Astrophysics (Index)About

solar mass

(MSun, Msun, M)
(mass unit representing the mass of the Sun)

The unit, solar mass, the mass of the Sun, is commonly used as a unit of mass for astronomical objects. It is approximately 2 × 1030 kilograms, with 1.98847 × 1030 kg being a nominal value based on recent respected determinations of the actual mass. Some example masses using the solar mass unit:

Body solar masses
Jupiter 0.00095
Neptune 5 × 10-5
Earth 3 × 10-6
Moon 3.69 × 10-8
O-type main-sequence (MS) star 16 to 100+
G-type MS star 0.8 to 1.04
M-type MS star 0.08 to 0.45
Taurus-Auriga Complex 35000
Milky Way 1.5 × 1012
Milky Way supermassive black hole 4.3 × 106

A solar mass is roughly 1047 Jupiter masses (MJupiter) or 333000 Earth masses (MEarth).

The actual solar mass is determined by dividing the solar mass parameter by the universal gravitational constant, two values which are determined experimentally. The former is determined much more precisely than the latter, which is currently determined to about six decimal places.


(unit,mass,Sun,astronomy)
Further reading:
https://en.wikipedia.org/wiki/Solar_mass
https://astronomy.swin.edu.au/cosmos/s/solar+mass
https://physics.stackexchange.com/questions/37550/the-official-mass-of-the-sun-as-unit
https://ui.adsabs.harvard.edu/abs/2016AJ....152...41P/abstract

Referenced by pages:
2M1207
A-type star (A)
AB Aurigae (AB Aur)
Abell 85 (A85)
astronomical quantities
asymptotic giant branch (AGB)
B-type star (B)
black hole (BH)
blue horizontal branch (BHB)
Bok globule
Centaurus A
Chandrasekhar limit
CNO cycle
core collapse supernova (CCSN)
DM Tau
DQ Tau
dredge-up
electron capture supernova
exotic star
F-type star (F)
FGK star
galaxy cluster (CL)
galaxy formation
giant molecular cloud (GMC)
Giclas 29-38 (G 29-38)
Hayashi track
HD 163296
HD 209458 b
HD 80606 b
helium flash
Herbig AeBe star (HAeBe)
HFLS3
high-velocity cloud (HVC)
horizontal branch (HB)
initial mass function (IMF)
intermediate-mass black hole (IMBH)
IRAS 13224-3809
Jupiter
K-type star (K)
Kennicutt-Schmidt law
Kepler-79
Laniakea Supercluster
Large Magellanic Cloud (LMC)
Large Millimeter Telescope (LMT)
LB-1
LHS 1140
low mass star (LMS)
luminous blue variable (LBV)
M-type star (M)
M87*
main-sequence lifetime (MS lifetime)
mass
mass-luminosity relation
mass-radius relation
mass-to-light ratio (M/L)
Messier 84 (M84)
Milky Way (MW)
molecular cloud
neutron star (NS)
O-type star (O)
open cluster (OC)
pair-instability supernova (PISN)
PG 1159 star
planetary nebula (PN)
post-main-sequence star
red dwarf
red-giant branch (RGB)
Ross 154
Ross 248
Sag A*
Schwarzschild radius (RS)
Small Magellanic Cloud (SMC)
SMBH formation
Smith Cloud
solar wind
spectral class
standard gravitational parameter (μ)
star formation rate (SFR)
starburst galaxy
stellar wind
stellar-mass black hole (stellar-mass BH)
subdwarf (sd)
substellar object
Sun
supercluster
supermassive black hole (SMBH)
supermassive star (SMS)
supernova progenitor
symbiotic binary (SS)
T-Tauri star (TTS)
Taurus-Auriga Complex (Tau-Aur Complex)
Tolman-Oppenheimer-Volkoff limit (TOV)
TW Hydrae (TW Hya)
Vega
WASP-12b
WASP-33b
WASP-67b
white dwarf (WD)
Wolf-Rayet star
ZTF J1539+5027

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