HD 108147

F8-type Main-Sequence Star (Yellow-White)
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HD 108147 Encyclopedic Information

HD 108147 is a notable astronomical star system. Observatories have captured its image, revealing its characteristics within the Crux constellation. According to the archive, it lies approximately 38.82 light-years from Earth.

History & Significance

As an established member of the Crux constellation, HD 108147 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 HD 108147 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 HD 108147 determine whether it will gently fade into a white dwarf or end its life in a spectacular supernova.

✨ Cosmic Secrets & Fun Facts

  • HD 108147 resides approximately 38.82 light-years away. The photons capturing your eye today actually left the star 38.82 years ago!
  • Every typical star you can see in the night sky is physically larger and brighter than our Sun.
Image/Render Reference: NASA / SDO (Yellow Star Concept)
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Related Celestial Bodies

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

Acrux Acrux B0.5-type Subgiant (Blue-White) Mimosa Mimosa B0.5-type Giant (Blue-White) Epsilon Crucis Epsilon Crucis K3-type Giant (Orange) NGC 7447 NGC 7447 Star