+ Conversion of nominal solar radius ! 1 = ! Units |
astronomical unit |
light-year |
parsec |
Solar radius is a unit of distance used to express the size of objects in astronomy relative to the Sun. The solar radius is usually defined as the radius to the layer in the Sun's photosphere where the optical depth equals 2/3:
is approximately 10 times [[the average radius|Jupiter radius]] of [[Jupiter]], 109 times [[the radius|Earth radius]] of the [[Earth]], and 1/215 of an astronomical unit, the approximate distance between Earth and the Sun. The solar radius to either pole and that to the equator differ slightly due to the Sun's [[rotation|stellar rotation]], which induces an [[oblateness|flattening]] in the order of 10 parts per million. The '''solar diameter''' is double the solar radius.
Haberreiter, Schmutz & Kosovichev (2008) determined the radius corresponding to the solar photosphere to be . This new value is consistent with helioseismic estimates; the same study showed that previous estimates using inflection point methods had been overestimated by approximately .
+Radius of another objects relative to the Sun's radius !Name !Radius !Radius (kilometers) | ||
Milky Way | ||
UY Scuti | 909 | |
Betelgeuse | 764 | |
Antares A | 680 | |
Rigel A | 74.1 | |
Aldebaran | 45.1 | |
Arcturus | 25.4 | |
Pollux | 9.06 | |
Sirius A | 1.711 | |
Sun | 1 | |
Proxima Centauri | 0.1542 | |
Jupiter | 0.1028 | |
Saturn | 0.0866 | |
Uranus | 0.03673 | |
Neptune | 0.03559 | |
Earth | 0.009168 | |
Venus | 0.00869 | |
Mars | 0.00488 | |
Mercury | 0.0035 | |
Moon | 0.0025 | |
Pluto | 0.0017 |
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