canis major dwarf galaxy planets

This category lists pages and subcategories relating to the Canis Major Dwarf Galaxy. It is the brightest member of the open cluster NGC 2362, having an apparent magnitude of 4.40. This star is 220,000 times brighter than our Sun, having 2,140% of its mass, and 6,500% of its radius. It is part of the Phantom Zone Subsector. Printable Canis Major Constellation Worksheets, https://www.thoughtco.com/thmb/opX5lqz30agaRn3I1iyIobw6sVA=/768x0/filters:no_upscale():max_bytes(150000):strip_icc()/sirius-and-procyon-5851b5b25f9b586e02633123.jpg, https://upload.wikimedia.org/wikipedia/en/thumb/8/89/Canis_Major_on_the_Manuchihr_Globe.jpg/640px-Canis_Major_on_the_Manuchihr_Globe.jpg, https://i1.wp.com/astrobob.areavoices.com/files/2020/03/Canis-Major-finder-March_FEA.jpg?fit=936%2C399, https://upload.wikimedia.org/wikipedia/commons/thumb/c/c1/Messier_041_2MASS.jpg/574px-Messier_041_2MASS.jpg, https://upload.wikimedia.org/wikipedia/commons/c/c7/CanisMajorCC.jpg, https://upload.wikimedia.org/wikipedia/commons/thumb/c/c9/Sirius_A_and_B_artwork.jpg/640px-Sirius_A_and_B_artwork.jpg, https://nineplanets.org/wp-content/uploads/2020/01/Adhara-1024x506.jpg, https://www.star-facts.com/wp-content/uploads/2020/07/Wezen.jpg?189db0&189db0, https://www.star-facts.com/wp-content/uploads/2020/07/Mirzam.jpg?189db0&189db0, https://pm1.narvii.com/6423/ce86c1657715ab0e5cdaca4cc97845daaab58cad_hq.jpg, https://sunnymeade.files.wordpress.com/2011/12/ngc-2362-650.jpg, https://theskylive.com/sky/stars/finder-charts/furud-zeta-canis-majoris-finder-chart.png?c=1586786672, https://www.davidmalin.com/fujii/image/CMa_www.jpg, https://theskylive.com/sky/stars/star-images/25/2580_800.jpg, https://www.constellation-guide.com/wp-content/uploads/2011/03/Tau-Canis-Majoris-Cluster-NGC-2362-Caldwell-64.jpg, https://astronomy.com/~/media/5600BB6F360F469890093E7D8607560F.jpg, https://www.universetoday.com/wp-content/uploads/2008/04/vycanis-1280x720.png, https://i.ytimg.com/vi/XU0iPq_7r_E/hqdefault.jpg, https://theskylive.com/sky/stars/finder-charts/iota-canis-majoris-finder-chart.png?c=1586732293, https://qph.fs.quoracdn.net/main-qimg-059fd1b7c0713677f548c5c242a77b31, https://www.syfy.com/sites/syfy/files/styles/1170xauto/public/wire/legacy/apo_sh2308_bubble_haoiii.jpg, https://www.constellation-guide.com/wp-content/uploads/2015/02/NGC-2359-638x640.jpg, https://upload.wikimedia.org/wikipedia/commons/2/2f/NGC_2359%2C_Thor%27s_Helmet_%28core%29.jpg, https://upload.wikimedia.org/wikipedia/commons/b/b3/NGC2360_-_SDSS_DR14_%28panorama%29.jpg, https://www.jwinman.com/starcharts/images/NGC%202362.jpg, https://upload.wikimedia.org/wikipedia/commons/8/8b/NGC_2354.png, https://live.staticflickr.com/65535/48108182927_e146c5ef1f_b.jpg, https://live.staticflickr.com/8652/16002621745_5f7f071b5e_b.jpg, https://upload.wikimedia.org/wikipedia/commons/3/33/NGC2207%2BIC2163.jpg, https://www.sciencemag.org/sites/default/files/styles/article_main_large/public/images/2003110721.jpg?itok=vsVqTEw2. Only these users can officially approve pitches: The planets orbit their star with periods of 4.08 days and 3.7 years with (assuming the star to have a mass of 0.9 times that of the Sun) orbital sizes of 0.05 and 2.3 Astronomical Units. Wezen is situated at around 1,600 light-years away. Alternative names include Canis Sequens and Canis Alter. Some of the small galaxies are Elliptical Galaxies as well, often referred to as Dwarf Ellipticals. Around the year of 3457 part of the UFAG fleet refugee in Edraria seeing the war lost choose to take refuge in the Canis Major Dwarf. VY Canis Majoris is a red hypergiant or supergiant located at around 3.900 light-years away. This nebula isis 30 light-years in size. Some speculate that this open cluster is around 2.2 billion years old. Adhara, designated as Epsilon Canis Majoris, is a binary star located at around 430 light-years away from us. Wezen has an apparent magnitude of 1.824. In 2003, the Canis Major Dwarf Galaxy was discovered - this is now the closest known galaxy to ours! The Canis Major Dwarf Galaxy: a brief history! Canis Major is a southern constellation, visible in its entirety from all locations south of latitude 60°N. The other galaxy, IC 2163, is a barred spiral galaxy. It is part of the Phantom Zone Subsector. Messier 41 has an apparent magnitude of 4.5. The distance between the two stars varies between 8.2 and 31.5 AU, and they complete one orbit around each other once every 50 years. VY Canis Majoris is also among the brightest stars known to us, being around 270,000 times brighter than our Sun, yet with estimated surface temperatures cooler than our Sun, at around 3,490 K. VY Canis Majoris has an apparent magnitude that varies from 6.5 to 9.6, and it is also a fast-spinning star having a rotational velocity of around 300 km / 186.4 mi per second. All material is © Swinburne University