Table of Contents
12 relations: A-type main-sequence star, Apparent magnitude, Camelopardalis, Circumpolar star, Epoch (astronomy), Orbital eccentricity, Orbital period, Perseus (constellation), Radial velocity, Star system, Stellar classification, Stellar parallax.
A-type main-sequence star
An A-type main-sequence star (A) or A dwarf star is a main-sequence (hydrogen burning) star of spectral type A and luminosity class (five). 2 Camelopardalis and a-type main-sequence star are a-type main-sequence stars.
See 2 Camelopardalis and A-type main-sequence star
Apparent magnitude
Apparent magnitude is a measure of the brightness of a star or other astronomical object.
See 2 Camelopardalis and Apparent magnitude
Camelopardalis
Camelopardalis is a large but faint constellation of the northern sky representing a giraffe.
See 2 Camelopardalis and Camelopardalis
Circumpolar star
A circumpolar star is a star that, as viewed from a given latitude on Earth, never sets below the horizon due to its apparent proximity to one of the celestial poles.
See 2 Camelopardalis and Circumpolar star
Epoch (astronomy)
In astronomy, an epoch or reference epoch is a moment in time used as a reference point for some time-varying astronomical quantity.
See 2 Camelopardalis and Epoch (astronomy)
Orbital eccentricity
In astrodynamics, the orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle.
See 2 Camelopardalis and Orbital eccentricity
Orbital period
The orbital period (also revolution period) is the amount of time a given astronomical object takes to complete one orbit around another object.
See 2 Camelopardalis and Orbital period
Perseus (constellation)
Perseus is a constellation in the northern sky, named after the Greek mythological hero Perseus.
See 2 Camelopardalis and Perseus (constellation)
Radial velocity
The radial velocity or line-of-sight velocity of a target with respect to an observer is the rate of change of the vector displacement between the two points.
See 2 Camelopardalis and Radial velocity
Star system
A star system or stellar system is a small number of stars that orbit each other, bound by gravitational attraction.
See 2 Camelopardalis and Star system
Stellar classification
In astronomy, stellar classification is the classification of stars based on their spectral characteristics.
See 2 Camelopardalis and Stellar classification
Stellar parallax
Stellar parallax is the apparent shift of position (parallax) of any nearby star (or other object) against the background of distant stars.
See 2 Camelopardalis and Stellar parallax
References
Also known as 2 Cam.