NASA
reveals the payloads for the first commercial Moon cargo deliveries
NASA has finalized the payloads for its first cargo deliveries scheduled to be
carried by commercial lunar landers, vehicles created by companies the agency
selected to take part in its Commercial Lunar Payload Services (CLPS) program.
In total, there are 16 payloads, which consist of a number of different science
experiments and technology experiments, that will be carried by landers built
by Astrobotic and Intuitive Machines. Both of these landers are scheduled to
launch next year, carrying their cargo to the Moon's surface and helping
prepare the way for NASA's mission to return humans to the Moon by 2024.
Astrobotic's Peregrine is set to launch aboard a rocket provided by the United
Launch Alliance (ULA), while Intuitive Machines' Nova-C lander will make its
own lunar trip aboard a SpaceX Falcon 9 rocket. Both landers will carry two of
the payloads on the list, including a Laser Retro-Reflector Array (LRA) that is
basically a mirror-based precision location device for situating the lander
itself; and a Navigation Doppler Lidar for Precise Velocity and Range Sensing
(NDL) -- a laser-based sensor that can provide precision navigation during
descent and touchdown. Both of these payloads are being developed by NASA to
ensure safe, controlled and specifically targeted landing of spacecraft on the
Moon's surface, and their use here is crucial in building robust lunar landing
systems to support Artemis through the return of human astronauts to the Moon
and beyond.
Besides those two payloads, everything else on either lander is unique to one
vehicle or the other. Astrobotic is carrying more, but its Peregrine lander can
hold more cargo -- its payload capacity tops out at around 585 lbs, whereas the
Nova-C can carry a maximum of 220 lbs. The full list of what each lander will
have on board is available below, as detailed by NASA.
Overall, NASA has 14 contractors that could potentially provide lunar payload
delivery services through its CLPS program. That basically amounts to a list of
approved vendors, who then bid on whatever contracts the agency has available
for this specific need. Other companies on the CLPS list include Blue Origin,
Lockheed Martin, SpaceX and more. Starting with these two landers next year,
NASA hopes to fly around two missions per year each year through the CLPS
program.
Astrobotic Payloads
Surface Exosphere Alterations by Landers (SEAL): SEAL will investigate the
chemical response of lunar regolith to the thermal, physical and chemical
disturbances generated during a landing, and evaluate contaminants injected
into the regolith by the landing itself. It will give scientists insight into
the how a spacecraft landing might affect the composition of samples collected
nearby. It is being developed at NASA Goddard.
Photovoltaic Investigation on Lunar Surface (PILS): PILS is a technology
demonstration that is based on an International Space Station test platform for
validating solar cells that convert light to electricity. It will demonstrate
advanced photovoltaic high-voltage use for lunar surface solar arrays useful
for longer mission durations. It is being developed at Glenn Research Center in
Cleveland.
Linear Energy Transfer Spectrometer (LETS): The LETS radiation sensor will
collect information about the lunar radiation environment and relies on
flight-proven hardware that flew in space on the Orion spacecraft's inaugural
uncrewed flight in 2014. It is being developed at NASA Johnson.
Near-Infrared Volatile Spectrometer System (NIRVSS): NIRVSS will measure
surface and subsurface hydration, carbon dioxide and methane - all resources
that could potentially be mined from the Moon -- while also mapping surface
temperature and changes at the landing site. It is being developed at Ames
Research Center in Silicon Valley, California.
Mass Spectrometer Observing Lunar Operations (MSolo): MSolo will identify
low-molecular weight volatiles. It can be installed to either measure the lunar
exosphere or the spacecraft outgassing and contamination. Data gathered from
MSolo will help determine the composition and concentration of potentially
accessible resources. It is being developed at Kennedy Space Center in Florida.
PROSPECT Ion-Trap Mass Spectrometer (PITMS) for Lunar Surface Volatiles: PITMS
will characterize the lunar exosphere after descent and landing and throughout
the lunar day to understand the release and movement of volatiles. It was
previously developed for ESA's (European Space Agency) Rosetta mission and is being
modified for this mission by NASA Goddard and ESA.
Neutron Spectrometer System (NSS): NSS will search for indications of water-ice
near the lunar surface by measuring how much hydrogen-bearing materials are at
the landing site as well as determine the overall bulk composition of the
regolith there. NSS is being developed at NASA Ames.
Neutron Measurements at the Lunar Surface (NMLS): NMLS will use a neutron
spectrometer to determine the amount of neutron radiation at the Moon's
surface, and also observe and detect the presence of water or other rare
elements. The data will help inform scientists' understanding of the radiation
environment on the Moon. It's based on an instrument that currently operates on
the space station and is being developed at Marshall Space Flight Center in
Huntsville, Alabama.
Fluxgate Magnetometer (MAG): MAG will characterize certain magnetic fields to
improve understanding of energy and particle pathways at the lunar surface.
NASA Goddard is the lead development center for the MAG payload.
Intuitive Machines Payloads
Lunar Node 1 Navigation Demonstrator (LN-1): LN-1 is a CubeSat-sized experiment
that will demonstrate autonomous navigation to support future surface and
orbital operations. It has flown on the space station and is being developed at
NASA Marshall.
Stereo Cameras for Lunar Plume-Surface Studies (SCALPSS): SCALPSS will capture
video and still image data of the lander's plume as the plume starts to impact
the lunar surface until after engine shut off, which is critical for future
lunar and Mars vehicle designs. It is being developed at NASA Langley, and also
leverages camera technology used on the Mars 2020 rover.
Low-frequency Radio Observations for the Near Side Lunar Surface (ROLSES):
ROLSES will use a low-frequency radio receiver system to determine
photoelectron sheath density and scale height. These measurements will aide
future exploration missions by demonstrating if there will be an effect on the
antenna response or larger lunar radio observatories with antennas on the lunar
surface. In addition, the ROLSES measurements will confirm how well a lunar
surface-based radio observatory could observe and image solar radio bursts. It
is being developed at NASA Goddard.
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