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Sirius

 Sirius


Table of Contents 

Sirius is the brightest star in the night sky. Its name is derived from the Greek word Σείριος. The star is designated α Canis Majoris, Latinized to Alpha Canis Majoris, and abbreviated Alpha CMa or α CMa. With a visual apparent magnitude of −1.46, Sirius is almost twice as bright as Canopus, the next brightest star. 


Information 

Distance to Earth :- 8.611 light years

Surface temperature :- 9,940 K

Magnitude :- -1.46

Radius :- 1.19 million km (1.711 R☉)

Constellation :- Canis Major

Coordinates :- RA 6h 45m 9s | Dec -16° 42′ 58″

Star system :- Solar System


Star age

The more massive of these, Sirius B, consumed its resources and became a red giant before shedding its outer layers and collapsing into its current state as a white dwarf around 120 million years ago.

 

Sirius.


Observation data Epoch J2000.0 Equinox ICRS

Rotation

16 km/s

Age

242 ± 5 Myr

Sirius B

Mass

1.018 ± 0.011 M


Composition

Sirius B is primarily made out of a carbon-oxygen mixture that was generated by helium fusion in the progenitor star. The outer atmosphere is now almost pure hydrogen, the element with the lowest mass.


Density

3.0 x 106 grams per cubic cm

Density is the total mass divided by the volume. Sirius B's density is 3.0 x 106 grams per cubic cm, or 3.0 x 109 kg per cubic meter.


Weight

Sirius B's powerful gravitational field is 350,000 times greater than Earth's, meaning that a 68 kilogram person would weigh 25 million kilograms standing on its surface.


About the Object.


Name:

Earth, Sirius B

Type:

Solar System : Planet Milky Way : Star : Evolutionary Stage : White Dwarf

Category:

Solar System

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