Thermal Infrared Observations of Asteroid (99942) Apophis with Herschel

Abstract

The near-Earth asteroid (99942) Apophis is a potentially hazardous asteroid. We obtained far-infrared observations of this asteroid with the Herschel Space Observatory's PACS instrument at 70, 100, and 160 micron. These were taken at two epochs in January and March 2013 during a close Earth encounter. These first thermal measurements of Apophis were taken at similar phase angles before and after opposition. We performed a detailed thermophysical model analysis by using the spin and shape model recently derived from applying a 2-period Fourier series method to a large sample of well-calibrated photometric observations. We find that the tumbling asteroid Apophis has an elongated shape with a mean diameter of 375${}_{-10}^{+14}$ m (of an equal volume sphere) and a geometric V-band albedo of 0.30${}_{-0.06}^{+0.05}$. We find a thermal inertia in the range 250-800 Jm${}^{-2}$s${}^{-0.5}$K${}^{-1}$ (best solution at 600 Jm${}^{-2}$s${}^{-0.5}$K${}^{-1}$), which can be explained by a mixture of low conductivity fine regolith with larger rocks and boulders of high thermal inertia on the surface. The thermal inertia, and other similarities with (25143) Itokawa indicate that Apophis might also have a rubble-pile structure. If we combine the new size value with the assumption of an Itokawa-like density and porosity we estimate a mass between 4.4 and 6.2 10${}^{10}$ kg which is more than 2-3 times larger than previous estimates. We expect that the newly derived properties will influence impact scenario studies and influence the long-term orbit predictions of Apophis.

Accepted for publication in Astronomy & Astrophysics, 21 pages, 8 figures, 2 tables

References in corpus (1)

• Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect

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