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With an apparent visual magnitude of 3.4, this star is bright enough to be seen with the naked eye. The star's Galacto-Centric Distance is 7,386.00 Parsecs or 24,090.42 Light Years. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. To give idea of size, the Sun is 99.86% the mass of the solar system.Vindemiatrix Iron Abundance is 0.13 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. A name is preferred even if its a random made up one by yourself. The number of A.U. Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 31.90000 which gave the calculated distance to Vindemiatrix as 102.25 light years away from Earth or 31.35 parsecs. It should not be taken as though the star is moving closer or further away from us. is from There's no register feature and no need to give an email address if you don't need to. Minelauva has an apparent magnitude of 3.39 which is how bright we see the star from Earth. The figure of 502.59 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. The value comes from the Hipparcos Extended Catalog. The star is moving -52.83 ± 0.14 milliarcseconds/year towards the north and -469.99 ± 0.22 milliarcseconds/year east if we saw them in the horizon. A faint star will have a high number. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. Minelauva brightness ranges from a magnitude of 3.483 to a magnitude of 3.414 over its variable period. Its variable/pulsating period lasts for 0.1 days (variability). which to calculate using this website is too large.
The Variable Type is usually named after the first star of that type to be spotted. has done some calculations as to how long it will take going at differing speeds. Apparent Magnitude is also known as Visual Magnitude.
The number of A.U. A name is preferred even if its a random made up one by yourself. If you want that in miles, it is about 601,089,444,408,024.12, based on 1 Ly = 5,878,625,373,183.61 miles.In 2007, Hipparcos data was revised with a new parallax of 29.76000 which put Vindemiatrix at a distance of 109.60 light years or 33.60 parsecs. An Astronomical Unit is the distance between Earth and the Sun. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. The Sun's radius is 695,800km, therefore the star's radius is an estimated 18,987,682.77.km. 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. is from There's no register feature and no need to give an email address if you don't need to.
The time it will take to travel to this star is dependent on how fast you are going.
The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. It is purely that the distance was recalculated.
A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).The source of the information if it has a Hip I.D. The Declination is how far north or south the object is compared to the celestial equator and is expressed in degrees. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 26.79089054689210477331589666. The figure of 93.31 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. The time it will take to travel to this star is dependent on how fast you are going. The star's effective temperature is 5,086 Kelvin which is cooler than our own Sun's effective Temperature which is 5,777 Kelvin Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. If the R.A. is positive then its eastwards. Using the 2007 distance, the star is roughly 12,547,000.74 Astronomical Units from the Earth/Sun give or take a few. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. For Minelauva, the location is 12h 55m 36.48 and +03° 23` 51.4 . The value comes from the Hipparcos Extended Catalog. Using the 2007 distance, the star is roughly 3,768,431.75 Astronomical Units from the Earth/Sun give or take a few.
The star is a pulsating Semi-Regular Star w variable type which means that its size changes over time. Based upon parallax measurements, it is located at a distance of about 198 light-years from the Sun. The star's Galacto-Centric Distance is 7,394.00 Parsecs or 24,116.52 Light Years. Vindemiatrix has an apparent magnitude of 2.85 which is how bright we see the star from Earth. If you want that in miles, it is about 601,089,444,408,024.12, based on 1 Ly = 5,878,625,373,183.61 miles.
A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).
Distance: 35.65 ± 0.09 ly (10.93 ± 0.03 pc) Absolute magnitude (M V) 3.41: Details; Mass: 1.25 M ☉ Radius: 1.681 ± 0.008 R ☉ Luminosity: 3.572 ± 0.052 L ☉ Surface gravity (log g) 4.25 cgs: Temperature: 6,132 ± 26 K: Metallicity [Fe/H] 0.20 dex: Rotational velocity (v sin i) … Distance to Vindemiatrix. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. As it has used up its primary energy, it doesn`t have the mass that it needs to keep its size and therefore has grown.
An Astronomical Unit is the distance between Earth and the Sun. has done some calculations as to how long it will take going at differing speeds.
In the case of a star, its the galactic centre. If the R.A. is positive then its eastwards.
The star has a B-V Colour Index of 1.57 which means the star's temperature is about 3,850 Kelvin. The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -14.19000 km/s with an error of about 0.16 km/s .
Minelauva estimated radius has been calculated as being 27.29 times bigger than the Sun.
