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- W2165236650 abstract "Observations with the adaptive optics system on the Very Large Telescope reveal that outer main belt asteroid (702) Alauda has a small satellite with primary to secondary diameter ratio of $sim$56. The secondary revolves around the primary in 4.9143 $pm$ 0.007 days at a distance of 1227 $pm$ 24 km, yielding a total system mass of (6.057 $pm$ 0.36) $times$ 10$^{18}$ kg. Combined with an IRAS size measurement, our data yield a bulk density for this B-type asteroid of 1570 $pm$ 500 kg~m$^{-3}$." @default.
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- W2165236650 date "2011-01-04" @default.
- W2165236650 modified "2023-10-16" @default.
- W2165236650 title "MASS AND DENSITY OF THE B-TYPE ASTEROID (702) ALAUDA" @default.
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- W2165236650 doi "https://doi.org/10.1088/0004-637x/727/2/69" @default.
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