MRO overview: Sixteen years in Mars orbit
Icarus,
Год журнала:
2024,
Номер
419, С. 116102 - 116102
Опубликована: Май 22, 2024
Launched
on
August
12,
2005,
the
Mars
Reconnaissance
Orbiter
(MRO)
entered
orbit
March
10,
2006.
Following
a
period
of
aerobraking,
MRO
completed
its
entry
into
primary
science
in
September
2006,
initiating
program
systematic
observations
that
still
continues.
Five
providers,
including
Italian
Space
Agency,
provided
6
instruments
for
flight,
observing
surface,
atmosphere,
and
subsurface
with
greater
spatial
resolution
coverage
than
ever
before.
Two
investigations
utilized
spacecraft
accelerometers
tracking
orbiter
via
Deep
Network
to
study
upper
atmosphere
densities
gravity
field
planet.
The
data
acquired
by
have
revealed
dynamic
planet
whose
change
from
an
ancient
wetter
climate
drier
today
was
complex
transition
not
simple
"drying
out".
Furthermore,
continues
even
today.
diversity
early
habitable
environments,
ice
ages
recorded
polar
cap
layering
deposits,
repeating
patterns
dust
storms,
revelation
new
features
at
limit
are
all
part
scientific
return
during
nearly
decade
years.
story
mission,
evolution
capabilities,
contributions
our
current
understanding
subject
two
dozen
papers
Icarus
special
issue,
MRO:
Sixteen
Years
Observing
Changing
Mars.
Three
describe
more
detail
instrument
operations
products
over
mission;
several
analysis
techniques
radar,
construction
3-dimensional
views,
atmospheric
sounder,
enabling
better
retrievals
dusty
lower
atmosphere.
Other
report
recent
research
including,
but
limited
to,
dune
movement,
roles
water
carbon
dioxide
surface
change,
attempts
understand
formation
fading
enigmatic
recurring
slope
lineae.
This
paper
describes
general
aspects
spacecraft,
payload,
mission
as
context
issue
papers;
it
also
summarizes
results
support
events
phase
basis
give
time
history
discovery
effort.
Язык: Английский
Revising the Basal Permittivity of the South Polar Layered Deposits of Mars With a Surficial Dust Cover
Geophysical Research Letters,
Год журнала:
2024,
Номер
51(12)
Опубликована: Июнь 22, 2024
Abstract
Bright
basal
reflections
from
the
Mars
Advanced
Radar
for
Subsurface
and
Ionosphere
Sounding
(MARSIS)
have
been
proposed
to
be
consistent
with
permittivities
characteristic
of
a
wet
material
beneath
south
polar
layered
deposits
(SPLD).
The
characterization
recently
formed
impact
crater
highlight
existence
several
meters
thick
ice‐poor
layer
associated
unit
blanketing
large
portion
SPLD.
We
revise
radar
propagation
model
used
invert
permittivity
by
including
surficial
thin
layer.
find
that
inverted
is
highly
sensitive
properties
such
layer,
solutions
ranging
common
dry
rocks
an
unambiguously
base.
advocate
toward
better
cover
assess
or
nature
base,
possibly
reconcile
most
literature
on
topic.
Язык: Английский