of Technology except where indicated. Since 1943, this star’s spectrum has served as one of the stable anchor points by which other stars are classified. No meteor showers are connected to it. The primary star, Sirius A, has 206% of the Sun’s mass, and 171% of its radius. The Canis Major and Sagittarius dwarf galaxies are the two closest galaxies to us, followed by another dwarf galaxy in Ursa Major. VY Canis Majoris has around 1.700% of our Sun’s mass and a whopping 142.000 % of its radius, to put that into perspective, it would take an object traveling with the speed of light around six hours to travel around the star’s circumference, while it would only take 14.5 seconds to encircle our Sun. Welcome, ! A small, irregular galaxy with a mass of about a billion solar masses, the Canis Major dwarf galaxy is one of our closest neighbours, lying approximately 25,000 light years from the Sun and 42,000 light years from the centre of the Milky Way. There is also the yellow-white supergiant Wezen, the blue-white giant Mirzam, the blue-white supergiants Aludra and Omicron. The Greeks referred to only one dog, however, during the Roman times, Canis Minor appears as Orion’s second celestial hunting dog. Canis Major Dwarf Galaxy | United Planets Wiki | … Furud is a spectroscopic binary star. It will become a red supergiant star in the future. Currently, seven stars that host planets have been discovered in Canis Major. THE PLANETS The upper circle shows the location of the class G7 dwarf star HD 47186 in the constellation Canis Major, which has two planets, one quite small. The constellation of Canis Major was known to the ancients. Aludra is an Alpha Cygni variable star, its brightness varies from +2.38 to 2.48 over a period of 4.7 days. This star has an apparent magnitude that varies slowly and irregularly from 6.35 to 7.90. Until recently, however, this dwarf galaxy lay unobserved behind the dust and gas in the disk of the Milky Way. Mirzam is located near the far end of the Local Bubble, a cavity in the local interstellar medium through which the Sun is also traveling. Messier 41, also designated as NGC 2287, is an open cluster situated at 2,300 light-years away from Earth. Sagittarius dwarf is considered to be a colonial neighbour of the Milky Way. Canis Syrius was the name used in the 1521 Alfonsine tables. This star cluster has an apparent dimension of 38 arcminutes, having between 25 to 26 light-years in diameter. Adhara is several times hotter than our Sun, having 1,200% of the Sun’s mass, and 1,300% of its radius. The Canis Major Dwarf galaxy is located in the same part of the sky as the constellation of Canis Major. However, there remains debate over whether it represents a disrupted dwarf galaxy or in fact a variation in the thin and thick disk and spiral arm populations of the Milky Way. It is an irregular variable star, varying between apparent magnitudes 3.78 and 3.99. Galaxies change their size and volume by colliding with other galaxies as well as consuming the smaller ones. NGC 2360 has an apparent magnitude of 7.2, a diameter of around 15 light-years, and contains many red giant stars. Canis Major is located in the second quadrant of the southern hemisphere (SQ2), and it can be seen at latitudes between +60o and -90o. Muliphein is a member of the Collinder 121 open star cluster. Mirzam is a blue-white giant star located at around 490 light-years away. It has an apparent magnitude of 4.1 and a radius of around 11.2 light-years. The Canis Major Dwarf Galaxy lies some 25,000 light-years from Earth’s solar system and about 42,000 light-years from the centre of the Milky Way, which makes it the closest galaxy to the Milky Way … 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. 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. These distances put it even closer than the previous record holder, the Sagittarius dwarf galaxy discovered in 1994, which lies 50,000 and 80,000 light-years from the galactic center and Earth, respectively. They can be no larger than a Star Clusters. This is a satellite galaxy of the Milky Way Galaxy. The constellation of Canis Major contains many bright stars above magnitude 2.0, however, Sirius, the brightest star in the night sky is also situated here, having an apparent magnitude of -1.47. It is believed that the character Sirius, in the Harry Potter series, who can transform into a dog, might have been inspired by Canis Major’s brightest star. Mirzam, designated as Beta Canis Majoris, is the fourth brightest star in the constellation, having an apparent magnitude of 1.985. It has recently been settled by the Solarian Kingdom. W Canis Majoris has carbon and s-process elements dredged up to the surface during thermal pulses of its helium-burning shell. The primary star, Tau Canis Majoris, is 5,000%  more massive than our Sun, having 1,980% its radius, and