Arcturus (Alpha Bootis), facts about the brightest star in the northern hemisphere

Facts

Arcturus is a massive star located 36.72 light years from the the Sun in the constellation of Bootes. It is orange in colour, meaning that its temperature, based on the Hertzsprung-Russell diagram, is between 4,000 to 5,250 Kelvin. The temperature is certainly hot enough to fry an egg. It is not as hot as the Sun, which has a rough temperature of about 5,300 to 6,000 k.

Arcturus is the fourth brightest star in the sky after -1.44 magnitude Sirius, -0.62 Magnitude Canopus and -0.27 Magnitude Alpha Centauri also known as Rigil Kentaurus. Even though Sirius is brighter than Arcturus, Arcturus is further away from our solar system.

No Extrasolar Planets (Exoplanets) have been discovered orbiting around this planet, but it's not to say that they aren't or weren't any. The star has held a position in science fiction for orbiting planets with life forms. For instance, Arcturans have been mentioned in Star Trek, where the aliens come from the fourth planet orbiting the star.

Arcturus, also known as Alpha Bootis (Bayer) is a red giant branch star located in the constellation of Bootes, The Bear Driver. Arcturus is a major star and forms part of the constellation.

Based on the spectral type (K2IIIp), Arcturus colour is orange to red, these are stars that are cooler than our own star.


Arcturus temperature is in the range of between 3,700 and 5,200 Kelvin. Arcturus effective temperature is 4,286 Kelvin which is cooler than the Sun's effective temperature which is 5,777 Kelvin.

Arcturus is the brightest star in Bootes and the 4th in the night sky based on the Hipparcos 2007 apparent magnitude. Based on a parallax of 88.83, Arcturus distance from Earth can be calculated at being 36.72 light years away or 11.25 parsecs.

Arcturus 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.

Arcturus is a variable star, its brightness varies in magnitude between 0.0930 to 0.1400. The smaller number is the brightest the star gets.

Location

The location of the Arcturus 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 Arcturus, the location is 14h 15m 40.35 and +19° 11` 14.2 .

Based on the location of Bootes, Arcturus can be located in the northern hemisphere of the celestial sky. The celestial hemisphere is equivalent to the hemispheres on Earth. Arcturus is north 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.

Physical Properties

Spectral Type

Arcturus spectral type of K2IIIp which means its colour and type is orange to red Red Giant Branch 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.

Arcturus 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. Arcturus luminosity figure of 206.84 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.

Arcturus Size (Radius)

Arcturus radius has been calculated as being 25.4 times bigger than the Sun. The Sun's radius is 695,800km, therefore, the Arcturus radius is an estimated 17,673,320.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 25.20000 and 25.60000.

Arcturus Mass

Arcturus mass is 1.08 times that of our star, the Sun. There is an uncertainty of between -1.020 and +1.1400. 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.

Arcturus Death

We can't be sure when Arcturus will die, we can have estimations based on its spectral type and mass. Based on current estimations with Arcturus having less than 10 solar masses, Arcturus will most likely first start losing its mass in solar winds in a Planetary Nebula phase before the nebula disperses leaving behind a White Dwarf.

Iron Abundance

Arcturus Iron Abundance is -0.5 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.

Arcturus Age

Arcturus age according to Hipparcos data files put the star at an age of about 7.1 billion years old but could be between 5.9 and 8.6 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. Arcturus lifespan could be between 15 to 45 billion years assuming it is a typical orange star (K Type).

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.

Arcturus apparent magnitude is -0.05, 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, Arcturus' absolute magnitude is -0.31. If you use the 2007 parallax value, Arcturus' absolute magnitude is -0.31. 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.

Arcturus 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. Arcturus is moving -2,000.06 ± 0.35 milliarcseconds/year towards the north and -1,093.39 ± 0.54 milliarcseconds/year east if we saw them in the horizon.

The radial velocity, the speed at which the Arcturus is towards the Sun, is -5.24000 km/s with an error of about 0.09 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.

Arcturus Fact Table

The table is scrollable if you can't see everything, just swipe the table to see the hidden information.

Primary NameArcturus
Spectral TypeK2IIIp
Star TypeRed Giant Branch Star
Colour orange to red
GalaxyMilky Way
ConstellationBootes
Main StarYes
Age 7.1 million years
Age Range5.9 - 8.6 billion years
Absolute Magnitude -0.31 / -0.31
Visual / Apparent Magnitude-0.05
Visible From Earth Yes
Right Ascension (R.A.)14h 15m 40.35
Declination (Dec.)+19° 11` 14.2
Galactic Latitude69.11106419 °
Galactic Longitude15.06558209 °
1997 Distance from Earth88.85000 Parallax (milliarcseconds)
 36.71 Light Years
 11.25 Parsecs
2007 Distance from Earth88.83000 Parallax (milliarcseconds)
 36.72 Light Years
 11.26 Parsecs
 2,322,525.535 Astronomical Units
Galacto-Centric Distance24,123.041 Light Years / 7,396 Parsecs
Proper Motion Dec.-2000.06000 ± 0.35000 milliarcseconds/year
Proper Motion RA.-1093.39000 ± 0.54000 milliarcseconds/year
B-V Index1.23
Radial Velocity-5.24000 ± 0.09 km/s
Iron Abundance (Fe/H)-0.5000 ± 9.99
Eccentricity0.75200
Semi-Major Axis2848.0000000
Luminosity (Lsun)206.8400000
Mass (Solars) 1.0800 (-1.020 / +1.1400)
Effective Temp. (Kelvin) 4,286
Radius25.4 (-25.2 / +25.6)
Brightest in Night Sky4th

Variable Star Details


Mean Variability Period in Days0.043
Variable Magnitude Range0.093 - 0.14

Sources and Links


Modified Date13th July 2024
Published DateJan 2015
SIMBAD SourceLink


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