Auva Star Facts (Delta Virginis)
Updated : 04/02/2025

Auva, also known as Delta Virginis (Bayer) is a red giant branch star located in the constellation of Virgo, The Virgin.
Based on the spectral type (M3III), Auva colour is red, which means that the star is one of the colder stars in the Universe, colder than our star.
Auva temperature is in the range of between 2,400 to 3,700 Kelvin. Based on the spectral type (M3III) as we don't have the exact temperature', we can deduce that the surface temperature of Auva is in the order of below 3,500K based on the notes from Harvard University. To put this in context, the temperature of our Sun is about 5,778 Kelvin as said by Google.
Based on a parallax of 16.44, Auva distance from Earth can be calculated at being 198.40 light years away or 62.07 parsecs.
Auva is a naked-eye star, so you don't need a telescope or binoculars when you look up on a clear night. The lower the magnitude, the easier it will be to see it.
Location
Auva location in sky is determined by the right ascension (R.A.) and declination (Dec.). These are equivalent to the Longitude and Latitude on Earth.
The Right Ascension (Longitude) is expressed in time (hh:mm:ss) and is how far the star is along Earth's celestial equator. If the R.A. is positive, then it's eastwards and vice versa.
The Declination (Latitude) is how far north or south the object is compared to the celestial equator and is expressed in degrees. If the value is positive, it is north of the celestial equator. For
Auva, the location is 12h 55m 36.48 and +03°23`51.4 .
Based on the location of Virgo, Auva can be located in the equatorial region of the celestial sky. The celestial hemisphere is equivalent to the hemispheres on Earth.
Being in the equatorial region, Auva can be seen in both terrestrial hemispheres but there is a caveat of depending how far south and north you are.
Auva is on the Ecliptic. The Ecliptic is the path that the Earth takes as it orbits the Sun. As the Earth is titled, we therefore have Celestial and Ecliptic hemispheres and they can be different for a star.
Physical Properties
Spectral Type
Auva spectral type of M3III which means its colour and type is red Red Giant Branch Star. There is no relationship between colour and size. For example, a red star can be large or small. Small stars are more energy efficient than larger stars and live longer.
Magnitude (Apparent / Absolute / Visible)
A number represents a star’s magnitude, whether apparent/visual or absolute. The smaller the number, the brighter the star is. The Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.
Auva apparent magnitude is 3.39, which is a measure of the star's brightness as seen from Earth. Apparent Magnitude is also known as Visual Magnitude.
If you use the 1997 parallax value, Auva' absolute magnitude is -0.57.
If you use the 2007 parallax value, Auva' absolute magnitude is -0.53.
Absolute Magnitude is the star's apparent magnitude from 10 parsecs or 32.6 light years. The magnitude assumes nothing is between the object and the viewer, such as dust clouds. To compare different stars' actual brightness, you would best use Absolute rather than Apparent Magnitude.
Auva is visible from Earth without needing binoculars or a telescope. The lower the Apparent Magnitude of a star or other object is, the easier it is to see in the night sky. An object with a magnitude greater than 6.5 cannot be seen without a telescope or other device.
Auva Distance from Earth
Auva distance from Earth is 202.46 light-years away from Earth or 62.07 parsecs. If you want that in miles, it is about 1,190,186,493,054,753.681, based on 1 Ly = 5,878,625,373,183.61 miles. The distance is calculated using the parallax from the original Hipparcos data released in 1997 which is 16.11000.
In 2007, Hipparcos data was revised with a new parallax of 16.44000, which puts the Auva distance from Earth as 198.40 light years or 60.83 parsecs. It should not be taken as though the star is moving closer or further away from Earth. It is purely that the distance was recalculated.
An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun. When you use the 2007 distance, Auva is roughly 12,547,000.735 Astronomical Units from the Earth/Sun give or take a few.
How long it will take to get to Auva
The time it takes to travel to Auva depends on how fast you are going. U.G. has done some calculations as to how long it will take to go at differing speeds. A note about the calculations, when I'm talking about years, I'm talking about non-leap years only (365 days).
The New Horizons space probe is the fastest one that we've sent into space at the time of writing. Its primary mission was to visit Pluto, which at the time of launch (2006), Pluto was still a planet.
Mach 1 is the speed of sound; Mach 2 is twice the speed. |Before retiring, Concorde was the fastest commercial aeroplane and the only passenger jet that could do Mach 2.
For some small screens, you may need to swipe the table to see the information. If you need an explanation, hover over the bold text. At methods are assuming you have unlimited fuel and travel at a constant speed.
- Walking - 33,262,584,798.4
- Car - 1,900,719,131.337
- Airbus A380 - 180,774,917.383
- Mach 1 - 173,407,682.565
- Mach 2 - 98,264,652.285
- New Horizons - 3,655,229.099
- Speed of Light - 198.4
Radial Velocity and Proper Motion
In simplistic terms, all non-rogue stars, like planets, orbit around a central object, although that is actually not true. Where is the centre of the Solar System. For simplicity it's the central star, such as the Sun. In the case of a star, it's the galactic centre. The constellations we see today will be different than they were 50,000 years ago or 50,000 years from now.
Proper motion details the movements of these stars and is measured in milliarcseconds. Auva 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.
The radial velocity, the speed at which the Auva is towards the Sun, is -18.87000 km/s . When the value is negative, the star and the Sun are getting closer to one another; likewise, a positive number means that two stars are moving away. It's nothing to fear as the stars are so far apart they won't collide in our lifetime, if ever.
Source of Information
The source of the information if it has a Hip I.D. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. Hipparcos was an E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated, so they could be wrong. Information regarding Metallicity and/or Mass is from the E.U. Exoplanets. The data was obtained as of 12th Feb 2017.
Auva Fact List
The table is scrollable if you can't see everything, just swipe the table to see the hidden information.
Summary Facts
Primary Name:
AuvaSpectral Type:
M3IIIStar Type:
Red Giant Branch StarColour:
redGalaxy:
Milky WayConstellation:
VirgoCelestial Hemisphere:
Equatorial RegionMain Star
: YesVisual / Apparent Magnitude
: 3.39Visible From Earth
: YesAbsolute Magnitude
: -0.53Radial Velocity
: -18.87000 km/sRedShift
: -0.0000630000Location/Coordinates
Right Ascension
: 12h 55m 36.48Declination
: +03°23`51.4Distance from Earth
Parallax
: 16.44000Light Years
: 198.40Parsecs
: 60.83Astronomical Units (A.U.)
: 12,547,000.735Proper Motion
: (milliarcseconds/year)Declination
: -52.83 ± 0.14Right Ascension
: -469.99 ± 0.22Miscellaneous Facts
B-V Index
: 1.57Alternate Names
:Delta Virginis, Minelauva, HIP 63090
Sources and Links
- Modified Date: 4th February 2025
- SIMBAD Source: Hipparcos Catalogue & Simbad
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