"Solar mass" හි සංශෝධන අතර වෙනස්කම්

විකිපීඩියා වෙතින්
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{{Infobox unit
| name = Solar mass
| image = Sun vs planets en.svg
| caption = The Sun contains more than 99% of the mass of the Solar System. Bodies lighter than [[Saturn]] are not visible at this scale.
| standard = [[astronomy]]
| quantity = [[mass]]
| symbol = {{Solar mass}}
| extralabel = In [[SI base unit]]s
| extradata = {{val|1.98847|0.00007|e=30|u=kilogram}}<ref>{{cite web |year=2014 |title=Astronomical Constants |url=http://asa.usno.navy.mil/static/files/2014/Astronomical_Constants_2014.pdf |pages=2 |access-date=10 April 2019 |work=[[The Astronomical Almanac]]}}</ref><ref>{{cite web |url=http://physics.nist.gov/cgi-bin/cuu/Value?bg |title=Newtonian constant of gravitation |access-date=10 April 2019 |work=Physical Measurement Laboratory}}</ref>
}}

[[File:Rho Cassiopeiae Sol VY Canis Majoris - 2019-05-14.svg|thumb|400px|Size and mass of very large stars, from right to left: [[VY Canis Majoris]] ({{solar mass|17 ± 8}}), [[Betelgeuse]] ({{solar mass|11.6 ± 5.0}}), [[Rho Cassiopeiae]] ({{solar mass|14-30}}), and the blue [[Pistol Star]] ({{solar mass|27.5}}). The concentric ovals indicate the size of Neptune's (blue), Jupiter's (red) and the Earth's (grey) orbits. Properly scaled, the [[Sun]] ({{solar mass|1}}) only appears as a tiny dot in the center of the ovals (click for higher resolution to see Earth orbit and Sun).]]
[[File:Rho Cassiopeiae Sol VY Canis Majoris - 2019-05-14.svg|thumb|400px|Size and mass of very large stars, from right to left: [[VY Canis Majoris]] ({{solar mass|17 ± 8}}), [[Betelgeuse]] ({{solar mass|11.6 ± 5.0}}), [[Rho Cassiopeiae]] ({{solar mass|14-30}}), and the blue [[Pistol Star]] ({{solar mass|27.5}}). The concentric ovals indicate the size of Neptune's (blue), Jupiter's (red) and the Earth's (grey) orbits. Properly scaled, the [[Sun]] ({{solar mass|1}}) only appears as a tiny dot in the center of the ovals (click for higher resolution to see Earth orbit and Sun).]]


5 පේළිය: 16 පේළිය:
:{{math|{{solar mass}} {{=}} {{val|1.98855|0.00025|e=30|u=kilogram}}}}
:{{math|{{solar mass}} {{=}} {{val|1.98855|0.00025|e=30|u=kilogram}}}}


=ආශ්‍රිත==
{{අසම්පූර්ණ}}
*[[Chandrasekhar limit]]
*[[Gaussian gravitational constant]]
*[[Orders of magnitude (mass)]]
*[[Stellar mass]]
*[[Sun]]

==මූලාශ්‍ර==
{{reflist}}

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[[ප්‍රවර්ගය:තාරකා විද්‍යාව]]
[[ප්‍රවර්ගය:තාරකා විද්‍යාව]]

{{අසම්පූර්ණ}}

03:22, 12 මාර්තු 2021 වන විට නවතම සංශෝධනය

Solar mass
The Sun contains more than 99% of the mass of the Solar System. Bodies lighter than Saturn are not visible at this scale.
General information
Unit systemastronomy
Unit ofmass
SymbolM
In SI base units(1.98847±0.00007)×1030 kg[1][2]
Size and mass of very large stars, from right to left: VY Canis Majoris (17 ± 8 M), Betelgeuse (11.6 ± 5.0 M), Rho Cassiopeiae (14-30 M), and the blue Pistol Star (27.5 M). The concentric ovals indicate the size of Neptune's (blue), Jupiter's (red) and the Earth's (grey) orbits. Properly scaled, the Sun (1 M) only appears as a tiny dot in the center of the ovals (click for higher resolution to see Earth orbit and Sun).

සූර්ය ස්කන්ධ (ඉංග්‍රීසි:  solar mass) (M) යනු තාරකා විද්‍යාවේ සම්මත ඒකකයකි. එය ආසන්න වශයෙන් 2×1030 kg පමණ වේ.

M = (1.98855±0.00025)×1030 kg

ආශ්‍රිත=[සංස්කරණය]

මූලාශ්‍ර[සංස්කරණය]

  1. "Astronomical Constants" (PDF). The Astronomical Almanac. 2014. p. 2. සම්ප්‍රවේශය 10 April 2019.
  2. "Newtonian constant of gravitation". Physical Measurement Laboratory. සම්ප්‍රවේශය 10 April 2019.
"https://si.wikipedia.org/w/index.php?title=Solar_mass&oldid=477058" වෙතින් සම්ප්‍රවේශනය කෙරිණි