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433 Eros: Problems with the meteorite magnetism record in attempting an asteroid match

机译:433爱神:尝试进行小行星比赛时陨石磁记录的问题

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The magnetometer experiment (MAG) onboard the Near-Earth Asteroid Rendezvous (NEAR)-Shoemaker spacecraft detected no global scale magnetization and established a maximum magnetization of 2.1 * 10~(-6) Am~2 kg~(-1) for asteroid 433 Eros. This is in sharp contrast with the estimated magnetization of other S-class asteroids (Gaspra, ~2.4 * 10~(-2) Am~2 kg~(-1); Braille, ~2.8 * 10~(-2) Am~2 kg~(-1)) and is below published values for all types of ordinary chondrites. This includes the L/LL types considered to most closely match 433 Eros based on preliminary interpretations of NEAR remote geochemical experiments. The ordinary chondrite meteorite magnetization intensity data was reviewed in order to assess the reasonableness of an asteroid-meteorite match based on magnetic property measurements. Natural remanent magnetization (NRM) intensities for the ordinary chondrite meteorites show at least a 2 order of magnitude range within each of the H, L, and LL groups, all well above the 2.1 * 10~(-6) Am!2 kg~(-1) level for 433 Eros. The REM values (ratio of the NRM to the SIRM (saturation remanent magnetization)) range over 3 orders of magnitude for all chondrite groups indicating no clear relationship between NMR and the amount of magnetic material. Levels of magnetic noise in chondrite meteorites can be as much as 70% or more of the NRM. Consequently, published values of the NMR should be considered suspect unless careful evaluation of the noise sources is done. NASA Goddard SFC studies of per unit mass intensities in large (>10 000 g) and small (down to <1 g) samples from the same meteorite demonstrate magnetic intensity decreases as size increases. This would appear to be explained by demagnetization due to magnetic vector randomness at unknown scale sizes in the larger samples. This would then argue for some level of demagnetization of large objects such as an asteroid. The possibility that 433 Eros is an LL chondrite cannot be discounted.
机译:近地小行星交会(NEAR)-鞋匠航天器上的磁力计实验(MAG)未检测到整体规模的磁化强度,并确定了小行星433的最大磁化强度为2.1 * 10〜(-6)Am〜2 kg〜(-1)爱神。这与其他S级小行星的估计磁化强度形成鲜明对比(Gaspra,〜2.4 * 10〜(-2)Am〜2 kg〜(-1);盲文,〜2.8 * 10〜(-2)Am〜 2 kg〜(-1)),并且低于所有类型的普通球粒石的公布值。根据对NEAR远程地球化学实验的初步解释,这包括认为最匹配433 Eros的L / LL类型。审查了普通球粒陨石磁化强度数据,以便根据磁性能测量评估小行星与陨石匹配的合理性。普通球粒陨石的自然剩磁强度(NRM)在H,L和LL组中的每个组中显示至少2个数量级范围,都远高于2.1 * 10〜(-6)Am!2 kg〜 (-1)级为433爱神。对于所有球粒陨石基团,REM值(NRM与SIRM的比值(剩余剩磁))的范围都超过3个数量级,表明NMR与磁性材料的含量之间没有明确的关系。球粒陨石中的磁噪声水平可能高达NRM的70%或更高。因此,除非仔细评估噪声源,否则应将NMR的公开值视为可疑的。 NASA Goddard SFC对来自同一陨石的大(> 10000 g)和小(低至<1 g)样品的单位质量强度的研究表明,磁强度随尺寸增加而减小。这似乎是由于较大样本中未知标度尺寸下的磁矢量随机性而导致的退磁解释。然后,这将要求对小行星等大型物体进行一定程度的消磁。 433 Eros是LL球粒陨石的可能性不可小视。

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