Minelauva has an apparent magnitude of 3.39 which is how bright we see the star from Earth. The value comes from the Hipparcos Extended Catalog. When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Minelauva, also designated as δ Virginis (delta Virginis), is a variable and double giant star in the constellation of Virgo. It is purely that the distance was recalculated. Thank you! Improved in 24 Hours. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*. is the number of times that the star is from the Earth compared to the Sun. The figure is derived at by using the formula from Minelauva Iron Abundance is -0.06 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. The table below shows key The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. Just better. The star has a B-V Colour Index of 1.57 which means the star's temperature is about 3,850 Kelvin. Based on the star's spectral type of M3III , Minelauva's colour and type is red giant star. The time it will take to travel to this star is dependent on how fast you are going. The red dot in the diagram below shows where Minelauva is situated in
DSS2 image of Minelauva. in the constellation of which can be observed only with the help of very large telescopes.
The simplified sky map below shows the position of Minelauva in the sky: summarizes the key facts about Minelauva: In the case of a star, its the galactic centre. Proper Motion details the movements of these stars and are measured in milliarcseconds. Delta Virginis is a red giant belonging to the spectral class M3 III, approximately 198 light years distant. The red arrow shows the motion of Minelauva during the next It is this cool temperature that gives it the orange-red glow of an M-type star. Languages.
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 Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -18.87000 km/s with an error of about 0.21 km/s . Delta Vir is one of the sky's rather few naked-eye class M red giants, and a coolish one (class M3) at that. Apparent Magnitude is also known as Visual Magnitude. The Sun's radius is 695,800km, therefore the star's radius is an estimated 18,987,682.77.km.
Simplified finder chart for Minelauva - δ Virginis (delta Virginis).
A name is preferred even if its a random made up one by yourself. Delta Virginis is a red giant belonging to the spectral class M3 III. H-R diagram showing the position of Minelauva. Minelauva visual magnitude is 3.38. can be barely visible, or not visible at all, from skyes affected by light pollution. Minelauva estimated radius has been calculated as being 27.29 times bigger than the Sun. moving towards the Sun at the speed of The star is a pulsating Semi-Regular Star w variable type which means that its size changes over time. 18 kilometers per second. The temperature was calculated using information from 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 you used the 1997 Parallax value, you would get an absolute magnitude of -0.57 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.53. Live Statistics. Beta Virginis (β Virginis, abbreviated Beta Vir, β Vir), formally named Zavijava / ˌ z æ v ɪ ˈ dʒ æ v ə /, is (despite its designation 'beta') the fifth-brightest star in the constellation of Virgo.Larger and more massive than the Sun, it is comparatively metal-rich (that is, it has a higher preponderance of elements heavier than helium). Appropriately ranking fourth in brightness (though named "Delta" more for position), the star shines toward the faint end of third magnitude (3.38) from a … Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever. is a variable and double giant star It should not be taken as though the star is moving closer or further away from us. Using the 2007 distance, the star is roughly 12,547,000.74 Astronomical Units from the Earth/Sun give or take a few. It has a mass 1.4 times solar, but with a radius 48 times that of the Sun, it is about 468 times more luminous. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. A faint star will have a high number. the Minelauva is distant The source of the information if it has a Hip I.D.
information about the Minelauva double sysyem:If you find this website useful please consider a small donation that will help covering hosting costs. The star's Galacto-Centric Distance is 7,386.00 Parsecs or 24,090.42 Light Years. Added in 24 Hours. Thank you! However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 26.79089054689210477331589666. the Minelauva is a visual double star Minelauva brightness ranges from a magnitude of 3.483 to a magnitude of 3.414 over its variable period. Celestial coordinates for the J2000 equinox as well as galactic coordinates of Minelauva are provided in the following table:
Minelauva, also designated as δ Virginis (delta Virginis), Minelauva (Delta Virginis) is a red giant star that can be located in the constellation of Virgo. It is approximately 198 light-years distant.