T Monocerotis is a orange to red pulsating star that can be located in the constellation of Monoceros. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
The Id of the star in the Yale Bright Star Catalogue is HR2310. HIP30541 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD44990.
T Monocerotis has alternative name(s), T Mon.
The location of the star in the galaxy 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 star is compared to the celestial equator and is expressed in degrees. For T Monocerotis, the location is 06h 25m 13.00 and +07d 05` 08.6 .
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 -2.01 ± 0.49 miliarcseconds/year towards the north and 1.40 ± 0.80 miliarcseconds/year east if we saw them in the horizon. The Radial Velocity, that is the speed at which the star is moving away/towards us is 30.70000 km/s with an error of about 0.40 km/s .
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 13500.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.
T Monocerotis has a spectral type of K1Iabv SB. This means the star is a orange to red star. The star has a B-V Colour Index of 0.85 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,308 Kelvin.
T Monocerotis Radius has been calculated as being 146.93 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 102,230,662.77.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 51.18. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is -0.03 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.
T Monocerotis has an apparent magnitude of 6.26 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 -5.62 If you used the 2007 Parallax value, you would get an absolute magnitude of -3.33. 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.
Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 0.42 which gave the calculated distance to T Monocerotis as 7765.79 light years away from Earth or 2380.95 parsecs. It would take a spaceship travelling at the speed of light, 7765.79 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
In 2007, Hipparcos data was revised with a new parallax of 1.21 which put T Monocerotis at a distance of 2695.56 light years or 826.45 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.
The star is a pulsating Delta Cepheid variable type which means that its size changes over time. The Variable Type is usually named after the first star of that type to be spotted. T Monocerotis brightness ranges from a magnitude of 6.737 to a magnitude of 5.803 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 27.0 days (variability).
|Traditional/Proper Name||T Monocerotis|
|Short Name||T Mon|
|Hipparcos Library I.D.||30541|
|Yale Bright Star Catalogue (HR) Id||2310|
|Bonner Durchmusterung||BD+07 1273|
|Henry Draper Designation||44990|
|Absolute Magnitude||-5.62 / -3.33|
|Visual / Apparent Magnitude||6.26|
|Naked Eye Visible||Yes - Magnitudes|
|Right Ascension (R.A.)||06h 25m 13.00|
|Declination (Dec.)||+07d 05` 08.6|
|Galactic Latitude||-2.56 degrees|
|Galactic Longitude||203.63 degrees|
|1997 Distance from Earth||0.42 Parallax (milliarcseconds)|
|7765.79 Light Years|
|2007 Revised Distance from Earth||1.21 Parallax (milliarcseconds)|
|2695.56 Light Years|
|Proper Motion Dec.||-2.01 ± 0.49 milliarcseconds/year|
|Proper Motion RA.||1.40 ± 0.80 milliarcseconds/year|
|Radial Velocity||30.70 ± 0.40 km/s|
|Iron Abundance||-0.03 ± 9.99 Fe/H|
|Spectral Type||K1Iabv SB|
|Colour||(K) Orange to Red|
|Variable Star Class||Pulsating|
|Variable Star Type||Delta Cepheid|
|Mean Variability Period in Days||27.029|
|Variable Magnitude Range (Brighter - Dimmer)||5.803 - 6.737|
|Luminosity (x the Sun)||13,500.0000000|
|Calculated Effective Temperature||5,308 Kelvin|