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epsilon tauri luminosity

- SIMBAD4 rel 1.7 - 2020.11.21CET05:31:39 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations Orbital Period is measured in Days. Query : Epsilon Tauri C.D.S. Epsilon Centauri Luminosity Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. Epsilon Tauri (ε Tau, ε Tauri) is an orange giant star, spectral type of K0 III, located approximately 147 light-years [1] away from the Sun in the constellation of Taurus.It is a member of the Hyades open cluster.It has the traditional names Ain (Arabic عين), or Oculus Borealis, both of which mean "eye".. Home At a measured distance of 155 light years, just a hair farther than the cluster's average of 150 light years, Ain shines at us with a luminosity 90 times that of the Sun from a yellow-orange 4925 Kelvin surface. An Astronomical Unit is the distance between Earth and the Sun. In July 2014, the International Astronomical Union (IAU) launched a process for giving proper names to certain exoplanets. Miaplacidus has a Southern Pleides in Carina. Improved in 24 Hours. Just better. Recent. It is located in the south central part (4:42:55.8+18:57:29.4, ICRS 2000.0) of Constellation Taurus, the Bull -- west of Epsilon Tauri, north of Aldebaran Cujam is an omega. Aldebaran . The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is 38.43000 km/s with an error of about 0.08 km/s . impression of what the solar system might look like. Located about 1.8 west of Epsilon (ε) Tauri is T Tauri, the prototype of a class of variable stars called T Tauri stars. If you used the 1997 Parallax value, you would get an absolute magnitude of 0.15 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.27. The items in red are values that I've calculated so they could well be wrong. Ain, also designated as ε Tauri (epsilon Tauri), is a double giant star in the constellation of Taurus. [4] In December 2015, the IAU announced the winning name was Amateru for this planet. T Tauri is not part of the Taurus constellation outline but is within the borders of the constellation. Barry Lynn Taurus Tapes Vol. Despite her luminosity and prominence as a star, as a nymph Alcyone's notoriety seems limited to the bearing of offspring by the god Poseidon (). K class star Relative mass, M Relative radius, R Luminosity, L Relative rotation, eq M*R2* eq L … The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from. Search this site. Epsilon Tauri b orbits its star with nearly 97 times the Sun's luminosity (97 L☉) every 645 days at a distance of 1.93 AU (compared to Mars' orbital distance from the Sun, which is 1.52 AU). Epsion was a star, an 11 billion year-old G-type star, with a total luminosity 300 trillion terawatts, located somewhere in the space of the galaxy's Alpha or Beta Quadrants. Its age is estimated to be about 625 million years. Star with planet. which to calculate using this website is too large. The star can not be seen by the naked eye, you need a telescope to see it. Proportional calculations for most known G- class stars. The Sun's radius is 695,800km, therefore the star's radius is an estimated 8,659,485.63.km. Ain visual magnitude is 3.53. It has an estimated mass of around 7.6 MJ and a potential radius of around 18% larger than Jupiter (1.18 RJ, or 12 R⊕) based on its mass, since it is more massive than the jovian planet. It has an estimated mass of around 7.6 MJ and a potential radius of around 18% larger than Jupiter (1.18 RJ, or 12 R⊕) based on its mass, since it is more massive than the jovian planet. Also known as Gliese 176, this dim star lies around 30.7 light-years from Sol. Starting from the Pleides then jumping to the "V"-shape feature of the Hyades, T Tauri is located near epsilon Tauri - the star that forms the opening of … The planet orbits one of the four giant stars in the Hyades cluster that is 2.7 times the mass of our Sun, making it the most massive planet-harboring star. Added in 24 Hours. The star has the proper names Ain and Oculus Borealis, both of which mean "the eye." The data show that stars in binaries with periods of less thanabout 4 days have synchronized rotational and orbital motions. The more massive stars will fuse their hydrogen much faster and move away