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30 Vulpeculae

30 Vulpeculae Facts

  • 30 Vulpeculae is a giant star that can be located in the constellation of Vulpecula. The description is based on the spectral class.
  • 30 Vulpeculae is not part of the constellation outline but is within the borders of the constellation.
  • Based on the spectral type (K2III) of the star, the star's colour is orange to red .
  • The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
  • Using the most recent figures given by the 2007 Hipparcos data, the star is 324.86 light years away from us. Distance

30 Vulpeculae's Alternative Names

The Id of the star in the Yale Bright Star Catalogue is HR7939. HIP102388 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD197752.

Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John named the stars in the constellation with a number and its latin name, this star's Flamsteed designation is 30 Vulpeculae. The Flamsteed name can be shortened to 30 Vul.

BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD+24 4229.

More details on objects' alternative names can be found at Star Names .

Location of 30 Vulpeculae

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. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. If the R.A. is positive then its eastwards. The Declination is how far north or south the object is compared to the celestial equator and is expressed in degrees. For 30 Vulpeculae, the location is 20h 44m 52.52 and +25° 16` 15.8 .

Radial Velocity and Proper Motion of 30 Vulpeculae

Proper Motion

All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. In the case of a star, its the galactic centre. The constellations that 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 are measured in milliarcseconds. The star is moving -177.96 ± 0.27 milliarcseconds/year towards the north and -29.06 ± 0.47 milliarcseconds/year east if we saw them in the horizon.

Radial Velocity

The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is 30.00000 km/s with an error of about 0.30 km/s . 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. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.

Physical Properties of 30 Vulpeculae

30 Vulpeculae Temperature and Colour

Based on the star's spectral type of K2III , 30 Vulpeculae's colour and type is orange to red giant star. The star has a B-V Colour Index of 1.18 which means the star's temperature is about 4,524 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu.

30 Vulpeculae 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. The figure of 156.12 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

30 Vulpeculae Radius

30 Vulpeculae estimated radius has been calculated as being 17.61 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 12,255,916.10.km. If you need the diameter of the star, you just need to multiple the radius by 2. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 15.698526864755626984247331582. The figure is derived at by using the formula from SDSS rather than peer reviewed papers. It has been known to produce widely incorrect figures.

30 Vulpeculae Iron Abundance

30 Vulpeculae Iron Abundance is -0.10 with an error value of 0.06 Fe/H with the Sun has a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.

30 Vulpeculae Apparent and Absolute Magnitudes

30 Vulpeculae has an apparent magnitude of 4.92 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. If you used the 1997 Parallax value, you would get an absolute magnitude of -0.32 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.07. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.

Distance to 30 Vulpeculae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 8.94000 which gave the calculated distance to 30 Vulpeculae as 364.84 light years away from Earth or 111.86 parsecs. If you want that in miles, it is about 2,144,757,681,152,308.27, based on 1 Ly = 5,878,625,373,183.61 miles.

In 2007, Hipparcos data was revised with a new parallax of 10.04000 which put 30 Vulpeculae at a distance of 324.86 light years or 99.60 parsecs. It should not be taken as though the star is moving closer or further away from us. It is purely that the distance was recalculated.

Using the 2007 distance, the star is roughly 20,543,831.55 Astronomical Units from the Earth/Sun give or take a few. 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. The star's Galacto-Centric Distance is 7,365.00 Parsecs or 24,021.93 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Travel Time to 30 Vulpeculae

The time it will take to travel to this star is dependent on how fast you are going. U.G. has done some calculations as to how long it will take going at differing speeds. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

The New Horizons space probe is the fastest probe 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.

DescriptionSpeed (m.p.h.)Time (years)
Walking454,464,129,524.24
Car1201,815,470,984.14
Airbus A380736296,000,703.94
Speed of Sound (Mach 1)767.269283,937,599.59
Concorde (Mach 2)1,534.54141,968,614.76
New Horizons Probe33,0006,601,712.67
Speed of Light670,616,629.00324.86

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 a E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated so they could well be wrong. Information regarding Metallicity and/or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.

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Additional 30 Vulpeculae Facts and Figures

Visual Facts


Primary / Proper / Traditional Name30 Vulpeculae
Alternative NamesHD 197752, HIP 102388, HR 7939, 30 Vul, BD+24 4229
Spectral TypeK2III
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeGiant Star
ColourOrange to Red
GalaxyMilky Way
ConstellationVulpecula
Absolute Magnitude -0.32 / -0.07
Visual / Apparent Magnitude4.92
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)20h 44m 52.52
Declination (Dec.)+25° 16` 15.8
Galactic Latitude-10.81434894 degrees
Galactic Longitude68.82057104 degrees
1997 Distance from Earth8.94000 Parallax (milliarcseconds)
 364.84 Light Years
 111.86 Parsecs
2007 Distance from Earth10.04000 Parallax (milliarcseconds)
 324.86 Light Years
 99.60 Parsecs
 20,543,831.55 Astronomical Units
Galacto-Centric Distance24,021.93 Light Years / 7,365.00 Parsecs
Proper Motion Dec.-177.96000 ± 0.27000 milliarcseconds/year
Proper Motion RA.-29.06000 ± 0.47000 milliarcseconds/year
B-V Index1.18
Radial Velocity30.00000 ± 0.30 km/s
Iron Abundance-0.1000 ± 0.06 Fe/H
Eccentricity0.46990
Semi-Major Axis9236.0000000
Stellar Luminosity (Lsun)156.1200000

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Calculated Facts


Radius (x the Sun)15.70
Effective Temperature4,524 Kelvin

Sources and Links


SIMBAD SourceLink

Related Stars


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