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Trash variable star 5 EP

58 Eri

RA 71.9012° · Dec -16.9345° · 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. ≈ 760.9 thousand years at Voyager 1's speed (17 km/s).
  • Fastest probe ever. ≈ 67.6 thousand years even at the Parker Solar Probe's 192 km/s.
  • At 10% light speed. ≈ 433 years in a starship at a tenth of light speed.
  • Distance. 43.3 light-years from Earth.

Look-back time

  • Look-back time. The light you'd see left around the year 1983.

Saying hello

  • Say hello. A radio message and its reply would take 86.6 years round-trip.

Properties

absmag
4.875
bv
0.632
constellation
Eri
dist ly
43.3028
mag
5.49
name
58 Eri
spect
G3V

About 58 Eri

58 Eri is a trash variable star. It lies about 43.3 light-years from Earth, sits in the constellation Eri, shines at apparent magnitude 5.49 and has spectral type G3V.

58 Eri 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 58 Eri in the constellation Eri. At apparent magnitude 5.49, it can be glimpsed with the unaided eye under dark skies.

Like any astronomical target, 58 Eri 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 58 Eri is a trash variable star

58 Eri 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.