# NASA-ESA Mars Sample Return

The NASA-ESA Mars Sample Return is a proposed Flagship-class Mars sample return (MSR) mission to collect Martian rock and soil samples in 43 small, cylindrical, pencil-sized, titanium tubes and return them to Earth around 2033.
The NASA–ESA plan, approved in September 2022, 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). The mission hopes to resolve the question of whether Mars once harbored life.
Although the proposal is still in the design stage, the Perseverance rover is currently gathering samples on Mars and the components of the sample retrieval lander are in testing phase on Earth.
After a project review critical of its cost and complexity, NASA announced that the project was "paused" as of 13 November 2023. On 22 November 2023, NASA was reported to have cut back on the Mars sample-return mission due to a possible shortage of funds. In April 2024, in a NASA update via teleconference, the NASA Administrator emphasized continuing the commitment to retrieving the samples. However, under the then-current mission profile, the cost of $11 billion was infeasible, therefore NASA would turn to industry and the Jet Propulsion Laboratory to form a new, more fiscally feasible mission profile to retrieve the samples, with responses expected by fall 2024.

## History
### 2001 to 2004

In the summer of 2001, the Jet Propulsion Laboratory (JPL) requested mission concepts and proposals from industry-led teams (Boeing, Lockheed Martin, and TRW). The science requirements included at least 500 grams (18 oz) of samples, rover mobility to obtain samples at least 1 kilometre (0.62 mi) from the landing spot, and drilling to obtain one sample from a depth of 2 metres (6 ft 7 in). That following winter, JPL made similar requests of certain university aerospace engineering departments (MIT and the University of Michigan).
Also in 2001, a separate set of industry studies was done for the Mars ascent vehicle (MAV) due to the uniqueness and key role of the MAV for MSR. Figure 11 in this reference summarized the need for MAV flight testing at a high altitude over Earth, based on Lockheed Martin's analysis that the risk of mission failure is "extremely high" if launch vehicle components are only tested separately.
In 2003, JPL reported that the mission concepts from 2001 were too costly. A subsequent study yielded a more affordable plan that was accepted by two groups of scientists: a new MSR Science Steering Group, and the Mars Exploration Program Analysis Group (MEPAG). Instead of a rover and deep drilling, a scoop on the lander would dig 20 centimetres (7.9 in) deep and place multiple samples together into one container. After five years of technology development, the MAV would be flight-tested twice above Earth before the mission PDR (Preliminary Design Review) in 2009.
Based on the simplified mission plan, assuming a launch from Earth in 2013, two weeks on Mars, and a 2016 return, technology development was initiated to ensure that potential Mars microbes would not contaminate Earth, and also that the Mars samples would not be contaminated with Earth-origin biological materials. The sample container would be clean on the outside before departing from Mars, with installation onto the MAV inside an "Earth-clean MAV garage".
In 2004, JPL published an update on the 2003 plan. MSR would use the new large sky crane landing system in development for the Mars Science Laboratory rover (later named Curiosity). An MSR Technology Board was formed, and it was noted that the use of a rover might return to the MSR plan, in light of success with the Spirit and Opportunity rovers that arrived early in 2004. A 285-kilogram (628 lb) ascent rocket would carry 0.5-kilogram (1.1 lb) of samples inside a 5-kilogram (11 lb) payload, the Orbiting Sample (OS). The MAV would transmit enough telemetry to reconstruct events in case of failure on the way up to Mars orbit.

