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2011 SP189 (French Wikipedia)

Analysis of information sources in references of the Wikipedia article "2011 SP189" in French language version.

refsWebsite
Global rank French rank
3arxiv.org
69th place
232nd place
2issn.org
57th place
4th place
2doi.org
2nd place
3rd place
2oup.com
485th place
416th place
1nasa.gov
75th place
160th place
1minorplanetcenter.net
1,397th place
672nd place

arxiv.org (Global: 69th place; French: 232nd place)

  • (en) A. A. Christou, N. Georgakarakos, M. ´Cuk, A. Dell’Oro, A. Marshall-Lee, A. Humpage, « New asteroid clusters and evidence of collisional fragmentation in the L5 Trojan cloud of Mars », ESO Astronomy & Astrophysics manuscript no. new_mt_clusters,‎ (lire en ligne)
  • (en) Apostolos A. Christou, Galin Borisov, Aldo Dell’Oro, Seth A. Jacobson, Alberto Cellino, Eduardo Unda-Sanzana, « Population control of Mars Trojans by the Yarkovsky & YORP effects », arXiv:1907.12858,‎ (lire en ligne) :

    « We have carried out numerical simulations to confirm that they are stable L5 Trojans of Mars and that their orbital evolution is similar to that of previously recognised family members. 2011 SP189 is also the faintest member so far identified, with H = 20.9. »

  • (en) Apostolos A. Christou, Galin Borisov, Aldo Dell’Oro, Seth A. Jacobson, Alberto Cellino, Eduardo Unda-Sanzana, « Population control of Mars Trojans by the Yarkovsky & YORP effects », Astrophysics > Earth and Planetary Astrophysics,‎ (lire en ligne) :

    « For the EC4 cluster we obtain nominal diameter estimates of 276m (2018 EC4), 191m (2011 SP189) and 175m (2018 FM29), yielding same-density mass ratios in the range 0.25-0.77, generally high for products of YORP-induced rotational fission (mass ratio ∼0.2; Pravec et al. 2010, 2018). »

doi.org (Global: 2nd place; French: 3rd place)

dx.doi.org

  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le )
  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le ) :

    « we will assume that these objects are the result of one or more YORP break-up events. The absolute value of the difference between the value of TMars for the object and that of Eureka is shown in Table 1 as ΔTMars. From these values, we find that ΔTMars < 0.054 could be compatible with a common origin under the assumptions made. On the other hand, we have that the Martian Trojan with the value of the Tisserand parameter closest to that of Eureka is 2011 UN63 followed by 2011 SP189 (see Table 1). »

issn.org (Global: 57th place; French: 4th place)

portal.issn.org

  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le )
  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le ) :

    « we will assume that these objects are the result of one or more YORP break-up events. The absolute value of the difference between the value of TMars for the object and that of Eureka is shown in Table 1 as ΔTMars. From these values, we find that ΔTMars < 0.054 could be compatible with a common origin under the assumptions made. On the other hand, we have that the Martian Trojan with the value of the Tisserand parameter closest to that of Eureka is 2011 UN63 followed by 2011 SP189 (see Table 1). »

minorplanetcenter.net (Global: 1,397th place; French: 672nd place)

nasa.gov (Global: 75th place; French: 160th place)

ssd.jpl.nasa.gov

oup.com (Global: 485th place; French: 416th place)

academic.oup.com

  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le )
  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le ) :

    « we will assume that these objects are the result of one or more YORP break-up events. The absolute value of the difference between the value of TMars for the object and that of Eureka is shown in Table 1 as ΔTMars. From these values, we find that ΔTMars < 0.054 could be compatible with a common origin under the assumptions made. On the other hand, we have that the Martian Trojan with the value of the Tisserand parameter closest to that of Eureka is 2011 UN63 followed by 2011 SP189 (see Table 1). »