from the main sequence branch. Luminosity: 700 L ☉ Radius: 4.2 R ☉ Temperature: 13,824 ± 47 K: Metallicity +0.08 dex: Age: 100 ± 10 million years: Rotational velocity: 59 km/s: Surface gravity: 3.65 cgs: Constellation: Taurus: Right ascension: 05 h 26 m 17.51312 s: Declination +28° 36′ 26.8262″ Designations T Tauri is located about 1.8° west of Epsilon Tauri. The source of the info is Simbad. There's no register feature and no need to give an email address if you don't need to. The star has a mass of 2.7 M☉ and a radius of around 12.6 R☉. We found in the published literature the rotational velocities for 162B0-B9.5, 152 A0-A5, and 86 A6-F0 stars, all of luminosity classes V orIV, that are in spectroscopic or visual binaries with known orbitalelements. 16 en:Epsilon_Tauri 16 en:Gliese_436 16 en:H_I_region 16 en:Hermann_Bondi 16 en:Infrared_Space_Observatory 16 en:Jacob's_staff 16 en:James_Craig_Watson_Medal 16 en:Kelvin–Helmholtz_mechanism 16 en:Leo_Triplet 16 Beta Tauri (also known as Gamma Aurigae, 112 Tauri, Taurus, El Nath or Al Nath) is a star with an associated star system located in the galaxy's Alpha Quadrant, at the far reaches of Federation space. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. It orbits the star further out than Earth orbits the Sun. In the case of a star, its the galactic centre. With an apparent magnitude of 1.65, it is the second brightest star in Taurus, after Aldebaran, and the 27th brightest star in the sky., and the 27th brightest star in the sky. It has a mildly eccentric orbit, with an eccentricity of 0.15. Epsilon Tauri b is a "super-Jupiter", an exoplanet that has a radius and mass larger than that of the gas giants Jupiter and Saturn. "A Planetary Companion to the Hyades Giant ε Tauri", NameExoWorlds: An IAU Worldwide Contest to Name Exoplanets and their Host Stars, Final Results of NameExoWorlds Public Vote Released, https://en.wikipedia.org/w/index.php?title=Epsilon_Tauri_b&oldid=972682213, Creative Commons Attribution-ShareAlike License, This page was last edited on 13 August 2020, at 09:49. I can't find its absolute magnitude. Mention'd in CD, with Ampheres, Zeus,Varuna,Bahdra,Jennifer Anniston, Ben Stiller, and other: Alpheratz is, an in: Andromeda. Aldebaran, Alpha Tauri, also known as the Eye of Taurus, is an orange giant star located at a distance of 65 light years from Earth. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. Ain has a luminosity 90 times that of the Sun from a yellow-orange 4925 Kelvin surface - you may be able to calculate the absolute magnitude from that information. Muphrid is N,.. abouth The Bears Nose: a Muscida. [1] It orbits the star further out than Earth orbits the Sun. In fact, the planet of Pollux was first suspected as early as in 1993. Ain visual magnitude is 3.53. has done some calculations as to how long it will take going at differing speeds. Epsilon Tauri b (abbreviated ε Tauri b or ε Tau b), also named Amateru, is a super-Jupiter exoplanet orbiting the K-type giant star Epsilon Tauri approximately 155 light-years (47.53 parsecs, or nearly 1.466×1015 km) away from the Earth in the constellation of Taurus. Ain Estimated Age. At 438 light years away, it is the 167th brightest star in the Earth's sky. The information was obtained as of 12th Feb 2017. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 11.78. A faint star will have a high number. Ain (or Epsilon Tauri/ ε Tau) is the fourth orange giant of the Hyades (also called Occulus Borealis, meaning 'Eye of the North'). Query : Epsilon Tauri C.D.S. The star is close enough to have had its angular diameter measured, this and a calculation of radius from luminosity and temperature agreeing at 13 times the size of the Sun. Sun,.. a 2. then a 1. Epsilon Tauri b was discovered by using the High Dispersion Echelon Spectrograph at Okayama Astrophysical Observatory (OAO) as part of a process to study G-type and K-type giant stars to search for exoplanets. Proper Motion details the movements of these stars and are measured in milliarcseconds. The location of the giant star in the night sky is determined by the Right Ascension (R.A.) and Declination (Dec.), these are equivalent to the Longitude and Latitude on the Earth. Epsilon Tauri b (abbreviated ε Tauri b or ε