### 2005 to 2008

As of 2005, a rover had returned to the MSR plan, with a rock core drill, in light of results from the Mars Exploration Rover discoveries. Focused technology development would start before the end of 2005 for mission PDR in 2009, followed by launch from Earth in 2013. Related technologies in development included potential advances for Mars arrival (navigation and descent propulsion), and implementing pump-fed liquid launch vehicle technology on a scale small-enough for a MAV.
In late 2005, a peer-reviewed analysis showed that ascent trajectories to Mars orbit would differ depending on liquid versus solid propulsion, largely because small solid rocket motors burn faster, requiring a steeper ascent path to avoid excess atmospheric drag, while slower burning liquid propulsion might take advantage of more efficient paths to orbit.
Early in 2006, the Marshall Space Flight Center noted the possibility that a science rover would cache the samples on Mars, then subsequently a mini-rover would be sent along with the MAV on a sample return lander. Then, either the mini-rover or the science rover would deliver the samples to the lander for loading onto the MAV. A two-stage 250-kilogram (550 lb) solid propellant MAV would be gas ejected from a launch tube. It would carry a 5-kilogram (11 lb) payload -- a 16-centimetre (6.3 in) diameter spherical package containing the samples. The second stage would send telemetry, and its steering thrusters would use hydrazine fuel with additives. The authors expected the MAV to need multiple flight tests at a high altitude over Earth.
A peer-reviewed publication in 2007 described testing of autonomous sample capture for Mars orbit rendezvous. Free-floating tests were done on board a NASA aircraft using a parabolic "zero-g" flight path.
In 2007, Alan Stern, then NASA's Associate Administrator for Science, was strongly in favor of completing MSR sooner, and he asked JPL to include sample caching on the Mars Science Laboratory mission (later named Curiosity). A team at the Ames Research Center was designing a hockey puck-sized sample-caching device to be installed as an extra payload on MSL.
A review analysis in 2008 compared Mars ascent to lunar ascent, noting that the MAV would pose not only a technical challenge, but also a cultural one for the planetary science community: given that lunar ascent has been done using known technology, and that science missions typically rely on proven propulsion for course corrections and orbit insertion maneuvers, similar to what Earth satellites do routinely.

### 2009 to 2011

Early in 2009, the In-Space Propulsion Technology project office at the NASA Glenn Research Center (GRC) presented a ranking of six MAV options, concluding that a 285-kilogram (628 lb) two-stage solid rocket with continuous telemetry would be best for delivering a 5-kilogram (11 lb) sample package to Mars orbit. A single-stage pump-fed bipropellant MAV was noted to be less heavy, and was ranked second.
Later in 2009, the chief technologist of the Mars Exploration Directorate at JPL referred to a 2008 workshop on MSR technologies at the Lunar and Planetary Institute, and wrote that particularly difficult technology challenges included: the MAV, sample acquisition and handling, and back planetary protection. He then further commented that, "The MAV, in particular, stands out as the system with highest development risk, pointing to the need for an early start," leading to flight testing before preliminary design review (PDR) of the lander that would deliver the MAV.
In October 2009, NASA and ESA established the Mars Exploration Joint Initiative to proceed with the ExoMars program, whose ultimate aim is the return of samples from Mars in the 2020s. ExoMars's first mission was planned to launch in 2018, with unspecified missions to return samples in the 2020–2022 time frame. As reported to the NASA Advisory Council Science Committee (NAC-SC) early in 2010, MEPAG estimated that MSR "will cost $8-10B, and it is obvious that NASA and ESA can't fund this amount by themselves." The cancellation of the caching rover MAX-C in 2011, and later NASA withdrawal from ExoMars, due to budget limitations, ended the mission. The pull-out was described as "traumatic" for the science community.
In 2010–2011, the NASA In-Space Propulsion Technology (ISPT) program at the Glenn Research Center received proposals and funded industry partners for MAV design studies with contract options to begin technology development, while also considering propulsion needs for Earth return spacecraft. Inserting the spacecraft into Mars orbit, then returning to Earth, was noted to need a high total of velocity changes, leading to a conclusion that solar electric propulsion could reduce mission risk by improving mass margins, compared to the previously assumed use of chemical propulsion along with aerobraking at Mars. The ISPT team also studied scenarios for MAV flight testing over Earth, and recommended two flight tests prior to MSR mission PDR, considering the historical low probability of initial success for new launch vehicles.
The NASA–ESA potential mission schedule anticipated launches from Earth in 2018, 2022, and 2024 to send respectively; a sample caching rover, a sample return orbiter, and a sample retrieval lander for a 2027 Earth arrival, with MAV development starting in 2014 after two years of technology development identified by the MAV design studies. The ISPT program summarized a year of propulsion technology progress for improving Mars arrival, Mars ascent, and Earth return, stating that the first flight test of a MAV engineering model would need to occur in 2018 to meet the 2024 launch date for the sample retrieval lander.
The 2011, MAV industry studies were done by Lockheed-Martin teamed with ATK, Northrop-Grumman, and Firestar Technologies, to deliver a 5-kg (11-lb), 16-cm (6.3-inch) diameter sample sphere to Mars orbit. The Lockheed-Martin-ATK team focused on a solid propellant first stage with either solid or liquid propellant for the upper stage, estimated MAV mass in the range 250 to 300 kg (550 to 660 lb), and identified technologies for development to reduce mass. Northrop-Grumman (the former TRW) similarly estimated a mass below 300 kg, using pressure-fed liquid bipropellants for both stages, and had plans for further progress. Firestar Technologies described a single-stage MAV design having liquid fuel and oxidizer blended together in one main propellant tank.
In early 2011 the US National Research Council's Planetary Science Decadal Survey, which laid out mission planning priorities for the period 2013–2022, declared an MSR campaign its highest priority Flagship Mission for that period. In particular, it endorsed the proposed Mars Astrobiology Explorer-Cacher (MAX-C) mission in a "descoped" (less ambitious) form. This mission plan (cancelled in April 2011 for budget reasons) had been for NASA and ESA to each build a rover to send together in 2018.