With an apparent visual magnitude of 3.4, this star is bright enough to be seen with the naked eye. The star's Galacto-Centric Distance is 7,386.00 Parsecs or 24,090.42 Light Years. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. To give idea of size, the Sun is 99.86% the mass of the solar system.Vindemiatrix Iron Abundance is 0.13 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. A name is preferred even if its a random made up one by yourself. The number of A.U. Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 31.90000 which gave the calculated distance to Vindemiatrix as 102.25 light years away from Earth or 31.35 parsecs. It should not be taken as though the star is moving closer or further away from us. is from There's no register feature and no need to give an email address if you don't need to. Minelauva has an apparent magnitude of 3.39 which is how bright we see the star from Earth. The figure of 502.59 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. The value comes from the Hipparcos Extended Catalog. The star is moving -52.83 ± 0.14 milliarcseconds/year towards the north and -469.99 ± 0.22 milliarcseconds/year east if we saw them in the horizon. A faint star will have a high number. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. Minelauva brightness ranges from a magnitude of 3.483 to a magnitude of 3.414 over its variable period. Its variable/pulsating period lasts for 0.1 days (variability). which to calculate using this website is too large.
The Variable Type is usually named after the first star of that type to be spotted. has done some calculations as to how long it will take going at differing speeds. Apparent Magnitude is also known as Visual Magnitude.
The number of A.U. A name is preferred even if its a random made up one by yourself. If you want that in miles, it is about 601,089,444,408,024.12, based on 1 Ly = 5,878,625,373,183.61 miles.In 2007, Hipparcos data was revised with a new parallax of 29.76000 which put Vindemiatrix at a distance of 109.60 light years or 33.60 parsecs. An Astronomical Unit is the distance between Earth and the Sun. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. The Sun's radius is 695,800km, therefore the star's radius is an estimated 18,987,682.77.km. 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. is from There's no register feature and no need to give an email address if you don't need to.
The time it will take to travel to this star is dependent on how fast you are going.
The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. It is purely that the distance was recalculated.
A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).The source of the information if it has a Hip I.D. The Declination is how far north or south the object is compared to the celestial equator and is expressed in degrees. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 26.79089054689210477331589666. The figure of 93.31 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. The time it will take to travel to this star is dependent on how fast you are going. The star's effective temperature is 5,086 Kelvin which is cooler than our own Sun's effective Temperature which is 5,777 Kelvin Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. If the R.A. is positive then its eastwards. Using the 2007 distance, the star is roughly 12,547,000.74 Astronomical Units from the Earth/Sun give or take a few. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. For Minelauva, the location is 12h 55m 36.48 and +03° 23` 51.4 . The value comes from the Hipparcos Extended Catalog. Using the 2007 distance, the star is roughly 3,768,431.75 Astronomical Units from the Earth/Sun give or take a few.
The star is a pulsating Semi-Regular Star w variable type which means that its size changes over time. Based upon parallax measurements, it is located at a distance of about 198 light-years from the Sun. The star's Galacto-Centric Distance is 7,394.00 Parsecs or 24,116.52 Light Years. Vindemiatrix has an apparent magnitude of 2.85 which is how bright we see the star from Earth. If you want that in miles, it is about 601,089,444,408,024.12, based on 1 Ly = 5,878,625,373,183.61 miles.
A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).
Distance: 35.65 ± 0.09 ly (10.93 ± 0.03 pc) Absolute magnitude (M V) 3.41: Details; Mass: 1.25 M ☉ Radius: 1.681 ± 0.008 R ☉ Luminosity: 3.572 ± 0.052 L ☉ Surface gravity (log g) 4.25 cgs: Temperature: 6,132 ± 26 K: Metallicity [Fe/H] 0.20 dex: Rotational velocity (v sin i) … Distance to Vindemiatrix. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. As it has used up its primary energy, it doesn`t have the mass that it needs to keep its size and therefore has grown.
An Astronomical Unit is the distance between Earth and the Sun. has done some calculations as to how long it will take going at differing speeds.
In the case of a star, its the galactic centre. If the R.A. is positive then its eastwards.
The star has a B-V Colour Index of 1.57 which means the star's temperature is about 3,850 Kelvin. The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -14.19000 km/s with an error of about 0.16 km/s .
Minelauva estimated radius has been calculated as being 27.29 times bigger than the Sun.