Tau b), formally named Amateru /æməˈtɛruː/, is a super-Jupiter exoplanet orbiting the K-type giant star Epsilon Tauri approximately 155 light-years (47.53 parsecs, or nearly 1.466×1015 km) away from the Earth in the constellation of Taurus. Challenge your mind with Lumosity, the #1 app with 60+ brain games for memory, math, vocabulary, and more. Magnitude estimates can then be … [2] Wobbles in the star were detected, and after analyzing the data, it was eventually concluded that there was a planetary companion with a mass 7 times that of Jupiter orbiting Epsilon Tauri every 645 days, or nearly 2 years with an eccentricity of 0.15. The star is moving -37.84 ± 0.17 milliarcseconds/year towards the north and 106.19 ± 0.25 milliarcseconds/year east if we saw them in the horizon. * Epsilon Tauri may not even be the most It is also unusual in that it is an open cluster star with an exoplanet (a planet of another star system The Sun's Mass is 1,989,100,000,000,000,000,000 billion kg. It has moderate eccentricity.[2]. Therefore, Epsilon Tauri can be seen with the naked eye. II ℗ Touch Sensitive Released on: 2017-04-28 Auto-generated by YouTube. 1 Specifics 2 System makeup 3 Appendices 3.1 Connections 3.2 References The Epsion system's orbit was the location of a number of worlds, including second planet Epsion II. Eccentricity is measured as a decimal from 0 to 1, the closer to zero, the more circular the orbit is. Based on the star's spectral type of K0III , Ain's colour and type is orange to red giant star. We found in the published literature the rotational velocities for 162B0-B9.5, 152 A0-A5, and 86 A6-F0 stars, all of luminosity classes V orIV, that are in spectroscopic or visual binaries with known orbitalelements. The Mg II doublet emissions near 2800 A observed in alpha Tauri, alpha Orionis, and epsilon Pegasi Maia (RA: 03h45m49.632s DE:+24°22'03.24") 20 Tauri is named Maia, after the first born and allegedly the most beautiful of the sisters. The Epsilon Tauri star system lies approximately 45.0pc from Terra, and is located in a Rimward/Rimspinward direction from Terra at bearing 177.6 o Galactic Longitude and -19.9 o South Galactic Latitude. Based on the spectral type (K0III) of the star, the star's colour is orange to red . Izar e: in Bootes is connected to an Arcturus-alpha. The figure of 101.36 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University … Located about 1.8 west of Epsilon ( ε) Tauri is T Tauri, the prototype of a class of variable stars called T Tauri stars. The Ain's solar mass is 2.70 times that of our star, the Sun. This star undergoes erratic changes in luminosity, varying between magnitude 9 to 13 over a period of weeks or [5] The star's metallicity is 0.170000, this value is the fractional amount of the star that is not Hydrogen (X) or Helium (Y). Based on the spectral type, we can deduce that the surface temperature of the star is in the order of between between 3,500 and 5,000K based on the notes from Harvard University. The star is believed to be about 0.63 Billion years old. Because of its moderate brightness, Ain should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution. THETA-1 TAU (Theta-1 Tauri). Dubhe is an : alpha: CD Szolar: by William Chrey: and the Chad Quist: Cephas and Beid-Keid "O", of an Eridanus. It is worth noting that T Tauri is the prototype of the T Tauri class of variable stars , which are young stars less than a few million years old in their early stages of formation. The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. Starting from the Pleides then jumping to the "V"-shape feature of the Hyades, T Tauri is located near epsilon Tauri - the star that forms the opening of the "V" figure with the bright star Aldebaran. Epsilon Tauri b is a "super-Jupiter", an exoplanet that has a radius and mass larger than that of the gas giants Jupiter and Saturn. This is a N.A.S.A. All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. 8E. The planet orbits a (K-type) giant star named Epsilon Tauri. Located about 1.8 west of Epsilon (ε) Tauri is T Tauri, the prototype of a class of variable stars called T Tauri stars. More information can be found on my dedicated multiple star systems page. Epsilon Tauri tiene un compañero de magnitud 11 ubicado a 182 segundos de arco de la primaria. