Looking its best ever is the star cluster NGC 2203, here imaged by the NASA/ESA Hubble Space Telescope. Aside from its dazzling good looks, this cluster of stars contains lots of astronomical treats that have helped astronomers puzzle together the lifetimes of stars.
A main sequence star, like our Sun, is the term applied to a star during the longest period of its life, when it burns fuel steadily. Our Sun’s fuel will run out in approximately 6 billion years, and it will then move on to the next stage of its life when it will turn into a red giant. Astronomers studying NGC 2203, which contais stars that are roughly twice as massive as our Sun, found that their rotation might be a factor as to why some of the stars stay longer than usual in this main-sequence phase of their life.
This is the best resolution obtained of the star cluster to date.
Credit:
ESA/Hubble & NASA, L. Girardi
CoordinatesPosition Position (RA): 6 4 39.02
Position (Dec): -75° 26' 0.45"
Field of view: 2.57 x 2.67 arcminutes
Orientation: North is 152.0° right of vertical
Colours & filters Band Wavelength Telescope
Optical U 336 nm Hubble Space Telescope WFC3
Optical g 475 nm Hubble Space Telescope WFC3
Optical I 814 nm Hubble Space Telescope WFC3
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== {{int:filedesc}} == {{Information |description={{en|1='''Stellar Sweet Shop Looking its best ever is the star cluster NGC 2203, here imaged by the NASA/ESA Hubble Space Telescope. Aside from its dazzling good looks, this cluster of stars contains lots of astronomical treats that have helped astronomers puzzle together the lifetimes of stars. A main sequence star, like our Sun, is the term applied to a star during the longest period of its life, when it burns fuel steadily. Our Sun’s fue...
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