being 280,000 times brighter. The other involves the Sagittarius dwarf galaxy. Classified as a K1III yellow/orange giant,it has a gas giant planet in orbit around it 2.6times the size of Jupiter. In 2003, an overdensity of stars in the region was announced to be the Canis Major Dwarf, the closest satellite galaxy to Earth. In Greek mythology, Canis Major represented the dog Laelaps, a gift from Zeus to Europa, or sometimes the hound of Procris, Diana’s nymph, or the one given by Aurora to Cephalus, so famed for its speed that Zeus elevated it to the sky. Answer to: How many planets are in the Canis Major dwarf galaxy? RX J0720.4-3125 is a neutron star first discovered in 1997 in the ROSAT All-sky survey. Omicron2 is classified as a massive supergiant of spectral type B3 la, appearing blue in color. Canis Major spreads out for over 380 square degrees. It has around 560 % of our Sun’s radius, and it is more than twice as hot, having temperatures of 13,596 K. Omicron1  Canis Majoris is a red supergiant star located at about 3,500 light-years away. The collision between these two galaxies is of great interest to astronomers since this event might reflect the probable fate of our Milky Way galaxy and the Andromeda galaxy. Monocular vs. Binoculars- Which One is Best for Stargazing. The primary star is a main-sequence star, having 770% of our Sun’s mass, 390% of its radius, and it is 3,603 times brighter than our Sun. When VY Canis Majoris will reach the end of its life, it will explode as a hypernova, an event that is over 100 times stronger than a supernova. The Adhara star system is comprised out of two stars, a blue star designated as Epsilon Canis Majoris A, and B. The Canis Major Dwarf Galaxy is a galaxy in the Local Group, located in the same part of the sky as the constellation Canis Major. The Canis Major Dwarf Galaxy's location is 07h 12m 35.0 (R.A.) and -27d 40' 0 (Dec.). NGC 2354 is a relatively fain open cluster that contains around 15 stars which are visible through binoculars. Canis Major was listed by Ptolemy as one of the 48 original constellations handed down from antiquity. There are no meteor showers associated with the Canis Major constellation. The Milky Way passes through Canis Major, and as such, several open clusters lie within its borders. It is also almost three times as hot, having surface temperatures of around 17,000 K. W Canis Majoris is a carbon star located at around 1,800 light-years away from us. Canis Major contains several notable deep sky objects: the Canis Major Dwarf Galaxy, the open cluster Messier 41, the emission nebula NGC 2359 Thor’s helmet), and the colliding spiral galaxies NGC 2207 and IC 2163. In Chinese astronomy, the constellation of Canis Major is located in the Vermilion Bird. Galactic cannibalism isn't limited to ellipticals, our galaxy is believed to be consuming the Canis Major Dwarf Galaxy. The Sirius star system is situated at around 8.6 light-years away from us, it is one of Earth’s nearest neighbors. They are closer to us than many globular star clusters that also belong to our galaxy. Canis Major spreads out for over 380 square degrees. Aludra is located at around 2,000 light-years away. The supposed small galaxy contains a relatively high percentage of red giant stars, and is thought to contain an estimated one billion stars in all. The galaxy contains a relatively high percentage of red giant stars, and is thought to contain an estimated one billion stars in all. Adhara is 38,700 times brighter than the Sun. the Canis Major Overdensity. The brightest star in Canis Major is Sirius, which is also the brightest star in the night sky, having an apparent magnitude of -1.46. An artist’s impression of the Monoceros Ring, which wraps three times around the, Centre for Astrophysics and Supercomputing, COSMOS - The SAO Encyclopedia of Astronomy, Study Astronomy Online at Swinburne University. Study Astronomy Online at Swinburne University Since they are low-mass, sparsely populated galaxies, they may or may not be able to form planets where life can exist. The Canis Major Dwarf Galaxy is estimated to contain 1 billion stars, many of which are red giants. The nebula contains hundreds of solar masses of ionized material and unionized gas. This galaxy is situated at around 42,000 light-years away from the Galactic Center. Wezen lies around 10 degrees south southeast of Sirius. There are no meteor showers associated with the Canis Major constellation. Sirius isn’t, however, a single star, it is a binary star consisting of a main-sequence star of spectral type A0, termed Sirius A, and a faint white dwarf companion designated as Sirius B. Muliphein, designated as Gamma Canis Majoris, is a blue-white B-type bright giant star located at around 440 light-years away. WR 7 is 19.3 times hotter than our Sun, having temperatures of around 112,000 K. The constellation