Binzel R P, Xu S, Bus S J, Skrutskie M F, Meyer M R, Knezek P, Barker E S
Science. 1993 Dec 3;262(5139):1541-3. doi: 10.1126/science.262.5139.1541.
Although ordinary chondrite material dominates meteorite falls, the identification of a main-belt asteroid source has remained elusive. From a new survey of more than 80 small main-belt asteroids comes the discovery of one having a visible and near-infrared reflectance spectrum similar to L6 and LL6 ordinary chondrite meteorites. Asteroid 3628 BoZnemcová has an estimated diameter of 7 kilometers and is located in the vicinity of the 3:1 Jovian resonance, a predicted meteorite source region. Although the discovery of a spectral match may indicate the existence of ordinary chondrite material within the main asteroid belt, the paucity of such detections remains an unresolved problem.
尽管普通球粒陨石物质在陨石坠落中占主导地位,但主带小行星源的确定一直难以捉摸。通过对80多颗小型主带小行星的新调查,发现了一颗小行星,其可见光和近红外反射光谱与L6和LL6普通球粒陨石相似。小行星3628 BoZnemcová估计直径为7公里,位于3:1木星共振附近,这是一个预测的陨石源区。尽管光谱匹配的发现可能表明主小行星带内存在普通球粒陨石物质,但此类探测的稀少仍然是一个未解决的问题。