Extinction in the Coma of Comet 17p/Holmes

On 2007 October 29, the outbursting comet 17P/Holmes passed within 0 79 of a background star. We recorded the event using optical, narrowband photometry and detect a 3%–4% dip in stellar brightness bracketing the time of closest approach to the comet nucleus. The detected dimming implies an optical depth τ ≈ 0.04 at 1 5 from the nucleus and an optical depth toward the nucleus center τ n < 13.3. At the time of our observations, the coma was optically thick only within ρ ≲ 0 01 from the nucleus. By combining the measured extinction and the scattered light from the coma, we estimate a dust red albedo p d = 0.006 ± 0.002 at α = 16° phase angle. Our measurements place the most stringent constraints on the extinction optical depth of any cometary coma.