### 2012 to 2013

In 2012, prospects for MSR were slowed further by a 38-percent cut in NASA's Mars program budget for fiscal year 2013, leading to controversy among scientists over whether Mars exploration could thrive on a series of small rover missions. A Mars Program Planning Group (MPPG) was convened as one response to budget cuts.
In mid-2012, eight weeks before Curiosity arrived on Mars, the Lunar and Planetary Institute hosted a NASA-sponsored three-day workshop to gather expertise and ideas from a wide range of professionals and students -- as input to help NASA reformulate the Mars Exploration Program, in response to the latest Planetary Decadal Survey that prioritized MSR, while also faced with recent deep budget cuts. 390 submissions were received, and the 185 people in attendance agreed that "credible steps toward MSR" could be done with reduced funding. The MAX-C rover (ultimately implemented as Mars 2020, Perseverance) was considered beyond financial reach at that time, so the summary report noted that progress toward MSR could include an orbiter mission to test autonomous rendezvous, or a Phoenix-class lander to demonstrate pinpoint landing while delivering a MAV as a technology demonstration. The workshop consisted largely of three breakout group discussions for Technology and Enabling Capabilities, Science and Mission Concepts, and Human Exploration and Precursors.
Wide-ranging discussions were documented by the Technology Panel, which suggested investments for improved drilling and "small is beautiful" rovers with an "emphasis on creative mass-lowering capabilities." The panel stated that MAV "functional technology is not new" but the Mars environment would pose challenges, and referred to MAV technologies as "a risk for most sample return scenarios of any cost range." MAV technology was addressed in numerous written submissions to the workshop, one of which described Mars ascent as "beyond proven technology," (velocity and acceleration in combination for small rockets) and a "huge challenge for the social system," referring to a "Catch-22" dilemma "in which there is no tolerance for new technology if sample return is on the near-term horizon, and no MAV funding if sample return is on the far horizon."
In September 2012, NASA announced its intention to further study MSR strategies as outlined by the MPPG – including a multiple-launch scenario, a single-launch scenario, and a multiple-rover scenario – for a mission beginning as early as 2018. A "fetch rover" would retrieve the sample caches and deliver them to a Mars ascent vehicle (MAV). In July 2018, NASA contracted Airbus to produce a "fetch rover" concept. As of late 2012, It was determined that the MAX-C rover concept to collect samples could be implemented for a launch in 2020 (Mars 2020), within available funding, using spare parts and mission plans developed for NASA's Curiosity Mars rover
In 2013, the NASA Ames Research Center proposed that a SpaceX Falcon Heavy could deliver two tons of useful payload to the Mars surface, including an Earth return spacecraft that would be launched from Mars by a one-ton single-stage MAV using liquid bipropellants fed by turbopumps. The successful landing of the Curiosity rover directly on its wheels (August 2012) motivated JPL to take a fresh look at carrying the MAV on the back of a rover. A fully guided 300-kg MAV (like Lockheed's 2011 two-stage solid) would avoid the need for a round-trip fetch rover. A smaller 150-kg MAV would permit one rover to also include sample collection while using MSL heritage to reduce mission cost and development time; placing most development risk on the MAV.
JPL later presented more details of the 150-kg solid propellant mini-MAV concept of 2012, in a summary of selected past efforts. The absence of telemetry data during the 1999 loss of the Mars Polar Lander had put an emphasis on "critical event communications," that was subsequently applied to MSR. Then after the MSL landing in 2012, requirements had been revisited with a goal to reduce MAV mass. Single fault tolerance and continuous telemetry data to Mars orbit were questioned. For the 500 grams (1.1 lb) of samples, a 3.6-kg (7.9 lb) payload was deemed possible instead of 5 kg (11 lb). The 2012 mini-MAV concept had single-string avionics, in addition to the spin-stabilized upper stage without telemetry.

