Table 1: Values for the mass of (4) Vesta determined by other authors.
Mass and $\sigma$ Perturbed Reference

in $10^{-10}~ M_{\odot}$ bodies

$1.17 \pm 0.10$ (197) Arete Hertz (1966)

$1.20 \pm 0.08$ (197) Arete Hertz (1968)

$1.38 \pm 0.12$ (197) Arete Schubart $\&$ Matson

(1979)

$1.50 \pm 0.03$ Mars Standish $\&$ Hellings

(1989)

1.34 DE403 solution Standish et al.

(1995)

$1.38 \pm 0.06$ (197) Arete Rapaport $\&$ Viateau

(1998)

$1.35 \pm 0.01$ DE405 solution Standish (1998)

$1.52 \pm 0.15$ (1) Ceres Hilton (1999)

$1.34 \pm 0.09$ 22 asteroids Kuznetsov (1999)

$1.36 \pm 0.05$ 26 asteroids Michalak (2000)

$1.46 \pm 0.10$ 4 asteroids Krasinsky (2001)

$1.29 \pm 0.02$ (197) Arete Viateau $\&$ Rapaport

(2001)

$1.31 \pm 0.02$ (17) Thetis Viateau $\&$ Rapaport

(2001)

**Table 1:** Values for the mass of (4) Vesta determined by other authors.
Mass and $\sigma$	Perturbed	Reference
in $10^{-10}~ M_{\odot}$	bodies
$1.17 \pm 0.10$	(197) Arete	Hertz (1966)
$1.20 \pm 0.08$	(197) Arete	Hertz (1968)
$1.38 \pm 0.12$	(197) Arete	Schubart $\&$ Matson
		(1979)
$1.50 \pm 0.03$	Mars	Standish $\&$ Hellings
		(1989)
1.34	DE403 solution	Standish et al.
		(1995)
$1.38 \pm 0.06$	(197) Arete	Rapaport $\&$ Viateau
		(1998)
$1.35 \pm 0.01$	DE405 solution	Standish (1998)
$1.52 \pm 0.15$	(1) Ceres	Hilton (1999)
$1.34 \pm 0.09$	22 asteroids	Kuznetsov (1999)
$1.36 \pm 0.05$	26 asteroids	Michalak (2000)
$1.46 \pm 0.10$	4 asteroids	Krasinsky (2001)
$1.29 \pm 0.02$	(197) Arete	Viateau $\&$ Rapaport
		(2001)
$1.31 \pm 0.02$	(17) Thetis	Viateau $\&$ Rapaport
		(2001)

Source LaTeX | All tables | In the text

	1 Introduction
	2 Procedure of mass determination
	3 Results and discussion
	4 Conclusion
	References