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Sirius
Canis Major constellation map.svg
Red circle.svg
Location of Sirius (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Canis Major
Sirius A
Right ascension 06h 45m 08.917s
Declination −16° 42′ 58.02″
Apparent magnitude (V) −1.46
Sirius B
Right ascension 06h 45m 09.0s
Declination −16° 43′ 06″
Apparent magnitude (V) 8.44
Characteristics
Sirius A
Evolutionary stage Main sequence
Spectral type A0mA1 Va
U−B colour index −0.05
B−V colour index +0.00
Sirius B
Evolutionary stage White dwarf
Spectral type DA2
U−B colour index −1.04
B−V colour index −0.03
Astrometry
Radial velocity (Rv) −5.50 km/s
Sirius A
Proper motion (μ) RA: −546.01 mas/yr
Dec.: −1,223.07 mas/yr
Parallax (π) 378.9 ± 1.4 mas
Distance 8.61 ± 0.03 ly
(2.639 ± 0.010 pc)
Absolute magnitude (MV) +1.43
Sirius B
Proper motion (μ) RA: −461.571 mas/yr
Dec.: −914.520 mas/yr
Parallax (π) 378.9 ± 1.4 mas
Distance 8.61 ± 0.03 ly
(2.639 ± 0.010 pc)
Absolute magnitude (MV) +11.18
Orbit
Primary α Canis Majoris A
Companion α Canis Majoris B
Period (P) 50.1284±0.0043 yr
Semi-major axis (a) 7.4957±0.0025"
(19.8 AU)
Eccentricity (e) 0.59142±0.00037
Inclination (i) 136.336±0.040°
Longitude of the node (Ω) 45.400±0.071°
Periastron epoch (T) 1994.5715±0.0058
Argument of periastron (ω)
(secondary)
149.161±0.075°
Details
Sirius A
Mass 2.063±0.023 M☉
Radius 1.7144±0.0090 R☉
Luminosity 24.74±0.70 L☉
Surface gravity (log g) 4.33 cgs
Temperature 9,845±64 K
Metallicity [Fe/H] 0.50 dex
Rotational velocity (v sin i) 16.3±0.1 km/s
Age 242±5 Myr
Sirius B
Mass 1.018±0.011 M☉
Radius 0.008098±0.6% R☉
Radius 5,634±34 km
Luminosity 0.02448±1.3% L☉
Surface gravity (log g) 8.591±0.016 cgs
Temperature 25,369±46 K
Age 228+10
−8
 Myr
Other designations
Dog Star, Aschere, Canicula, Al Shira, Sothis, Alhabor, Mrgavyadha, Lubdhaka, Tenrōsei, α Canis Majoris (α CMa), 9 Canis Majoris (9 CMa), HD 48915, HR 2491, BD−16°1591, GJ 244, LHS 219, ADS 5423, LTT 2638, HIP 32349
Sirius B: EGGR 49, WD 0642-166, GCTP 1577.00
Database references
SIMBAD A
B

Sirius is the brightest star in the entire night sky. It shines brightly in the southern constellation called Canis Major, which means the Greater Dog. Because of this, people often call it the Dog Star. Its official scientific name is Alpha Canis Majoris. Sirius looks almost twice as bright as Canopus, the second brightest star visible from Earth. It shines with a visual apparent magnitude of −1.46. Only the Moon and planets like Venus, Jupiter, Mars, and Mercury outshine it. When you look up at Sirius, you are actually seeing a binary star system where two stars dance around each other.

Why Does the Star Sirius Shine So Brightly?

Canis Major - Orion
The constellations Canis Major and Orion. Sirius shines brightly near the center.

Sirius looks amazingly bright to us for two main reasons. First, the main star has a very strong luminosity, creating 25 times more light than our Sun. Second, it is located very close to our Solar System. Sirius is only 8.6 light-years away from us, making it one of the nearest neighbours to Earth.

The star is slowly traveling closer toward our Solar System. Its speed towards us is about 5.5 kilometers every second. Astronomers found that it will become even brighter over the next 60,000 years. It will easily stay the most radiant star in our night sky for another 210,000 years. Eventually, the distant star Vega will take over the top spot as Sirius drifts further away.

