activity
19992023
most citedSurface Compositions Across Pluto and Charon

291 citations · 1.9k across the 33 of their papers we have counts for

collaborators
Showing 2020Show all

12 papers · 1 filter

astro-ph.EP2020★ 27 cited

Water abundance at the surface of C-complex main-belt asteroids

Pierre Beck, Jolantha Eschrig, Sandra Potin +4

Recently published space-based observations of main-belt asteroids with the AKARI telescope provide a full description of the 3 μm band, related to the presence of OH bearing miner…

astro-ph.EP2020★ 23 cited

Visible and near-infrared reflectance of hyperfine and hyperporous particulate surfaces

Robin Sultana, Olivier Poch, Pierre Beck +2

The composition of Solar System surfaces can be inferred through reflectance and emission spectroscopy, by comparing these observations to laboratory measurements and radiative tra…

astro-ph.EP2020★ 20 cited

Mineralogy, chemistry and composition of organic compounds in the fresh carbonaceous chondrite Mukundpura: CM1 or CM2?

S. Potin, P. Beck, L. Bonal +7

We present here several laboratory analyses performed on the freshly fallen Mukundpura CM chondrite. Results of infrared transmission spectroscopy, thermogravimetry analysis and re…

astro-ph.EP2020★ 26 cited

Low-phase spectral reflectance and equivalent geometric albedo of meteorites powders

Pierre Beck, Bernard Schmitt, Sandra Potin +2

The reflectance of a particulate surface depends on the phase angle at which it is observed. This is true for laboratory measurements on powders of natural materials as well as rem…

astro-ph.EP2020★ 52 cited

On the Origin and Thermal Stability of Arrokoths and Plutos Ices

C. M. Lisse, L. A. Young, D. P. Cruikshank +30

We discuss in a thermodynamic, geologically empirical way the long-term nature of the stable majority ices that could be present in Kuiper Belt Object 2014 MU69 after its 4.6 Gyr r…

astro-ph.EP2020★ 20 cited

Modeling Pluto's Minimum Pressure: Implications for Haze Production

Perianne E. Johnson, Leslie A. Young, Silvia Protopapa +6

Pluto has a heterogeneous surface, despite a global haze deposition rate of ~1 micrometer per orbit (Cheng et al., 2017; Grundy et al., 2018). While there could be spatial variatio…