defined by a quadrilateral; in the equatorial coordinate system, the right ascension coordinates of these borders lie between 06h 12.5m and 07h 27.5m , while the declination coordinates are between −11.03° and −33.25°. [68] At the other extreme in size is RX J0720.4-3125, a neutron star with a radius of around 5 km. In the later compendium of Babylonian astronomy and astrology titled MUL.APIN, the arrow, Sirius, was also linked with the warrior Ninurta, and the bow with Ishtar, daughter of Enlil. If located in the centre of the Solar System, it would extend out to Earth as its diameter is 200 times that of the Sun.

It is one of largest stars known (sometimes described as the largest known)[64] and is also one of most luminous with a radius varying from 1,420 to 2,200 times the Sun's radius, and a luminosity around 300,000 times greater than the Sun. [40] It is a binary star; the secondary is of magnitude 7.4. Another, NR Canis Majoris, will be brightest at magnitude −0.88 in about 2.87 million years' time. Both stars are surrounded by a large envelope of in-falling material left over from the original cloud that formed the system. [58] Nu Canis Majoris is a yellow-hued giant star of magnitude 5.7, 278 light-years away; it is at the threshold of naked-eye visibility. Also called Mirzam or Murzim, Beta is a blue-white Beta Cephei variable star of magnitude 2.0, which varies by a few hundredths of a magnitude over a period of six hours. Located 4 degrees south of Sirius, it contains contrasting blue, yellow and orange stars and covers an area the apparent size of the full moon—in reality around 25 light-years in diameter. [81], Z Canis Majoris is a star system a mere 300,000 years old composed of two pre-main-sequence stars—a FU Orionis star and a Herbig Ae/Be star,[82] which has brightened episodically by two magnitudes to magnitude 8 in 1987, 2000, 2004 and 2008. [21] To the Boorong people of Victoria, Sigma Canis Majoris was Unurgunite (which has become the official name of this star[22]), and its flanking stars Delta and Epsilon were his two wives. [29] John Flamsteed numbered 31 stars, with 3 Canis Majoris being placed by Lacaille into Columba as Delta Columbae (Flamsteed had not recognised Columba as a distinct constellation). Find out more about how we use your information in our Privacy Policy and Cookie Policy.

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