Regor / Gamma Velorum Star Facts (Type, Distance, Magnitude, Age, Mass, Colour, Location and more)
Facts
It is the nearest and brightest Wolf-Rayet star to our own Sun. It is one of only two wolf-rayet stars that can be seen with the naked eye. The other naked-eye Wolf Rayet is Theta Muscae. The star is a binary star with another star revolving, but as only one of those stars is catalogued in Hipparcos, only one is detailed here. It is more appropriate to call this star Gamma2 Velorum.
Regor's Name
Regor is an unofficial name that American pioneer astronaut Gus Grissom created. The star was to be used to help them navigate. Gus Grissom nicknamed the star Regor after fellow astronaut Roger Chaffee, and after their deaths along with Edward White II on Jan 27th 1967, the name stuck. The star Gamma Cassiopeiae is sometimes referred to as Navi, which is Gus' middle name. The star Iota Ursae Majoris has an unofficial name of Dnoces after White. In addition to being known as Regor, it has a more traditional name of, Suhail al Muhlif. Neither Regor nor Suhail al Muhlif are recognised by the International Astronomer Union (I.A.U.). Ref: One Min Astronomer.
Regor, also known as Gamma Velorum (Bayer) is a very luminous supergiant starwolf-rayet star located in the constellation of Vela, The Sails. Regor is a major star and forms part of the constellation.


Regor is the 1st brightest star in Vela based on the Hipparcos 2007 apparent magnitude. Based on a parallax of 2.92, Regor distance from Earth can be calculated at being 1,117.00 light years away or 257.73 parsecs.
Regor 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.
Regor is an eruptive wolf-rayet variable star. Variable stars are stars whose size and/or brightness changes over time. Regor brightness ranges from 1.724 (dimmest) to 1.68 over a period of 0.034 days.
Location
The location of the Regor in the night 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 Regor, the location is 08h 09m 31.96 and -47° 20` 11.8 .
Based on the location of Vela, Regor can be located in the southern hemisphere of the celestial sky. The celestial hemisphere is equivalent to the hemispheres on Earth. Regor is south of 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.
Wolf-Rayet Star
Regor is a Wolf-Rayet, a rare type of star of which not many are known. These stars are extremely luminous and large compared to our Sun. They live fast and die hard in a matter of millions not billions of years like our Sun. They exhaust their hydrogen supplies, turning to other gasses and expand outwards with massive solar winds, moving a step closer in the stellar evolution towards their death in a super or hypernova explosion.
Physical Properties
Spectral Type
Regor spectral type of WC8 + O9I 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.
Regor Luminosity
Luminosity is the amount of energy a star pumps out relative to the amount that our star, the Sun, gives out. Our star, the Sun's value is 1. Regor luminosity figure of 64,399.63 is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. The star generates more energy than our star.
Regor Size (Radius)
Regor radius has been calculated as being 17 times bigger than the Sun. The Sun's radius is 695,800km, therefore, the Regor radius is an estimated 11,828,600.km. If you need the star's diameter, you just need to multiply the radius by 2. The error range for the radius is between 2.00000 and 2.00000.
Regor Mass
Regor mass is 28.5 times that of our star, the Sun. There is an uncertainty of between -1.100 and +1.1000. The Sun's Mass is 1,989,100,000,000,000,000,000 billion kg. which to calculate using this website is too large. To give an idea of size, the Sun is 99.86% of the solar system's mass.
Regor Death
We can't be sure when Regor will die, we can have estimations based on its spectral type and mass. Based on current estimations with Regor being more than 10 solar masses, it will at the end of its life, most likely die in a Supernova explosion. The explosion will leave behind either a Pulsar or a Black Hole.
Regor Age
Regor age according to Hipparcos data files put the star at an age of about 0.035 billion years old but could be between 0.035 and 0.055 billion years old. In comparison, the Sun's age is about 4.6 billion years old. The smaller star is, the more efficient it is with its fuel and so will live longer than a star which is very large. Regor is estimated at being 0.035000 billions of years old but could be between 0.0350 and 0.0550
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.
Regor apparent magnitude is 1.75, 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, Regor' absolute magnitude is -5.31. If you use the 2007 parallax value, Regor' absolute magnitude is -5.92. 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.
Regor 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.
Meteor Showers
There are 1 meteor showers that radiate from a location near Regor during the year.
- Gamma Velids Meteor Shower 1-17 Jan (Peak: 5th Jan).
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. Regor is moving 10.43 ± 0.25 milliarcseconds/year towards the north and -6.07 ± 0.3 milliarcseconds/year east if we saw them in the horizon.
The radial velocity, the speed at which the Regor is moving away from the Sun, is 15.00000 km/s with an error of about 3.10 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.
Regor Fact Table
The table is scrollable if you can't see everything, just swipe the table to see the hidden information.
| Primary Name | Regor | |
|---|---|---|
| Spectral Type | WC8 + O9I | |
| Star Type | Wolf-Rayet Star | |
| Galaxy | Milky Way | |
| Constellation | Vela | |
| Main Star | Yes | |
| Age | 35 million years | |
| Age Range | 0.035 - 0.055 billion years | |
| Absolute Magnitude | -5.31 / -5.92 | |
| Visual / Apparent Magnitude | 1.75 | |
| Visible From Earth | Yes | |
| Right Ascension (R.A.) | 08h 09m 31.96 | |
| Declination (Dec.) | -47° 20` 11.8 | |
| Galactic Latitude | -7.68581898 ° | |
| Galactic Longitude | 262.80257939 ° | |
| 1997 Distance from Earth | 3.88000 Parallax (milliarcseconds) | |
| 840.63 Light Years | ||
| 257.73 Parsecs | ||
| 2007 Distance from Earth | 2.92000 Parallax (milliarcseconds) | |
| 1117.00 Light Years | ||
| 342.47 Parsecs | ||
| 70,639,015.976 Astronomical Units | ||
| Galacto-Centric Distance | 24,322.001 Light Years / 7,457 Parsecs | |
| Proper Motion Dec. | 10.43000 ± 0.25000 milliarcseconds/year | |
| Proper Motion RA. | -6.07000 ± 0.30000 milliarcseconds/year | |
| B-V Index | -0.14 | |
| Radial Velocity | 15.00000 ± 3.1 km/s | |
| Eccentricity | 0.03510 | |
| Semi-Major Axis | 7721.0000000 | |
| Luminosity (Lsun) | 64399.6300000 | |
| Mass (Solars) | 28.5000 (-1.100 / +1.1000) | |
| Radius | 17 (-2 / +2) |
Variable Star Details
| Variable Star Class | Eclipsing binary system |
| Variable Star Type | Eruptive Wolf-Rayet |
| Mean Variability Period in Days | 0.034 |
| Variable Magnitude Range | 1.68 - 1.724 |
Estimated Calculated Facts
| Radius (x the Sun) | 17 (2 - 2) |
| Surface Temperature |
Sources and Links
| Modified Date | 13th July 2024 |
| Published Date | Jan 2015 |
| SIMBAD Source | Link |
Vela's Main Stars in Brightness Order
Advertisements


Comments and Questions
Adding comments or questions is currently suspended at the moment. Should you need to contact me because there's a mistake or something missing, you can do so from the About Us page.