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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

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.


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      <creatorName>Shcherbina, M. P.</creatorName>
      <givenName>M. P.</givenName>
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      <affiliation>Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia</affiliation>
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      <creatorName>Barabanov, S. I.</creatorName>
      <givenName>S. I.</givenName>
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      <creatorName>Irsmambetova, T. R.</creatorName>
      <givenName>T. R.</givenName>
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      <affiliation>Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia</affiliation>
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      <creatorName>Kokhirova, G. I.</creatorName>
      <givenName>G. I.</givenName>
      <familyName>Kokhirova</familyName>
      <affiliation>Acad Sci Republ Tajikistan, Inst Astrophys, Dushanbe, Tajikistan</affiliation>
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      <creatorName>Khamroev, U. Kh.</creatorName>
      <givenName>U. Kh.</givenName>
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      <affiliation>Acad Sci Republ Tajikistan, Inst Astrophys, Dushanbe, Tajikistan</affiliation>
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      <creatorName>Khamitov, I. M.</creatorName>
      <givenName>I. M.</givenName>
      <familyName>Khamitov</familyName>
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    <creator>
      <creatorName>Bikmaev, I. F.</creatorName>
      <givenName>I. F.</givenName>
      <familyName>Bikmaev</familyName>
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    <creator>
      <creatorName>Gumerov, R. I.</creatorName>
      <givenName>R. I.</givenName>
      <familyName>Gumerov</familyName>
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      <creatorName>Irtuganov, E. N.</creatorName>
      <givenName>E. N.</givenName>
      <familyName>Irtuganov</familyName>
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    <creator>
      <creatorName>Mel'nikov, S. S.</creatorName>
      <givenName>S. S.</givenName>
      <familyName>Mel'nikov</familyName>
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  <titles>
    <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</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2019</publicationYear>
  <dates>
    <date dateType="Issued">2019-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/114078</alternateIdentifier>
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  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1134/S0038094619040014</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">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.</description>
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