The Amazing Double Star System

Orbit Sirius B arcsec
The orbit of Sirius B around Sirius A.

Even though Sirius looks like a single shining diamond, it actually consists of two separate stars. They circle around each other once every 50 years. The distance between them is around 20 astronomical units, similar to the distance from our Sun to Uranus.

The Brilliant Sirius A

Sirius A-Sun comparison2
Comparison of Sirius A and our Sun to scale.

The bigger star is called Sirius A. It is a hot, white main-sequence A-type star. Sirius A has about twice the mass of our Sun. Its surface reaches a scorching heat of nearly 9,940 degrees Kelvin. It spins around at a speed of 16 kilometers per second. This huge star was born inside a collapsing molecular cloud roughly 240 million years ago. Deep in its fiery core, it burns through hydrogen fuel using a nuclear reaction called the CNO cycle. Scientists calculate that Sirius A will live another billion years before it puffs out into a huge red giant.

The Tiny White Dwarf Sirius B

Sirius B-Earth comparison2
Size comparison between Sirius B and Earth.

The companion star is named Sirius B, nicknamed "the Pup". It is a tiny, super-dense white dwarf. It was once a large B-type star that ran out of fuel and shrank about 120 million years ago. Sirius B packs the mass of our entire Sun into a ball roughly the same size as planet Earth. A single teaspoon of its matter would weigh as much as an elephant on Earth. Because it no longer creates nuclear energy, it is slowly cooling off into space over billions of years.

How Was the Hidden Companion Discovered?

Sirius A and B Hubble photo
Hubble Space Telescope picture showing Sirius A and tiny Sirius B at the lower left.

In 1844, a German astronomer named Friedrich Wilhelm Bessel noticed that Sirius wobbled slightly as it moved across space. He guessed that an unseen object was pulling on it gravitationally. In 1862, an American telescope builder named Alvan Graham Clark peered through a new great refractor telescope at Dearborn Observatory and spotted Sirius B for the first time. Later, in 1915, astronomer Walter Sydney Adams studied its light at Mount Wilson Observatory and realized it was one of the first white dwarfs ever found.

Sirius in the Night Sky

Hubble heic0206j
Sirius, Betelgeuse, and Procyon create the famous Winter Triangle.

You can spot Sirius from almost everywhere on Earth, except north of 73 degrees north latitude. Along with the stars Betelgeuse and Procyon, Sirius forms a giant pattern in the winter sky known as the Winter Triangle. Because Sirius shines so brilliantly through the moving air of Earth's atmosphere, it often seems to rapidly twinkle with flashes of red, blue, and green light.

Ancient Legends and Cultural History

Sopdet
The Egyptian goddess Sopdet, who represented the star Sirius.

Sirius has fascinated human cultures for thousands of years. The name comes from the Ancient Greek word Seirios, which means "glowing" or "scorching".

Ancient Egypt and the Nile River

To people in Ancient Egypt, Sirius represented the goddess Sopdet. Its yearly morning rising in July happened right before the vital flooding of the Nile river. The waters brought rich soil that helped farmers grow delicious crops. Because of this, Egyptians based their early calendar on this star's return. They connected it with the goddess Isis and the god Osiris.

The "Dog Days" of Summer

Ancient Greek and Roman watchers believed that the rising of Sirius added heat to the sun, bringing the hottest weeks of summer. They called this stifling time the "dog days" of summer. Roman farmers even held ceremonies to protect their fields from crop damage during this warm weather.

Ocean Voyagers of the Pacific

To ancient Polynesians, Sirius was a crucial beacon for navigating boats across the vast Pacific Ocean. Because the star passed directly above Fiji, sailors used it to steer their canoes safely between distant islands. In Hawaii, the star was celebrated as the "Queen of Heaven". In New Zealand, the Māori people saw Sirius as a sign that winter was beginning.

Images for kids

See also

Kids robot.svg In Spanish: Sirio para niños

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