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Stephenson 2-18 facts for kids

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Stephenson 2-18
Stephenson 2-18 zoomed in, 2MASS survey, 2003.png
Dense starfield around the red supergiant star St2-18 (brightest star in the image) as seen from the 2MASS astronomical survey. The picture was published in 2003.
Credit: Université de Strasbourg/CNRS
Observation data
Epoch J2000      Equinox J2000
Constellation Scutum
Right ascension 18h 39m 02.3709s
Declination -06° 05′ 10.5357″
Evolutionary stage Red supergiant
Spectral type ~M6
Apparent magnitude (G) 15.2631±0.0092
Apparent magnitude (J) 7.150
Apparent magnitude (H) 4.698
Apparent magnitude (K) 2.9
Proper motion (μ) RA: −3.045±0.511 mas/yr
Dec.: −5.950±0.480 mas/yr
Parallax (π) −0.0081 ± 0.3120 mas
Distance 19,560 ly
(6,000 pc)
Radius 2,150 R
Luminosity 90,000–440,000; 630,000 L
Temperature 3,200 K
Other designations
Stephenson 2-18, Stephenson 2 DFK 1, RSGC2-18, 2MASS J18390238-0605106, IRAS 18363-0607
Database references

Stephenson 2-18 (St2-18, also known as Stephenson 2-DFK 1 and RSGC2-18) is a red supergiant (RSG) star. It is close to, and a possible member of, the open cluster Stephenson 2. It is about 6,000 parsecs (20,000 ly) away from Earth in the constellation of Scutum and is one of the largest known stars.

It is also one of the most luminous of its type. It has a radius of 2,150 times that of the Sun, and has a volume 10 billion times that of the Sun. This star has a spectral type of M6, which is pretty unusual for a supergiant star and corresponds to its cool temperature of 3,200 Kelvin.

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