2MASS J04414489+2301513

M8.5-type Star (Red)
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2MASS J04414489+2301513 Encyclopedic Information

2MASS J04414489+2301513 is a notable astronomical star system. Observatories have captured its image, revealing its characteristics within the Taurus constellation. According to the archive, it lies approximately 122.22 light-years from Earth.

History & Significance

As an established member of the Taurus constellation, 2MASS J04414489+2301513 has long been charted by astronomers charting the deep sky. Unlike our closest celestial neighbors, stars in this particular region require specialized telescopic equipment or clear, dark skies unaffected by modern light pollution to be fully appreciated in their historical context.

Physical Structure

Astronomical spectroscopy classifies 2MASS J04414489+2301513 as a Star star. This classification dictates its absolute magnitude, lifecycle, and eventual fate. While standard stars fuse hydrogen into helium steadily over billions of years, the unique mass and metallic composition of 2MASS J04414489+2301513 determine whether it will gently fade into a white dwarf or end its life in a spectacular supernova.

✨ Cosmic Secrets & Fun Facts

  • 2MASS J04414489+2301513 resides approximately 122.22 light-years away. The photons capturing your eye today actually left the star 122.22 years ago!
  • Every typical star you can see in the night sky is physically larger and brighter than our Sun.
Image/Render Reference: Wikimedia Commons / NASA / ESA
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Related Celestial Bodies

Explore other significant celestial entities in the Taurus constellation and beyond.

Taygeta Taygeta B6-type Subgiant (Blue-White) Celaeno Celaeno B7-type Subgiant (Blue-White) Beta Tauri Beta Tauri B7-type Giant (Blue-White) NGC 1988 NGC 1988 Star