### 2014 to 2017

In 2014–2015, JPL analyzed many options for Mars ascent including solid, hybrid, and liquid propellants, for payloads ranging from 6.5 kg to 25 kg. Four MAV concepts using solid propellant had two stages, while one or two stages were considered for hybrid and liquid propellants. Seven options were scored for ten attributes ("figures of merit"). A single-stage hybrid received the highest overall score, including the most points for reducing cost and, separately, for reducing complexity, with the fewest points for technology readiness. Second overall was a single-stage liquid bi-propellant MAV using electric pumps. A pressure fed bi-propellant design was third, with the most points for technology readiness. Solid propellant options had lower scores, partly due to receiving very few points for flexibility. JPL and NASA Langley Research Center cautioned that the high thrust and short burn times of solid rocket motors would result in early burnout at a low altitude with substantial atmosphere remaining to coast through at high Mach numbers, raising stability and control concerns. With concurrence from the Mars Program Director, a decision was made in January 2016 to focus limited technology development funds on advancing a hybrid propellant MAV (liquid oxidizer with solid fuel).
Starting in 2015, a new effort for planetary protection moved the backward planetary protection function from the surface of Mars to the sample Return Orbiter, to "break-the-chain" in flight. Concepts for brazing, bagging, and plasma sterilization were studied and tested, with a primary focus on brazing, as of 2016.

