90 Tauri Star Facts (Type, Distance, Magnitude, Age, Colour, Location and more)
90 Tauri is a main sequence star located in the constellation of Taurus, The Bull. It is not part of the Taurus constellation outline but is within the borders of the constellation.
Based on the spectral type (A6V), 90 Tauri colour is blue - white, although not the hottest stars, they are considerably hotter than our own star which is white.
90 Tauri temperature is in the range of between 7,500 and 10,000 Kelvin. 90 Tauri effective temperature is 7,941 Kelvin which is hotter than the Sun's effective temperature, which is 5,777 Kelvin. Based on a parallax of 21.24, 90 Tauri distance from Earth can be calculated at being 153.56 light years away or 45.89 parsecs.
90 Tauri 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
The location of the 90 Tauri 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 90 Tauri, the location is 04h 38m 09.40 and +12° 30` 39.1 .
Based on the location of Taurus, 90 Tauri 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, 90 Tauri can be seen in both terrestrial hemispheres but there is a caveat of depending how far south and north you are. 90 Tauri 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
90 Tauri spectral type of A6V which means its colour and type is blue - white main sequence 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.
90 Tauri 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. 90 Tauri Luminosity figure of 31.673 comes from the Vizier online catalogue. The star generates more energy than our star.
90 Tauri Size (Radius)
90 Tauri radius has been calculated as being 2.97 times bigger than the Sun. The Sun's radius is 695,800km, therefore, the 90 Tauri radius is an estimated 2,066,526.km. If you need the star's diameter, you just need to multiply the radius by 2.
Iron Abundance
90 Tauri Iron Abundance is 0 with an error value of 9.99 Fe/H, with the Sun having a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.
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.
90 Tauri apparent magnitude is 4.27, 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, 90 Tauri' absolute magnitude is 0.96. If you use the 2007 parallax value, 90 Tauri' absolute magnitude is 0.91. 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.
90 Tauri 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.
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. 90 Tauri is moving -15.78 ± 0.38 milliarcseconds/year towards the north and 102.4 ± 0.56 milliarcseconds/year east if we saw them in the horizon.
The radial velocity, the speed at which the 90 Tauri is moving away from the Sun, is 40.30000 km/s with an error of about 1.00 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.
90 Tauri Fact Table
The table is scrollable if you can't see everything, just swipe the table to see the hidden information.
| Primary Name | 90 Tauri |
|---|---|
| Spectral Type | A6V |
| Star Type | High proper-motion Star |
| Colour | blue - white |
| Galaxy | Milky Way |
| Constellation | Taurus |
| Main Star | No |
| Absolute Magnitude | 0.96 / 0.91 |
| Visual / Apparent Magnitude | 4.27 |
| Visible From Earth | Yes |
| Right Ascension (R.A.) | 04h 38m 09.40 |
| Declination (Dec.) | +12° 30` 39.1 |
| Galactic Latitude | -22.24087752 ° |
| Galactic Longitude | 184.73661928 ° |
| 1997 Distance from Earth | 21.79000 Parallax (milliarcseconds) |
| 149.68 Light Years | |
| 45.89 Parsecs | |
| 2007 Distance from Earth | 21.24000 Parallax (milliarcseconds) |
| 153.56 Light Years | |
| 47.08 Parsecs | |
| 9,710,879.412 Astronomical Units | |
| Galacto-Centric Distance | 24,276.338 Light Years / 7,443 Parsecs |
| Proper Motion Dec. | -15.78000 ± 0.38000 milliarcseconds/year |
| Proper Motion RA. | 102.40000 ± 0.56000 milliarcseconds/year |
| B-V Index | 0.12 |
| Radial Velocity | 40.30000 ± 1 km/s |
| Iron Abundance (Fe/H) | 0.0000 ± 9.99 |
| Eccentricity | 0.13730 |
| Semi-Major Axis | 7188.0000000 |
| Luminosity (Lsun) | 31.6730000 |
| Effective Temp. (Kelvin) | 7,941 |
| Radius | 2.97 |
Sources and Links
| Modified Date | 13th July 2024 |
| Published Date | Jan 2015 |
| SIMBAD Source | Link |
| EPIC Source | Epic Search |
| Source | Vizier, |
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