G-24 - определение. Что такое G-24
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Что (кто) такое G-24 - определение

STAR IN THE CONSTELLATION BOÖTES
G Bootis; G Boötis; 24 Bootis; 24 Boo

G-24         
WIKIMEDIA DISAMBIGUATION PAGE
G-24; G 24; G.24; G24 (disambiguation)
Group of Twenty-Four
Junkers G 24         
  • Junkers G.23 (CH-133) operated by [[Ad Astra Aero]]
AIRLINER FAMILY BY JUNKERS
Junkers G 23; Junkers G.24; Junkers G24; Junkers G23; Junkers G-24; Junkers G-23; Junkers G.23; Junkers F 24; Junkers K 30; Junkers R 42; Junkers JuG-1; Junkers TB-2; Junkers F24kay; Junkers F.24kay; Junkers F.24ko; Junkers G 23W; Junkers G 24h1e
The Junkers G 24 was a German three-engine, all-metal low-wing monoplane passenger aircraft manufactured by Junkers from 1925. Junkers F 24 was the designation for single-engine versions of the same aircraft.
24 (puzzle)         
PUBLIC DOMAIN ARITHMETICAL CARD GAME
24 (game); Math 24; 24 Challenge; Maths24; Challenge 24; 24 Game; 24 game; 24 (card game)
The 24 puzzle is an arithmetical puzzle in which the objective is to find a way to manipulate four integers so that the end result is 24. For example, for the numbers 4, 7, 8, 8, a possible solution is (7-(8\div8))\times4=24.

Википедия

24 Boötis

24 Boötis or g Boötis is a single, yellow-hued star in the constellation Boötes. It is faintly visible to the naked eye with an apparent visual magnitude of +5.59. Based upon an annual parallax shift of 10.00 mas, it is located around 326 light years from the Sun. The star is moving closer to the Sun with a radial velocity of −8 km/s. It is a thick disk star with a high galactic space velocity and an orbital eccentricity of 0.47±0.01 that carries it as close as 3.30±0.05 kpc to the Galactic Center, and as far away as 9.15±0.02 kpc. An extrasolar planet was discovered orbiting this star in 2018.

This is an evolving red giant star with a stellar classification of G4 III-IV Fe-1, with the notation indicating the spectrum shows blended characteristics of a subgiant and giant star with an underabundance of iron. At the age of around 7 billion years old, it has 0.97 times the mass of the Sun but has expanded to 12 times the Sun's radius. The star is radiating 61.7 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,863 K.