130 Elektra

References

↑ "Organic Matter on Asteroid 130 Elektra". Science. 238 (4824): 183–184. 1987. Bibcode:1987Sci...238..183C. doi:10.1126/science.238.4824.183. PMID 17800458. S2CID 46168765. {cite journal}: Unknown parameter |authors= ignored (help)
↑ ^2.0 ^2.1 ^2.2 ^2.3 F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185 (1): 39–63. Bibcode:2006Icar..185...39M. doi:10.1016/j.icarus.2006.06.001. PMC 2600456. PMID 19081813.
↑ ^3.0 ^3.1 ^3.2 130 Elektra and S/2003 (130) 1, orbit data website maintained by F. Marchis. Archived 2007-07-24 at the Wayback Machine
↑ "IAUC 8183". Archived from the original on 2006-05-01. Retrieved 2007-12-25.
↑ Assuming a similar density to the primary.
↑ Discovery Circumstances: Numbered Minor Planets, Minor Planet Centre Archived 2008-05-10 at the Wayback Machine
↑ ASTORB^{[permanent dead link]} orbital elements database, Lowell Observatory
↑ Based in IRAS mean diameter of 182±12 km, a/b ratio of 1.4 as per the following references
↑ ^9.0 ^9.1 "Supplemental IRAS Minor Planet Survey". Archived from the original on 2010-01-17. Retrieved 2007-12-25.{cite web}: CS1 maint: bot: original URL status unknown (link)
↑ PDS node spin vector database(in particular, the synthetic compiled value of a/b=1.4). Archived 2008-05-15 at the Wayback Machine
↑ (130) Elektra and S/2003 (130) 1, at Johnston's archive (maintained by W. R. Johnston). Archived 2011-06-03 at the Wayback Machine
↑ 130 Elektra and S/2003 (130) 1, F. Marchis Archived 2007-07-24 at the Wayback Machine
↑ Error estimate derived from consideration of $M\propto a^{3}/P^{2$ and given errors in a and P. See propagation of uncertainty.
↑ ^14.0 ^14.1 On the extremities of the long axis.
↑ F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185 (1): 39–63. Bibcode:2006Icar..185...39M. doi:10.1016/j.icarus.2006.06.001. PMC 2600456. PMID 19081813.
↑ Supplemental IRAS minor planet survey Archived 2009-08-17 at the Wayback Machine
↑ PDS node taxonomy database Archived 2007-03-10 at the Wayback Machine

Other websites

130 Elektra and S/2003 (130) 1, orbit data website maintained by F. Marchis. Includes adaptive optics image of primary, and satellite orbit diagram.
Data on (130) Elektra from Johnston's archive (maintained by W. R. Johnston)

[CruBro87-1] "Organic Matter on Asteroid 130 Elektra". Science. 238 (4824): 183–184. 1987. Bibcode:1987Sci...238..183C. doi:10.1126/science.238.4824.183. PMID 17800458. S2CID 46168765. {cite journal}: Unknown parameter |authors= ignored (help)

[MarKaaHom06-2] 2.0 ^2.1 ^2.2 ^2.3 F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185 (1): 39–63. Bibcode:2006Icar..185...39M. doi:10.1016/j.icarus.2006.06.001. PMC 2600456. PMID 19081813.

[marchis-3] 3.0 ^3.1 ^3.2 130 Elektra and S/2003 (130) 1, orbit data website maintained by F. Marchis. Archived 2007-07-24 at the Wayback Machine

[iauc8183-4] "IAUC 8183". Archived from the original on 2006-05-01. Retrieved 2007-12-25.

[mass-5] Assuming a similar density to the primary.

[6] Discovery Circumstances: Numbered Minor Planets, Minor Planet Centre Archived 2008-05-10 at the Wayback Machine

[7] ASTORB^{[permanent dead link]} orbital elements database, Lowell Observatory

[about-8] Based in IRAS mean diameter of 182±12 km, a/b ratio of 1.4 as per the following references

[IRAS-9] 9.0 ^9.1 "Supplemental IRAS Minor Planet Survey". Archived from the original on 2010-01-17. Retrieved 2007-12-25.{cite web}: CS1 maint: bot: original URL status unknown (link)

[pds_spin-10] PDS node spin vector database(in particular, the synthetic compiled value of a/b=1.4). Archived 2008-05-15 at the Wayback Machine

[johnston-11] (130) Elektra and S/2003 (130) 1, at Johnston's archive (maintained by W. R. Johnston). Archived 2011-06-03 at the Wayback Machine

[berkeley-12] 130 Elektra and S/2003 (130) 1, F. Marchis Archived 2007-07-24 at the Wayback Machine

[error-13] Error estimate derived from consideration of $M\propto a^{3}/P^{2$ and given errors in a and P. See propagation of uncertainty.

[pointyend-14] 14.0 ^14.1 On the extremities of the long axis.

[harvard39-15] F. Marchis; et al. (2006). "Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey". Icarus. 185 (1): 39–63. Bibcode:2006Icar..185...39M. doi:10.1016/j.icarus.2006.06.001. PMC 2600456. PMID 19081813.

[psi-16] Supplemental IRAS minor planet survey Archived 2009-08-17 at the Wayback Machine

[PDStax-17] PDS node taxonomy database Archived 2007-03-10 at the Wayback Machine