Hidden Mass in the Asteroid Belt

By G. Krasinsky, E. Pitjeva, M. Vasilyev, E. Yagudina. 2002

192 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/4acf8366cb8843538c1b110ab4686205d2e10357

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In Astronomy and Astrophysics

Citations in the corpus

Processes that Promote and Deplete the Exosphere of Mercury (2007, methodology): “…which is assumed to be 2.5 g cm−3 consistent with the measurements of the densities of stratospheric cosmic dust particles (Rietmeijer 1998) and with densities data of S-type igneous asteroids (e.g., Krasinsky et al. 2002), which are the main constituents of the inner part of the Main Belt.”
Asteroids Were Born Big (2009, background): “tion of Mars, which constrains the contribution of asteroids too small to be observed individually (Krasinsky et al., 2002).”
Transience of Hot Dust around Sun-like Stars (2006, result): “…it is worth pointing out that this model is in excellent agreement with the properties of the asteroid belt in the solar system, since for a 4500 Myr belt at 3 AU the model predicts Mmax = 0.4× 10−3M⊕, which is close to the inferred mass of the asteroid belt of 0.6 × 10−3M⊕ (Krasinsky et al. 2002).”
THE LINK BETWEEN PLANETARY SYSTEMS, DUSTY WHITE DWARFS, AND METAL-POLLUTED WHITE DWARFS (2012, background): “This gives us the total mass of our asteroids normalized by the mass of the Solar System’s asteroid belt (Mbelt = 3.6×10 24 g) (Krasinsky et al. 2002).”
EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER's ORBIT (2010, background): “The current mass of the asteroid belt is estimated to be 3.6×1021 kg (Krasinsky et al., 2002) or 6×10−4 Earth masses (M⊕).”
INPOP06: a new numerical planetary ephemeris (2008, background): “The Krasinsky et al (2002) proposition of adding an asteroid ring potential in the inner planet orbit computations is also extended to the outer planets.”
The Compositional Structure of the Asteroid Belt (2015, background): “A. et al. (2008) The distribution of basaltic asteroids in the Main Belt.”
Relativistic effects and solar oblateness from radar observations of planets and spacecraft (2005, background): “…barycentric coordinate system are r̈i = A + B + C + D, where A are the Newtonian gravitational accelerations, B are the relativistic terms (Newhall et al. 1983), C are the terms attributable to the solar oblateness, and D are the terms attributable to the asteroid ring (Krasinsky et al. 2002).”
Phenomenology of the Lense-Thirring effect in the solar system (2010, background): “Fourth line: nominal values of the perihelion precessions due to the ring of the minor asteroids for mring = 5× 10 M⊙ (Krasinsky et al. 2002); the uncertainty in it amounts to δmring = 1× 10 M⊙ (Krasinsky et al.”
Relativistic effects and dark matter in the Solar system from observations of planets and spacecraft (2013, methodology): “…asteroid belt substantially affecting the motion of Mars and some other planets is modeled in the EPM ephemerides by using the motion of 301 large asteroids and a homogeneous material ring representing the influence of all other numerous small asteroids (Krasinsky et al., 2002; Pitjeva, 2010a).”
Building Terrestrial Planets (2012, background): “of such an outer edge and how to explain its compatibility with the existence of the asteroid belt between 2 and 4 AU. The asteroid belt has today a very little total mass (about 6x10-4 Earth masses; Krasinsky et al. 2002), but it must have contained at least a thousand times more solid material whe”