of Canis Major contains several interesting deep-sky objects as well, such as the Canis Major Dwarf Galaxy, the open cluster Messier 41, the emission nebula NGC 2359 – also known as Thor’s Helmet, or the colliding spiral galaxies NGC 2207 and IC 2163. RX J0720.4-3125 is part of the Magnificent Seven, a group of neutron stars that are relatively near to our Solar System. Sirius, also designated as Alpha Canis Majoris, is the brightest star in Canis Major, and overall the brightest in the night sky. Canis Major is a constellation located in the southern celestial hemisphere. This star is quite young, being only 8.2 million years old, however, it will not live for long. It is among the largest known stars ever discovered. The primary star is a Wolf-Rayet type of star, being among the top ten brightest Wolf-Rayet stars. The Canis Major dwarf galaxy (CMa dwarf) or Canis Major overdensity (CMa overdensity) is a disputed dwarf irregular galaxy in the Local Group. Iota Canis Majoris is 47,000 times brighter than our Sun, having 1,250% of its mass, and around 2,590% of its radius. NGC 2207 and IC 2163 are a pair of colliding spiral galaxies that are located at around 80 million light-years away from us. With a mass only 1% of that of the Milky Way, this is one of two minor mergers known to be currently occurring in the Milky Way. The constellation of Canis Major contains several interesting deep-sky objects as well, such as the Canis Major Dwarf Galaxy, the emission nebula NGC 2359 – also known as Thor’s Helmet, or the colliding spiral galaxies NGC 2207 and IC 2163. Looking up on more info, there's a ton of satellite galaxies from 70k-1.3m ly from Sol. For comparison, Sirius is twice as bright as Canopus, the second-brightest star in the night sky. Muliphein has an apparent magnitude of +4.10. NGC 2362 is believed to have been discovered before 1654. It is 43rd in size of the 88 internationally recognised modern constellations. This small star is located at around 1,200 light-years away. Iota Canis Majoris is a blue-white supergiant star located at around 3,100 light-years away. Most distant galaxy GN-z11 : Ursa Major: z=11.09 With an estimated distance of about 32 billion light-years (comoving distance,) or 13.4 GLY (light-travel distance,) astronomers announced it as the most distant astronomical galaxy known. Wezen, also designated as Delta Canis Majoris, is a yellow-white F-type supergiant star, being the third brightest star in Canis Major. It is known as the “dog star”. They only managed to reach the galaxy with the use of experimental wormhole drives which allow fleets of ships to move from the Milky Way to the Canis Major galaxy. How to choose your telescope magnification? The Maori and Tuamotus people recognized the figure of Canis Major as a distinct entity. Closest galaxy Canis Major Dwarf: Canis Major: 0.025 Mly Discovered in 2003, a satellite of the Milky Way, slowly being cannibalised by it. Canis Major contains one Messier object, the star cluster Messier 41 (NGC 2287), and has four stars with known planets. EZ Canis Majoris has an apparent magnitude that varies from 6.71 to 6.95 over a period of 3.76 days. The Canis Major Galaxy is the nearest dwarf galaxy to the Milky Way. Sirius is also known as the Dog Star, reflecting its prominence in its constellation – Canis Major – the celestial Greater Dog. This star is a chemically peculiar Hg-Mg star having abnormal lines of magnesium and mercury in its spectrum. If you are a new user, and would like to contribute to this galaxy, please create a pitch first. Its name is Latin for “Greater Dog” in contrast to Canis Minor the  “Lesser Dog”. So not that unviable at all for a FC if it could travel in a more freely way and use all that tritium it carries. This cluster has an apparent magnitude of 6.5. The cluster is in relation with the giant nebula Sh2-310. The Canis Major Dwarf Galaxy: The Epilogus of the Andarian Andromeda Wars The colonization of the Canis Major Dwarf Galaxy and the integration in the Imperial Galactic Republic . HD 56925, also designated as WR 7, is also a Wolf-Rayet star, located at around 17,000 light-years away from us. Tau Canis Majoris is a multiple star system located at around 5,000 light-years away. As the CMa Dwarf Galaxy is small, there is not much influence on our galaxy from consuming it. Gravitational interactions with the Milky Way have stripped long tidal tails from the Canis Major dwarf galaxy, which have wrapped themselves around the Milky Way three times in a structure known as the ‘Monoceros Ring’. Probably billions A small, irregular galaxy with a mass of about a billion solar masses, the Canis Major dwarf galaxy is one of our closest neighbors, lying approximately 25,000 light years from the Sun and 42,000 light years from the center of the Milky Way. 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