Kaus Borealis / Lambda Sagittarii Star Facts (Type, Distance, Magnitude, Age, Colour, Location and more)
Kaus Borealis, also known as Lambda Sagittarii (Bayer) is a giant star located in the constellation of Sagittarius, Half-Man/Half-Horse Archer. Kaus Borealis is a major star and forms part of the constellation.
Based on the spectral type (K1IIIb), Kaus Borealis colour is orange to red, these are stars that are cooler than our own star.


Kaus Borealis temperature is in the range of between 3,700 and 5,200 Kelvin. Kaus Borealis effective temperature is 4,732 Kelvin which is cooler than the Sun's effective temperature which is 5,777 Kelvin. Based on a parallax of 41.72, Kaus Borealis distance from Earth can be calculated at being 78.18 light years away or 23.70 parsecs.
Kaus Borealis 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 Kaus Borealis 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 Kaus Borealis, the location is 18h 27m 58.27 and -25° 25` 16.5 .
Based on the location of Sagittarius, Kaus Borealis can be located in the southern hemisphere of the celestial sky. The celestial hemisphere is equivalent to the hemispheres on Earth. Kaus Borealis 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
Kaus Borealis spectral type of K1IIIb which means its colour and type is orange to red giant 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.
Kaus Borealis 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. Kaus Borealis Luminosity figure of 53.03 comes from the Vizier online catalogue. The star generates more energy than our star.
Iron Abundance
Kaus Borealis Iron Abundance is -0.07 with an error value of 0.03 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.
Kaus Borealis apparent magnitude is 2.82, 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, Kaus Borealis' absolute magnitude is 0.95. If you use the 2007 parallax value, Kaus Borealis' absolute magnitude is 0.92. 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.
Kaus Borealis 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. Kaus Borealis is moving -185.66 ± 0.09 milliarcseconds/year towards the north and -44.76 ± 0.16 milliarcseconds/year east if we saw them in the horizon.
The radial velocity, the speed at which the Kaus Borealis is towards the Sun, is -43.20000 km/s with an error of about 0.80 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.
Kaus Borealis Fact Table
The table is scrollable if you can't see everything, just swipe the table to see the hidden information.
| Primary Name | Kaus Borealis |
|---|---|
| Spectral Type | K1IIIb |
| Star Type | High proper-motion Star |
| Colour | orange to red |
| Galaxy | Milky Way |
| Constellation | Sagittarius |
| Main Star | Yes |
| Absolute Magnitude | 0.95 / 0.92 |
| Visual / Apparent Magnitude | 2.82 |
| Visible From Earth | Yes |
| Right Ascension (R.A.) | 18h 27m 58.27 |
| Declination (Dec.) | -25° 25` 16.5 |
| Galactic Latitude | -6.52165704 ° |
| Galactic Longitude | 7.66074200 ° |
| 1997 Distance from Earth | 42.20000 Parallax (milliarcseconds) |
| 77.29 Light Years | |
| 23.70 Parsecs | |
| 2007 Distance from Earth | 41.72000 Parallax (milliarcseconds) |
| 78.18 Light Years | |
| 23.97 Parsecs | |
| 4,944,132.955 Astronomical Units | |
| Galacto-Centric Distance | 24,057.808 Light Years / 7,376 Parsecs |
| Proper Motion Dec. | -185.66000 ± 0.09000 milliarcseconds/year |
| Proper Motion RA. | -44.76000 ± 0.16000 milliarcseconds/year |
| B-V Index | 1.02 |
| Radial Velocity | -43.20000 ± 0.8 km/s |
| Iron Abundance (Fe/H) | -0.0700 ± 0.03 |
| Eccentricity | 0.16500 |
| Semi-Major Axis | 6617.0000000 |
| Luminosity (Lsun) | 53.0300000 |
| Effective Temp. (Kelvin) | 4,732 |
Sources and Links
| Modified Date | 13th July 2024 |
| Published Date | Jan 2015 |
| SIMBAD Source | Link |
| EPIC Source | Epic Search |
| Source | Vizier, |
Sagittarius's Main Stars in Brightness Order
- Kaus Media (Delta Sagittarii)
- Kaus Australis (Epsilon Sagittarii)
- Ascella (Zeta Sagittarii)
- Iota Sagittarii
- Kaus Borealis (Lambda Sagittarii)
- Xi1 Sagittarii
- Omicron Sagittarii
- Albaldah (Pi Sagittarii)
- Rho1 Sagittarri (Rho Sagittarii)
- Nunki (Sigma Sagittarii)
- Tau Sagittarii
- Upsilon Sagittarii
- Phi Sagittarii
- Chi1 Sagittarii
- Psi Sagittarii
- 62 Sagittarii
- 59 Sagittarii
- 52 Sagittarii
- 43 Sagittarii
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Comments and Questions
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shane jamieson
kaus borealis is the centre of the golden pyrimid of TICA IN SOUTH AMERICA.