Icarus 421 (2024) 116215
Available online 11 July 2024
0019-1035/© 2024 Elsevier Inc. All rights are reserved, including those for text and data mining, AI training, and similar technologies.
Detailed
chemical
composition
analysis
of the Soi crater
region
on Titan
A. Solomonidou
a,b,*
, M.J.
Malaska
c
, R.M.C.
Lopes
c
, A. Coustenis
b
, A.M.
Schoenfeld
c
,
B. Schmitt
d
, S.P.D.
Birch
e
, A. Le Gall
f,g
, K. Lawrence
c
, C. Matsoukas
h
, S.D. Wall
i
, C. Elachi
i
a
Hellenic
Space
Center,
Athens,
Greece
b
LESIA,
Paris
Observatory-PSL,
CNRS,
Sorbonne
Univ.,
Univ.
de Paris
Cit
́
e, Meudon,
France
c
Jet Propulsion
Laboratory,
California
Institute
of Technology,
Pasadena,
CA, USA
d
Univ.
Grenoble
Alpes,
IPAG,
F-38000
Grenoble,
France
e
Department
of Earth,
Environmental
and Planetary
Sciences,
Brown
University,
Providence
RI, USA
f
LATMOS/IPSL,
UVSQ
Universit
́
e Paris-Saclay,
Sorbonne
Universit
́
e, CNRS,
France
g
Institut
Universitaire
de France,
Paris,
France
h
KTH
Royal
Institute
of Technology,
Stockholm,
Sweden
i
California
Institute
of Technology,
Pasadena,
CA, USA
ARTICLE
INFO
Keywords:
Titan
Surface
composition
Radiative
transfer
Ocean
worlds
Icy satellites
ABSTRACT
The Soi crater
region
(0
◦
to 60
◦
N, 180
◦
W to