absolute magnitude
teraparsec
Local Volume
Hubble length
light millennium
light year
star
light century
kilolight
light day
interval
gigalightyear
parallax second
siriometer
light decade
semidiameter
Milky Way
mesoplanet
light hour
standard ruler
secpar
livid
parsec
infalling
oligogalacturonate
limb
metre
satellite
path length
luminosity distance
horizontal parallax
parallax
astrophysicist
bicapped
astroseismically
Akash
light second
light week
light minute
light equation
Denebola
optical telescope
galaxywide
zero
circle
exozodiacal
mean distance
intercosmic
meter
lucence
subhalo
heavens
microlensing
transcosmic
rational horizon
color
telescopic
ultrashort
giant radio galaxy
hyperradius
transit
Orion Nebula
visual magnitude
macrolensing
sublithospheric
cosmic
node
uranology
astroinformatics
Milky Way Galaxy
astronomy
Im
microverse
subgalactic
supervisual
active galactic nucleus
astronomics
orbitographic
risen
Olbers' paradox
Milky Way System
galactic
annular eclipse
starproof
galactographically
SAO
galactical
coronagraphy
Schmidt telescope
circumgalactic
astrodynamical
femtolensing
AU
black dwarf

English words for 'The intrinsic luminosity that a celestial body would have if viewed from a distance of 10 parsecs or about 32.6 light years.'

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