absolute magnitude
semidiameter
Proxima Centauri
Proxima
radiometric magnitude
constellation
teraparsec
Altair
subparsec
Urania
visual magnitude
light year
kilolight
apoapsis
point of apoapsis
parallax
coronagraphy
Local Volume
sidereal
bolometric correction
starrise
starlight
Hubble length
Denebola
astronomy unit
luminosity
pseudostar
digit
mean distance
luminosity function
astronomics
Maunder minimum
radial velocity
astrometry
standard candle
light equation
SAO
rational horizon
culmination
space velocity
sidereal time
ascension
secpar
parsec
astroinformatics
minimum
stargaze
asterism
Alderson disk
magnitude
photometry
standard ruler
siren
node
macrolensing
supersun
stargazing
sidereal month
exozodiacal
photoeccentric
quasistellar
Arcturus
AU
nucleocosmochronology
Astronomical Unit
solar gravity
siriometer
oligogalacturonate
Canopus
Zenithal Hourly Rate
Nemesis
star
Mira
astroseismically
heliac
Barnard's Star
starset
nocturlabe
starburst
Olbers' paradox
circle
intercosmic
heliacal
rope
solar parallax
Alphecca
gigaparsec
aster-
exosystem
heavenly body
multiple star
orb
Hertzsprung-Russell diagram
bright giant
bolometric magnitude

English words for '(astronomy) the magnitude that a star would have if it were viewed from a distance of 10 parsecs (32.62 light years) from the earth'

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