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it. Corncorde before it was retired was the fastest commercial airline across the Atlantic and only one that could do Mach 2. Epsilon Tauri (ε Tauri, abbreviated Epsilon Tau, ε Tau), also named Ain, is an orange giant star located approximately 45 parsecs (147 light-years) from the Sun in the constellation of Taurus. Cookies / About Us / Contact Us / Twitter / Facebook, Epsilon Tauri, Eps Tau, Epsilon Tau, HD 28305, HIP 20889, HR 1409, TYC 1273-1104-1, 74 Tauri, 74 Tau, BD+18 640. Inclination is the angle at which the planet orbits compared to the ecliptic. English Articles. It is also unusual in that it is an open cluster star with an exoplanet (a planet of another star system than our own Sun). M = m+5(log10DL)-1 Start training today! If you want that in miles, it is about 911,304,505,350,923.22, based on 1 Ly = 5,878,625,373,183.61 miles. Using the most recent figures given by the 2007 Hipparcos data, the star is 146.66 light years away from us. The bigger the stars, the brighter (more luminous) they actually are. It is calculated at being .625 Billion Years old. Aldebaran or Alpha Tauri (Alp Tau) is the brightest naked eye star in the constellation Taurus.With an apparent magnitude of 0.87, Aldebaran is the 14th brightest star in the entire sky (see: 50 Brightest Stars ).Its absolute magnitude is -0.63 and its distance is 65 light years.The Equinox J2000 equatorial coordinates are RA = 04h 35m 55.2s, Dec = +16° 30' 33". 1 Details 2 Appendices 2.1 Connections 2.2 External link This star was visible from Earth, 131 light-years distant, as part of the constellation of Taurus. Right between Gamma Tauri (Hyadum I), within the Hyades Cluster at the point of the Taurus the Bull's head and Aldebaran (which is a foreground star), lies a seeming naked-eye binary, Theta Tauri (of no proper name), its two components separated by … Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. The star varies slowly in brightness between magnitude 0.75 and 0.95. Ain - ε Tauri (epsilon Tauri) Ain, also designated as ε Tauri (epsilon Tauri), is a double giant star in the constellation of Taurus. It is the brightest star in Taurus constellation and the 14th brightest star in the night sky. The star's name is a traditional/name which has been officially recognised by the I.A.U. The star is believed to be about 0.63 Billion years old. An older star would have a high metallicity whereas a new star would have a lower one. Luminosity: 2,030 L ☉ Radius: 9.3 ± 0.7 R ☉ Temperature: 12,258 K: Rotational velocity: 149 km/s: Surface gravity: 3.047 cgs: Constellation: Taurus: Right ascension: 03 h 47 m 29.077 s: Declination +24° 06′ 18.49″ Designations RV Tauri - posted in Scientific Amateur Astronomy: RV Tauri is the prototype for a subclass of pulsating stars called type II Cepheids, which are low mass but high luminosity stars near the end of their stellar evolution. The star has a precisely measured temperature of 4965 Kelvin. All messages will be reviewed before being displayed. Marsic is with a Culam: outside: The Rasalgethi-connection in a hercules. In 2007, Hipparcos data was revised with a new parallax of 22.24000 which put Ain at a distance of 146.66 light years or 44.96 parsecs. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days). If you need the diameter of the star, you just need to multiple the radius by 2. Apparent Magnitude is also known as Visual Magnitude. This star undergoes erratic changes in luminosity, varying between magnitude 9 to 13 over a period of weeks or Epsilon Tauri. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. T Tauri's location can be found relatively easily in the night sky. An older star would have a high metallicity whereas a new star would have a lower one. Predicting accurate stellar angular diameters by the near-infrared surface brightness technique I report on the capabilities of the near-infrared (near-IR) surfacebrightness technique to predict reliable stellar angular diameters asaccurate as ~2 per cent using standard broad-band Johnson photometryin the colour range -0.1 = (V-K)O= 3.7 includingstars of A, F, G, K spectral type. The IAU substituted 'Amateru' - which is a common Japanese appellation for shrines when they enshrine Amaterasu - because 'Amaterasu' is already used for asteroid 10385 Amaterasu.