[2]2022astro-ph.EPPeer-reviewed
Mid-IR Observations of IRAS, AKARI, WISE/NEOWISE and Subaru for Large Icy Asteroid (704) Interamnia: a New Perspective of Regolith Properties and Water Ice Fraction
Haoxuan Jiang, Jianghui Ji, Liangliang Yu & 3 others
What they foundThermal fits suggest Interamnia's surface has regolith grains of about 190 microns and may hide water ice beneath.
Why it mattersIt sharpens estimates of Interamnia's surface and water-ice content.
What they studied
Mid-infrared data from Subaru, IRAS, AKARI and WISE/NEOWISE with a thermophysical model.
[3]2017astro-ph.EPPreprint
New candidates for active asteroids: main-belt (145) Adeona, (704) Interamnia, (779) Nina, (1474) Beira, and near-Earth (162173) Ryugu
Vladimir V. Busarev, Andrei B. Makalkin, Faith Vilas & 2 others
What they foundSpectra suggested subtle comet-like activity on Interamnia and other primitive asteroids near their closest approach to the Sun.
Why it mattersIf confirmed, it hints that ice lies just beneath their surfaces.
What they studied
Ground-based spectral observations in 2012 and 2016.
[4]2015astro-ph.EPPreprint
Spectrophotometry of asteroids 32 Pomona, 145 Adeona, 704 Interamnia, 779 Nina, 330825, and 2012 QG42 and laboratory study of possible analog samples
Vladimir V. Busarev, Sergey I. Barabanov, Vyacheslav S. Rusakov & 2 others
What they foundSpectra of Interamnia showed a feature interpreted as possible sublimation and a temporary coma near perihelion.
Why it mattersIt is one of the first claims of activity on Interamnia; fresh ice exposed by impacts is an alternative explanation.
What they studied
Low-resolution spectrophotometry in September 2012.