Astrophysics (Index)About

light-year

(ly)
(distance that light travels in a year)

A light-year is the distance that light travels in a year. The count of light-years to some object under observation also represents how far into the past this view of the object represents, i.e., if a star is ten light-years away, then when we see it, our view is of that star's appearance ten years ago. In the science of astronomy/astrophysics, the unit light-year is often used for communications to the public, but the unit parsec (pc) is generally used in scientific calculations and communication. Approximate equivalences:

The International Astronomical Union (IAU) has standardized a precise definition of the light-year: the speed of light in a vacuum (c) times a Julian year, 365.25 days of standard (SI) seconds. This distance is an exact number of meters because the standard meter is defined in relation to c and the standard second: 9,460,730,472,580,800 meters.


(distance,unit,astronomy)
Further reading:
https://en.wikipedia.org/wiki/Light-year
https://astronomy.swin.edu.au/cosmos/l/Light+Year
https://exoplanets.nasa.gov/faq/26/what-is-a-light-year/

Referenced by pages:
2M1207
3C 273
3C 279
3C 295
3C 48
47 Tucanae (47 Tuc)
51 Eridani b
51 Pegasi b (51 Peg b)
Achernar
AD Leonis (AD Leo)
Algol (Beta Per)
Alpha Centauri (α Centauri)
Andromeda (M31)
Arcturus
astronomical quantities
astronomical unit (AU)
Automated Planet Finder (APF)
AzTEC-3
Barnard's Star
Beta Centauri
Beta Pictoris b (β Pic b)
Canis Major Dwarf Galaxy
Capella
Cassiopeia A
CHIPS
Circinus Galaxy (ESO 97-G13)
Coma Supercluster
Comet Galaxy (PGC 3234374)
cosmological redshift
Crab Nebula (M1)
Elias 2-27
Epsilon Eridani (ε Eridani)
Epsilon Indi (ε Indi)
ESO 137-001
fuzzy dark matter (FDM)
G239-25
Giclas 29-38 (G 29-38)
gigayear (Gy)
Great Attractor
Great Wall
GRO J1655-40
HD 189733 b
HD 209458 b
HD 80606 b
Hercules-Corona Borealis Great Wall (Her-CrB GW)
HL Tau
HR 8799
Hulse-Taylor Binary (PSR B1913+16)
Hyades Cluster
Hydra-Centaurus Supercluster
IC 342
IRAS 13224-3809
J1407
K2-18b
Kapteyn's Star
Kepler-79
Lalande 21185
Large Magellanic Cloud (LMC)
LHS 1140
LHS 3844 b
Local Bubble
Local Group (LG)
Local Interstellar Cloud (LIC)
Luhman 16
Luyten 726-8
M64
M82
M87
Messier 100 (M100)
Messier 106 (M106)
Messier 15 (M15)
Messier 67 (M67)
Messier 74 (M74)
Messier 77 (M77)
Messier 84 (M84)
Milky Way (MW)
NANOGrav
NGC 1600
NGC 253
NGC 2770
NGC 3201
NGC 3314
NGC 6946
NGC 7469
NGC 7727
OB association
observable universe
Oort Cloud
Orion
parsec (pc)
Perseus-Pisces Supercluster
Pinwheel Galaxy (M101)
Pisces-Cetus Supercluster Complex
Procyon
Proxima b
pulsar timing array (PTA)
Puppis A
quasar (QSO)
Radcliffe wave
Rho Ophiuchi Cloud Complex
Rigel
Ross 154
Ross 248
Sachs-Wolfe effect (SWE)
Sagittarius Dwarf Elliptical Galaxy (Sgr dE)
Sagittarius Dwarf Irregular Galaxy (SagDIG)
Scholz's Star
Sculptor Wall
Sirius
Sloan Great Wall (SGW)
Small Magellanic Cloud (SMC)
SN 1987A (1987A)
SN 2014J
Sombrero Galaxy (M104)
Spindle Galaxy (NGC 5866)
Sun
supercluster
survey depth
Teegarden's Star
TOI 700 d
TRAPPIST-1
Triangulum Galaxy (M33)
TW Hydrae (TW Hya)
Vega
Vela supernova remnant
Voyager
WASP-43b
Whirlpool Galaxy (M51a)
WISE 0855-0714 (W0855)
WISE 1506+7027
Wolf 359

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