Solar radius

 ( Radius ) 

+ Conversion of nominal solar radius ! 1 = ! Units

astronomical unit

light-year

parsec

A solar radius is a unit of distance, commonly understood as 695,700 km and expressed as $R\_\{\backslash odot\}$, used mostly to express the size of an Astronomy objects relative to that of the Sun, or their distance from it. This length is also called the nominal solar radius. The sun's actual radius, from which the unit of measurement is derived, is usually calculated as the radius from the sun's center out to the layer in the Sun's photosphere where the optical depth equals 2/3. One solar radius can be described as follows:$$1\backslash ,R\_\{\backslash odot\}\; =\; 6.957\backslash times\; 10^8\; \backslash hbox\{\; m\}$$This is an approximation: both because such distance is difficult to measure and can be measured in various ways, and because the sun is not a perfectly spherical object itself, and thus the actual radius varies depending on the point(s) measured and modality of measurement employed.

is approximately 10 times [[the average radius|Jupiter radius]] of [[Jupiter]]; 109 times the 6378 km [[radius|Earth radius]] of the [[Earth]] at its equator; and $\{1\; \backslash over\; 215\}$ or 0.0047 of an astronomical unit, the approximate average distance between Earth and the Sun. The solar radius to the sun's poles 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.

---

Measurements The uncrewed SOHO spacecraft was used to measure the radius of the Sun by timing transits of Mercury across the surface during 2003 and 2006. The result was a measured radius of .

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 .

---

Nominal solar radius In 2015, the International Astronomical Union passed Resolution B3, which defined a set of nominal conversion constants for stellar and planetary astronomy. Resolution B3 defined the nominal solar radius (symbol $R^\{N\}\_\{\backslash odot\}$) to be equal to exactly . The nominal value, which is the rounded value, within the 140 km uncertainty band given by Haberreiter, Schmutz & Kosovichev (2008), was adopted to help astronomers avoid confusion when quoting stellar radii in units of the Sun's radius, even when future observations will likely refine the Sun's actual photospheric radius (which is currently only known to about an accuracy of ±).

---

Examples Solar radii as units of distance measurement are common especially when describing the paths of spacecraft moving close to the sun. Two such spacecraft in the 2010s include:

• Solar Orbiter (which flew as close as to the sun)
• Parker Solar Probe (which flew as close as to the sun)

+Radius of other objects relative to the Sun's radius !Name !Radius !Radius (kilometers)
Milky Way
WOH G64 A	1,540
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

---

See also

• Astronomical unit
• Earth radius
• Jupiter radius
• List of largest stars
• Orders of magnitude (length)
• Solar luminosity
• Solar mass
• Solar parallax

---

External links

Post Comment