THUNDER: A Titan Orbiter Mission Concept for the New Frontiers Program Designed at the JPL Planetary Science Summer School
The Planetary Science Journal,
Journal Year:
2025,
Volume and Issue:
6(2), P. 45 - 45
Published: Feb. 1, 2025
Abstract
Saturn's
moon
Titan
is
an
enigmatic
icy
world
whose
surface
constantly
modified
by
its
active,
Earthlike
precipitation
system.
Here,
we
propose
the
Titan's
Hydrocarbons:
Uncovering
New
Dimensions
of
Evolutionary
pRocesses
(THUNDER)
mission
concept
to
investigate
how
reflects
nature
interior
and
active
hydrocarbon
cycle.
This
will
change
our
understanding
through
three
science
objectives:
characterizing
heat
material
transport
properties
outer
layer,
tracing
liquid
storage
across
crust,
assessing
total
budget
time.
Frontiers-class
mission,
designed
as
part
Jet
Propulsion
Laboratory
Planetary
Science
Summer
School,
responds
directly
call
for
a
orbiter
in
NASA
Astrobiology
Decadal
Survey
2023–2032.
THUNDER's
focused
geology
geophysics
could
achieve
full
mapping
complement
both
Cassini–Huygens
Dragonfly
missions
using
gravity
science,
radar
with
operational
modes,
visible-to-infrared
spectrometer.
These
instruments
together
give
us
first
look
at
fully
connected
geologically
world,
revolutionizing
bodies,
fluvial
atmospheric
processes,
habitability
geologic
summarize
goals
engineering
approaches,
well
challenges
future
directions
study
before
THUNDER
can
become
viable
concept.
Language: Английский
Glacial isostatic adjustment reveals Mars’s interior viscosity structure
Nature,
Journal Year:
2025,
Volume and Issue:
639(8053), P. 109 - 113
Published: Feb. 26, 2025
Investigating
glacial
isostatic
adjustment
has
been
the
standard
method
to
decipher
Earth's
interior
viscosity
structure1,2,
but
such
an
approach
rarely
applied
other
planets
because
of
a
lack
observational
data3,4.
The
north
polar
cap
Mars
is
only
millions-of-years-old
surface
feature
that
can
induce
measurable
deformation
on
this
planet,
thereby
holding
clues
its
present-day
internal
structure5,6.
Here
we
investigate
emplacement
ice
by
combining
thermal
evolution
models7,
viscoelastic
calculations8
and
radar
observations6.
We
show
downward
motion
northern
regions
ongoing
be
constrained
analyses
time-variable
gravity
field9
NASA's
InSight
seismic
moment
rate10.
Only
models
with
high
viscosities
(2-6
×
1022
Pa
s
for
depths
greater
than
500
km),
strong
mantle
depletion
in
radiogenic
elements
(more
90%)
thick
average
crusts
(thicker
40
km)
are
consistent
negligible
flexure
beneath
seen
radars.
lithosphere
must
deform
at
less
0.13
mm
per
year
have
efficiency
0.3
satisfy
constraints,
respectively.
Our
formed
over
last
1.7-12.0
Myr
further
future
recovery
missions
Mars11,12.
Language: Английский