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Trash variable star 5 EP

HIP 108057

RA 328.3973° · Dec -82.7788° · star

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Score breakdown

· 1 badge
5 pts · Trash
Trash 15 pts → Common
  • Variable star +5
Total score 5

10 more points to reach Common.

Badges

  • Variable star · +5

Trivia

Could we get there?

  • Verdict. Hopelessly far for any craft humanity can build today.

Getting there

  • Aboard Voyager 1. ≈ 13.4 million years at Voyager 1's speed (17 km/s).
  • Fastest probe ever. ≈ 1.2 million years even at the Parker Solar Probe's 192 km/s.
  • At 10% light speed. ≈ 7603 years in a starship at a tenth of light speed.
  • Distance. 760 light-years from Earth.

Look-back time

  • Look-back time. The light you'd see left around the year 1266.

Saying hello

  • Say hello. A radio message and its reply would take 1521 years round-trip.

Properties

absmag
5.182
constellation
Oct
dist ly
760.2703
mag
12.02
name
HIP 108057

About HIP 108057

HIP 108057 is a trash variable star. It lies about 760.3 light-years from Earth, sits in the constellation Oct and shines at apparent magnitude 12.02.

HIP 108057 is a trash variable star worth 5 points across 1 science badge. Explore its facts, badges and place on the sky map, then add it to your dex on Spacedle.

How to see it

Look for HIP 108057 in the constellation Oct. At apparent magnitude 12.02, it takes a larger telescope or a long-exposure image to capture.

Like any astronomical target, HIP 108057 is best seen from a dark site away from city lights, and when it is above the horizon depends on your latitude and the time of year. The visibility panel above works out tonight's viewing window for your saved location.

Why HIP 108057 is a trash variable star

HIP 108057 scores 5 points on Spacedle's rarity scale, which places it in the trash tier. Another 10 points would lift it into a rarer tier.

That score comes from 1 science badge — Variable star — each earned for a real, measurable property of the object. Rarity on Spacedle is never random: the more remarkable an object's astrophysics, the more badges it collects, the higher it scores, and the rarer it ranks.

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Sky imagery and survey data courtesy of Aladin Lite & CDS, Strasbourg. Object data from the NASA Exoplanet Archive, JPL Small-Body Database, and the ATNF Pulsar Catalogue.