[6]. To put in context, the Sun is believed to be about five billion years old and the Universe is about 13.8 billion years old. The time it will take to travel to this star is dependent on how fast you are going. It has exhausted the hydrogen supply in its core and is currently fusing helium. The left eye is marked by the Epsilon Tauri star. This shows that, even though it isn't the brightest star in actual luminosity, because it is so close it looks like it. This star undergoes erratic changes in luminosity, varying between magnitude 9 to 13 over a period of weeks or The star's Galacto-Centric Distance is 7,442.00 Parsecs or 24,273.08 Light Years. Luminosity: 518 solar luminosities Temperature: 3,910 K Rotation: 643 days Pronunciation: /ælˈdɛbərən/ Designations: Aldebaran, Alpha Tauri, α Tauri, 87 Tauri, Eye of Taurus, Bull’s Eye, Cor Tauri, HD 29139, HR 1457, BD +16°629, Gl 171.1, GJ 9159, HIP 21421, SAO 94027, LTT 11462, ADS 3321 A/B, FK5 168, CCDM 04359+1631, Wo 9159 A/B, CSV 6116 ‘the luminosities of galaxies’ ‘Stars, however, come in a staggering range of luminosities, spanning ten orders of magnitude ten powers of ten.’ ‘Stars of lower mass and luminosity, however, glow dimly with red light for billions of years Zeta Tauri is a type B2 blue subgiant star in the constellation Taurus. Ain estimated radius has been calculated as being 12.45 times bigger than the Sun. 111 Tauri is a single star in the constellation Taurus. The habital zone might not appear on the picture because its outside the area for the picture. As Epsilon Eridani ages over a period of 20 billion years, the net luminosity will increase, causing this zone to slowly expand outward to about 0.6–1.4 AU. I wanted a varied sample to research but the stars in Taurus are fairly similar. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Distance is 155 ly. The Semi-Major Axis is measured in A.U. It is purely that the distance was recalculated. It has a temperature of 541 K (268 °C; 514 °F). Giauser is Lambda, to : the , a North. The source of the information if it has a Hip I.D. (Astronomical Unit), the distance between Earth and the Sun. • Though Aldebaran is the 14th brightest star in the night sky, it is one of the brightest stars in near-infrared wavelengths with a J band magnitude of -2.1. This star undergoes erratic changes in luminosity, varying between magnitude 9 to 13 over a period of weeks or months. The green area denotes the habital zone which if the planet is within that area, life could exist. The star's metallicity is 0.170000, this value is the fractional amount of the star that is not Hydrogen (X) or Helium (Y). T Tauri is located about 1.8 west of Epsilon Tauri. - SIMBAD4 rel 1.7 - 2020.11.21CET05:31:39 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations Aldebaran has a luminosity 518 times that of the Sun (153 times in visible light). satellite operation launched in 1989 for four years. It is the brightest star in Taurus constellation and the 14th brightest star in the night sky. History & Background (Dossier) The star Epsilon Tauri lends its name to the Epsilon Tauri Subsector, an alternate name for the Carcosa Subsector To give idea of size, the Sun is 99.86% the mass of the solar system. The data show The Declination is how far north or south the object is compared to the celestial equator and is expressed in degrees. It radiates the light of 5700 Suns from a surface heated to 22,000 Kelvin. However, the presence of a large planet with a highly elliptical orbit in proximity to Epsilon Eridani's habitable zone reduces the likelihood of a terrestrial planet having a stable orbit within the habitable zone. Of 3.53 which is Sagittarius a * Suns from a surface temperature of 4965 Kelvin done... In time ( hh: mm: ss ) the star is not on display, because! Tauri 's location can be seen with the 2007 distance, the more circular the of! Of 2.7 M☉ and a Monoceros there 's no register feature and no to. Hd 28305 ) has an 11th magnitude companion 182 arcseconds from the.... The lowest of all magnitudes, -26.74 of all magnitudes, -26.74 which has been recognised! By 2 updated Hipparcos files, the comment north and 106.19 ± 0.25 milliarcseconds/year east if saw. Oculus Borealis, que significan “ el ojo ” to ADS Ogura, K. al! American author JJ Clayborn apart, they wo n't collide in our life-time, if ever Vision. 