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Trash variable star 5 EP

GL Gl 775

RA 300.6960° · Dec 3.3262° · 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. ≈ 737.1 thousand years at Voyager 1's speed (17 km/s).
  • Fastest probe ever. ≈ 65.5 thousand years even at the Parker Solar Probe's 192 km/s.
  • At 10% light speed. ≈ 419 years in a starship at a tenth of light speed.
  • Distance. 41.9 light-years from Earth.

Look-back time

  • Look-back time. The light you'd see left around the year 1984.

Saying hello

  • Say hello. A radio message and its reply would take 83.9 years round-trip.

Properties

absmag
6.914
bv
1.128
constellation
Aql
dist ly
41.944
mag
7.46
name
GL Gl 775
spect
K4V

About GL Gl 775

GL Gl 775 is a trash variable star. It lies about 41.9 light-years from Earth, sits in the constellation Aql, shines at apparent magnitude 7.46 and has spectral type K4V.

GL Gl 775 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 GL Gl 775 in the constellation Aql. At apparent magnitude 7.46, it is an easy target for binoculars.

Like any astronomical target, GL Gl 775 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 GL Gl 775 is a trash variable star

GL Gl 775 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.