

Primarily for those who are appearing in administrative examinations, in order to help them especially in their General Science part of General Studies.
The star had been discovered previously in the Peony nebula near the galaxy's dusty centre is Milky Way's brightest star. But infrared observations taken from the ground and with NASA's Spitzer Space Telescope have pierced the dust to reveal just how bright the star is.
It boasts a wattage of about 3.2 million Suns. That is close to the output of Eta Carinae, the current record holder, which shines with the light of about 4.7 million Suns. However, measuring stellar brightness is not an exact science, and the stars may actually radiate similar amounts of light.
It's possible that the galaxy's brightest star has not even been discovered yet. Both Eta Carinae and the Peony nebula star are evolved blue giants known as "Wolf-Rayet" stars, which have masses of 100 to 200 Suns.The Peony nebula star lies about 26,000 light years away and Eta Carinae about 7500 light years away.
Journal reference: Astronomy & Astrophysics (forthcoming)
http://space.newscientist.com/article/dn14328-whos-the-brightest-star-of-all.html
The largest star measured in solar diameters is either VV Cephei or VY Canis Majoris (right image)
"What's the Biggest Star in the Universe"? Generally students ask this question.
I may give an easy answer, the Universe is a big place, and there's no way we can possibly know what the biggest star is. That didn't go over so well.
However the question may be refined:- What's the biggest star that we know of ?
Pistol Star: The largest known star, in terms of mass and brightness is called the Pistol Star. It is believed to be 100 times as massive as our Sun, and 10,000,000 times as bright! In 1990, a star named the Pistol Star was known to lie at the center of the Pistol Nebula in the Milky Way Galaxy. Observations from the Hubble Space Telescope in 1997 confirmed the relationship between the star and the nebula.
Eta Carinae: One huge, famous star in our galaxy is the monster Eta Carinae, located approximately 7,500 light years away, and weighing in at 100 solar masses. It's 4 million times as bright as the Sun. Most stars blow with a solar wind, losing mass over time. But Eta Carinae is so large that it casts off 500 times the mass of the Earth every year. With so much mass lost, it's very difficult for astronomers to accurately measure where the star ends, and its stellar wind begins.
So the best answer astronomers have right now is that Eta Carinae's radius is 400 times the size of the Sun. Eta Carinae should explode pretty soon as one of the most spectacular supernovae humans have ever seen.
VY Canis Majoris: The largest known star is VY Canis Majoris; a red hypergiant star in the constellation Canis Major, located about 5,000 light-years from Earth. University of Minnesota professor Roberta Humphreys recently calculated its upper size at more than 2,100 times the size of the Sun. Placed in our Solar System, its surface would extend out past the orbit of Saturn. Light takes more than 8 hours to cross its circumference!
Some astronomers disagree, and think that VY Canis Majoris might be smaller; merely 600 times the size of the Sun, extending past the orbit of Mars.
That's the biggest star that we know of, but the Milky way probably has dozens of stars that are even larger, obscured by gas and dust so we can't see them.
But let's see if we can work out the original question, what's the biggest star in the Universe?
Obviously, it's impossible for us to actually find it - the Universe is a big place, and there's no way we can peer into every corner. The largest stars are the coolest. So even though Eta Carinae is the most luminous star we know of, it's extremely hot - 25,000 Kelvin - and so only a mere 400 solar radii.
![]() |
Phoenix's telescoping arm scoops up soil samples |
The International Astronomical Union has decided on the term "plutoid" as a name for dwarf planets like Pluto.
The name plutoid was proposed by the members of the IAU Committee on Small Body Nomenclature (CSBN), accepted by the Board of Division III and by the IAU Working Group for Planetary System Nomenclature (WGPSN), and approved by the IAU Executive Committee at its recent meeting in Oslo, according to a statement released on 11th June, 2008.
Here's the official new definition:
"Plutoids are celestial bodies in orbit around the sun at a distance greater than that of Neptune that have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (near-spherical) shape, and that have not cleared the neighborhood around their orbit."
In short:
small round things beyond Neptune that orbit the sun and have lots of rocky neighbors.
The two known and named plutoids are Pluto and Eris. The organization expects more plutoids will be found.
The dwarf planet Ceres is not a plutoid as it is located in the asteroid belt between Mars and Jupiter, according to the IAU. Current scientific knowledge lends credence to the belief that Ceres is the only object of its kind, the IAU stated. Therefore, a separate category of Ceres-like dwarf planets will not be proposed at this time, the reasoning goes.
The term plutoid joins a host of other odd words -- plutinos, centaurs, cubewanos and EKOs -- that astronomers use to define objects in the outer solar system.