1 Ocak 2019 Dergi makalesi Açık Erişim

Busarev, V. V.; Shcherbina, M. P.; Barabanov, S. I.; Irsmambetova, T. R.; Kokhirova, G. I.; Khamroev, U. Kh.; Khamitov, I. M.; Bikmaev, I. F.; Gumerov, R. I.; Irtuganov, E. N.; Mel'nikov, S. S.

Dublin Core

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  <dc:creator>Busarev, V. V.</dc:creator>
  <dc:creator>Shcherbina, M. P.</dc:creator>
  <dc:creator>Barabanov, S. I.</dc:creator>
  <dc:creator>Irsmambetova, T. R.</dc:creator>
  <dc:creator>Kokhirova, G. I.</dc:creator>
  <dc:creator>Khamroev, U. Kh.</dc:creator>
  <dc:creator>Khamitov, I. M.</dc:creator>
  <dc:creator>Bikmaev, I. F.</dc:creator>
  <dc:creator>Gumerov, R. I.</dc:creator>
  <dc:creator>Irtuganov, E. N.</dc:creator>
  <dc:creator>Mel'nikov, S. S.</dc:creator>
  <dc:date>2019-01-01</dc:date>
  <dc:description>This paper presents the results that confirm the sublimation activity at the perihelion of the primitive main-belt asteroids 779 Nina, 704 Interamnia, and 145 Adeona; this activity was first discovered in September 2012 (Busarev et al., 2015; Busarev et al., 2016). The new spectrophotometric and/or UBVRI photometric observations of Nina, Interamnia, and Adeona were carried out in 2016-2018 during a regular perihelion passage of these asteroids. Additionally, probable spectral signs of weak sublimation activity were discovered on another two primitive main-belt asteroids, 51 Nemausa and 65 Cybele. In this study, we discuss the conditions for the occurrence of a periodic and/or continuous sublimation process on main-belt asteroids with low-temperature mineralogy; in particular, the conditions that are associated with their formation close to the "snow line" or beyond. We also consider general evolution processes that are able sustain a sufficiently high concentration of water ice close to the surface of the bodies in question and, therefore, their continuous sublimation activity, or lead to the recurrence of extinct activity.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/114078</dc:identifier>
  <dc:identifier>oai:zenodo.org:114078</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:source>SOLAR SYSTEM RESEARCH 53(4) 261-277</dc:source>
  <dc:title>Confirmation of the Sublimation Activity of the Primitive Main-Belt Asteroids 779 Nina, 704 Interamnia, and 145 Adeona, as well as its Probable Spectral Signs on 51 Nemausa and 65 Cybele</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
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