Solar radius

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Template:Short description

Conversion of nominal solar radius
1 Template:Solar radius = Units
Decimal Scientific notation
Template:Val Template:Val metres
Template:Val Template:Val kilometres
Template:Val Template:Val astronomical unit
Template:Val Template:Val miles
Template:Val Template:Val light-year
Template:Val Template:Val parsec
Template:Val Template:Val light-seconds

A solar radius is a unit of distance, commonly understood as 695,700 km and expressed as R⊙, used mostly to express the size of an astronomical 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.[1] One solar radius can be described as follows:1R⊙=6.957×108 mThis 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.

Template:Convert is approximately 10 times the average radius of Jupiter; 109 times the 6378 km radius of the Earth at its equator; and 1215 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, which induces an oblateness in the order of 10 parts per million.[2]

The solar diameter is double the solar radius.

Measurements

Evolution of the solar luminosity, radius and effective temperature compared to the present-day Sun. After Ribas (2009)[3]

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 Template:Convert.[4]

Haberreiter, Schmutz & Kosovichev (2008)[1] determined the radius corresponding to the solar photosphere to be Template:Convert. This new value is consistent with helioseismic estimates; the same study showed that previous estimates using inflection point methods had been overestimated by approximately Template:Cvt.

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) to be equal to exactly Template:Val.[5] 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[6] only known to about an accuracy of ±Template:Val).

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:

Radius of other objects relative to the Sun's radius
Name Radius Template:Nowrap Radius (kilometers)
Milky Way Template:Val Template:Val[7]
WOH G64 A 1,540[8] Template:Val
UY Scuti 909[9] Template:Val
Betelgeuse 764[10] Template:Val
Antares A 680[11] Template:Val
Rigel A 74.1[12] Template:Val
Aldebaran 45.1[13] Template:Val
Arcturus 25.4[14] Template:Val
Pollux 9.06[15] Template:Val
Sirius A 1.711[16] Template:Val
Sun 1 Template:Val
Proxima Centauri 0.1542[17] Template:Val
Jupiter 0.1028 Template:Val[18]
Saturn 0.0866 Template:Val[18]
Uranus 0.03673 Template:Val[18]
Neptune 0.03559 Template:Val[18]
Earth 0.009168 Template:Val[18]
Venus 0.00869 Template:Val[18]
Mars 0.00488 Template:Val[18]
Mercury 0.0035 Template:Val[18]
Moon 0.0025 Template:Val[19]
Pluto 0.0017 Template:Val[18]

See also

References

Template:Reflist

Template:Units of length used in Astronomy Template:Portal bar