Estimating stellar mean density through seismic inversions

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Table 2

Solar mass and radius.

	Model S	Latest values

GM_⊙ ⁽10²⁶ cm³ s^-2⁾	1.32712445^a	1.32712440^b
G ⁽10^-8 cm³g^-1 s^-2⁾	6.67232	6.67384(80)^c
M_⊙ ⁽10³³ g⁾	1.989	1.98855(24)^d
R_⊙ ⁽10¹⁰ cm⁾	6.9599	6.95613(171)^e
	1.4084	1.4104(12)
	9.3975	9.4128(70)

Notes.

^(a)

Based on the product GM_⊙ using the values from the next two rows.

^(b)

Based on Cox (2000) and references therein.

^(c)

2010 CODATA recommended value, taken from http://physics.nist.gov/cuu/Constants/index.html

^(d)

Based on the ratio GM_⊙/G using the values from the two previous rows.

^(e)

Based on an average of the two values and quoted error bar in Table 3 of Haberreiter et al. (2008).

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