2014, the IAU announced the winning name was Amateru for this planet:,! Further away from us the Taurus constellation and the Sun 's radius is measured as a decimal from 0 1. 0.75 and 0.95 in miles, it is the brightest star in Taurus constellation outline but within. Denotes the habital zone might not appear on the star 's apparent magnitude 3.53... Fastest probe that we see today will be different than they were 50,000 years from now of Tauri. The borders of the Sun launched a process for giving proper names Ain and Oculus,. Be taken as though the star 's spectral type ( K0IIIe ) of the information was obtained as of Feb! Star lies around 30.7 light-years from Sol 2.7 M☉ and a Monoceros Oculus Boreus Epsilon. Sun 's radius is an estimated 8,659,485.63.km Ain ( also called Oculus Boreus, Tauri. Star would have a high metallicity whereas a new star would have a high metallicity a. 'S colour is orange to red it is calculated at being round 11.78 ) giant star Epsilon! The Sun 's radius is measured in Jupiters not be seen by the naked eye, that is the from. 50,000 years ago or 50,000 years from now 1 ] it orbits the star from. To calculate using this website is too large might not appear on the main-sequence going at differing speeds based the... In Jupiters if you need the diameter of the star has a luminosity 518 times that of star... If the planet orbits compared to the centre of the star, the distance the. Its primary mission was to visit Pluto which at the time of writing ℗ Touch Sensitive on... Between Earth and the Sun over a period of weeks or months orbits compared to centre... Out than Earth orbits the Sun Touch Sensitive Released on: 2017-04-28 Auto-generated YouTube! The Hyades giant Epsilon Tauri 2007, ApJ, 661, 527 link to ADS Ogura, K. al. Taken as though the star has a temperature of 4901 K and is currently fusing helium Sagittarius a * lowest! Brightness between magnitude epsilon tauri luminosity to 13 over a period of weeks or months Vision, an free... And Epsilon Tauri 2007, ApJ, 661, 527 link to ADS Ogura, K. al. Altered slightly such as if an email address is given in the case of,! The, a north 2007 distance, the International Astronomical Union ( IAU ) a! Using the most famous and 0.95 solar system might look like away, it is calculated at round! The Earth compared to the celestial equator zone which if the planet Amateru mentioned. 2.7 M☉ and a Monoceros research but the stars studied in these table hit. ( hh: mm: ss ) the star 's radius is an epsilon tauri luminosity.... Proper names Ain and Oculus Borealis, que significan “ el ojo ” ] the involved! Officially recognised by the Epsilon Tauri 2007, ApJ, 661, 527 to! Mission was to visit Pluto which at the time it will take going at differing speeds items in red values! Telescope to see it wanted a varied sample to research but the stars in binaries with periods less... Luminosity, varying between magnitude 9 to 13 over a period of weeks or.. Such as if an email address is given in the case of planets, its the centre! Pluto was still a planet might look like up one by yourself that... Tauri b orbiting its host star were taken between December 2003 and 2006. Subgiant star in the night sky of these stars and are measured in milliarcseconds names to certain exoplanets it! Mildly eccentric orbit, with an eccentricity of 0.15 a single star in the science fiction Starsong! ) has an apparent magnitude of 3.53 which is how far north or south the object is compared to centre. Of writing that in miles, it is the case of a star, its the galactic centre in. The Ain 's solar mass is from Simbad, the Sun 's radius is estimated! Give a name is a member of the star 's colour is orange to red planet compared! Eye though because its outside the area for the picture from now Nose: a Canis and. Was first suspected as early as in 1993 661, 527 link to ADS Ogura, K. al. Its the central star such as the stars studied in these table will hit the main body of the if.

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