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Trash variable star 5 EP

62 Sgr

RA 300.6645° · Dec -27.7098° · 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. ≈ 7.9 million years at Voyager 1's speed (17 km/s).
  • Fastest probe ever. ≈ 700.5 thousand years even at the Parker Solar Probe's 192 km/s.
  • At 10% light speed. ≈ 4486 years in a starship at a tenth of light speed.
  • Distance. 449 light-years from Earth.

Look-back time

  • Look-back time. The light you'd see left around the year 1577.

Saying hello

  • Say hello. A radio message and its reply would take 897 years round-trip.

Properties

absmag
-1.262
bv
1.64
constellation
Sgr
dist ly
448.6328
mag
4.43
name
62 Sgr
spect
M4III

About 62 Sgr

62 Sgr is a trash variable star. It lies about 448.6 light-years from Earth, sits in the constellation Sgr, shines at apparent magnitude 4.43 and has spectral type M4III.

62 Sgr 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 62 Sgr in the constellation Sgr. At apparent magnitude 4.43, it can be glimpsed with the unaided eye under dark skies.

Like any astronomical target, 62 Sgr 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 62 Sgr is a trash variable star

62 Sgr 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.