The NASA-ESA plan is to return samples using three missions: a sample collection mission (Perseverance), a sample retrieval mission (Sample Retrieval Lander + Mars ascent vehicle + Sample Transfer arm + 2 Ingenuity class helicopters), and a return mission (Earth Return Orbiter).[1][2][3] The mission hopes to resolve the question of whether Mars once harbored life.
The Mars 2020 mission landed the Perseverance rover, which is storing samples to be returned to Earth later. After consideration, it was decided that given Perseverance's expected longevity, it will be the primary means of transporting samples to Sample Retrieval Lander (SRL).
The sample retrieval mission involves launching a sample return lander in 2028 with the Mars Ascent Vehicle and two Ingenuity class sample recovery helicopters, both of which will be collecting the samples with a tiny robotic arm as a backup for Perseverance. The rover and helicopters will transport the samples to the SRL lander. SRL's EAS-built sample transfer arm will be used to extract the samples and load them into the Sample Return Capsule in the Ascent Vehicle.[1] It is planned to land near the Octavia E. Butler Landing site in 2029.
MAV is a 3 m (9.8 ft) long, two-stage, solid-fueled rocket that will deliver the collected samples from the surface of Mars to the Earth Return Orbiter. Early in 2022, Lockheed Martin was awarded a contract to partner with NASA's Marshall Space Flight Center in developing the MAV.[5] It is planned to be catapulted into the air just before it ignites, at a rate of 16 feet (5 meters) per second, to remove the odds of wrong liftoff like slipping or tilting of SRL under rocket's shear weight and exhaust at liftoff. This Vertically Ejected Controlled Tip-off Release (VECTOR) system adds a slight rotation during launch, pitching the rocket up and away from the surface.[6] MAV would enter a 380 km orbit.[7] It will remain stowed inside a cylinder on the SRL and will have a thermal protective coating. The rocket's first stage (SRM-1) would be run by a single modified STAR-20 engine burning for 70 seconds, while the second stage (SRM-2) would have a single modified STAR-15G engine burning for another 25 seconds.[8] They would be separated by a coast phase, after which the sample container would be released in orbit. As of early 2022, the second stage is planned to be spin-stabilized to save weight in lieu of active guidance, while the Mars samples will result in an unknown payload mass distribution.[7]
MAV is scheduled to be launched in 2028 on board the SRL lander.[1]
ERO is an ESA-developed spacecraft.[9][10] It includes the NASA-built Capture and Containment and Return System to rendezvous with the samples delivered by MAV in low Mars orbit (LMO). ERO orbiter is planned to weigh ~6,000 kg (13,000 lb) and has solar arrays that have a wingspan of more than 40 m (130 ft) (these are some of the largest solar panels ever launched into space).
ERO is scheduled to launch on an Ariane 64 rocket[11] in 2027 and arrive at Mars in 2028,[1] using ion propulsion and a separate propulsion element to gradually reach the proper orbit and then rendezvous with the orbiting sample. The MAV's second stage will have a radio beacon that will give controllers the information they need to get the ESA Earth Return Orbiter close enough to the Orbiting Sample to see it through reflective light and capture it for return to earth. The orbiter will retrieve and seal the canisters in orbit and use a NASA-built robotic arm to place the sealed container into an Earth-entry capsule. It will raise its orbit, release the propulsion element, and return to Earth during the 2033 Mars-to-Earth transfer window.
The Capture/Containment and Return System (CCRS) would stow the sample in the EEV. EEV would return to Earth and land passively, without a parachute. The desert sand at the Utah Test and Training Range and shock absorbing materials in the vehicle were planned to protect the samples from impact forces.[12][13][10] EEV is scheduled to land on Earth in 2033.[14]
Planetary Decadal 2010
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