VY Canis Majoris

From Wikipedia, the free encyclopedia

VY Canis Majoris
Observation data
Epoch J2000
Constellation
(pronunciation)
Canis Major
Right ascension 07h 22m 58.29s
Declination −25° 46′ 03.5″
Apparent magnitude (V) 9.527

VY Canis Majoris (VY CMa) is a red hypergiant star located in the constellation Canis Major. It is the largest known star and also one of the most luminous known. It is located about 1.5 kiloparsecs (or 5,000 light-years) from Earth.

[edit] Size

University of Minnesota professor Roberta M. Humphreys[1] estimates the radius of VY CMa at 1800 to 2100 solar radii.[2] To illustrate, if our Sun was replaced with VY Canis Majoris, its surface would extend to the orbit of Saturn. Assuming the upper size limit of 2100 solar radii, light would take more than 8 hours to travel around the star's circumference. Dr. Humphreys recently estimated[3] that the largest possible star is approximately 2,600 times the radius of the Sun.

Size comparison between the Sun and VY Canis Majoris
Size comparison between the Sun and VY Canis Majoris

Similarly, if a human could walk on the surface of Canis Majoris – assuming a speed of 5 km/h (3 mph) for 8 hours a day – the person would have to walk for 650,000 years to circle the star (compared with 2 years 11 months to complete the same task on the Earth, and 310 years 7 months on the Sun).

[edit] Controversy

There are two controversial opinions of the properties of VY CMa. One view (such as Roberta M. Humphreys' study[2]), the star is a very large and very luminous red hypergiant. In another opinion (such as Massey, Levesque, & Plez's study[4]), the star is a normal red supergiant, with a radius around 600 solar radii. In this case, its surface would extend well past the orbit of Mars.

[edit] References

  1. ^ Roberta Humphreys, Professor (Astronomy), University of Minnesota School of Physics and Astronomy
  2. ^ a b VY Canis Majoris: The Astrophysical Basis of Its Luminosity arXiv, 2006-10-13 Retrieved on 05-15-07
  3. ^ Roberta Humphreys, Professor (Astronomy), University of Minnesota School of Physics and Astronomy
  4. ^ Bringing VY Canis Majoris Down to Size: An Improved Determination of Its Effective Temperature arXiv, 2006-04-11 Retrieved on 05-15-07

[edit] See also

[edit] External links