### 2018 to 2022

In April 2018, a letter of intent was signed by NASA and ESA that may provide a basis for a Mars sample-return mission. The agreement came out of the 2nd International Mars Sample Return Conference in Berlin, Germany. The conference program was archived along with 125 technical submissions that covered sample science (anticipated findings, site selection, collection, curation, analysis) and mission implementation (Mars arrival, rovers, rock drills, sample transfer robotics, Mars ascent, autonomous orbit rendezvous, interplanetary propulsion, Earth arrival, planetary protection). In one of many presentations, an international science team noted that collecting sedimentary rock samples would be required to search for ancient life. A joint NASA-ESA presentation described the baseline mission architecture, including sample collection by the Mars 2020 Rover derived from the MAX-C concept, a Sample Retrieval Lander, and an Earth Return Orbiter. An alternative proposal was to use a SpaceX Falcon Heavy to decrease mission cost while delivering more mass to Mars and returning more samples. Another submission to the Berlin conference noted that mission cost could be reduced by advancing MAV technology to enable a significantly smaller MAV for a given sample payload.
In July 2019 a mission architecture was proposed. In 2019, JPL authors summarized sample retrieval, including a sample fetch rover, options for fitting 20 or 30 sample tubes into a 12-kilogram (26 lb) payload on a 400-kilogram (880 lb) single-stage-to-orbit (SSTO) MAV that would use hybrid propellants, a liquid oxidizer with a solid wax fuel, which had been prioritized for propulsion technology development since 2016. Meanwhile, the Marshall Space Flight Center (MSFC) presented a comparison of solid and hybrid propulsion for the MAV. Later in 2019, MSFC and JPL had collaborated on designing a two-stage solid propellant MAV, and noted that an unguided spinning upper stage could reduce mass, but this approach was abandoned at the time due to the potential for orbital variations.
Early in 2020 JPL updated the overall mission plan for an orbiting sample package (the size of a basketball) containing 30 tubes, showing solid and hybrid MAV options in the range 400 to 500 kilograms (880 to 1,100 lb). Adding details, MSFC presented designs for both the solid and hybrid MAV designs, for a target mass of 400 kilograms (880 lb) at Mars liftoff to deliver 20 or 30 sample tubes in a 14-to-16-kilogram (31 to 35 lb) payload package. In April 2020, an updated version of the mission was presented. The decision to adopt a two-stage solid rocket MAV was followed by Design Analysis Cycle 0.0 in the spring of 2020, which refined the MAV to a 525-kilogram (1,157 lb) design having guidance for both stages, leading to reconsideration of an unguided spin-stabilized second stage to save mass.
In October 2020, the MSR Independent Review Board (IRB) released its report recommending overall that the MSR program proceed, then in November NASA responded to detailed IRB recommendations. The IRB noted that MSR would have eight first-time challenges including the first launch from another planet, autonomous orbital rendezvous, and robotic sample handling with sealing to "break-the-chain." The IRB cautioned that the MAV will be unlike any previous launch vehicle, and experience shows that the smaller a launch vehicle, the more likely it is to end up heavier than designed. Referring to the unguided upper stage of the MAV, the IRB stated the importance of telemetry for critical events, "to allow useful reconstruction of a fault during second stage flight." The IRB indicated that the most probable mission cost would be $3.8 to $4.4B. As reported to the NAC-SC in April 2021, the Planetary Science Advisory Committee (PAC) was "very concerned about the high cost" of MSR, and wanted to be sure that astrobiology considerations would be included in plans for returned sample laboratories.
Early in 2022 MSFC presented the guided-unguided MAV design for a 125-kilogram (276 lb) mass reduction, and documented remaining challenges including aerodynamic complexities during the first stage burn and coast to altitude, a desire to locate hydrazine steering thrusters farther from the center of mass, and stage separation without tip-off rotation. While stage separation and subsequent spin-up would be flight tested, the authors noted that it would be ideal to flight test an entire flight-like MAV, but there would be a large cost.
In April 2022, the United States National Academies released the Planetary Science Decadal Survey report for 2023-2032, a review of plans and priorities for the upcoming ten years - after many committee meetings starting in 2020, with consideration of over 500 independently submitted white papers, more than 100 regarding Mars, including comments on science and technology for sample return. The published document noted NASA's 2017 plan for a "focused and rapid" sample return campaign with essential participation from ESA, then recommended, "The highest scientific priority of NASA's robotic exploration efforts this decade should be completion of Mars Sample Return as soon as is practicably possible." Decadal white papers emphasized the importance of MSR for science, included a description of implementing MSR, and noted that the MAV has been underestimated despite needing flight performance beyond the state of the art for small rockets, needs a sustained development effort, and that technology development for a smaller MAV has the potential to reduce MSR mission cost. Decadal Survey committee meetings hosted numerous invited speakers, notably a presentation from the MSR IRB.
As of March 2022, separate landers were planned for the fetch rover and the MAV, because together they would be too large and heavy for a single lander. A cost-saving plan as of July was to send only one lander with the MAV, and rely on the Perseverance rover to pass sample tubes to the MAV in the absence of a fetch rover. Two new lightweight helicopters on the MAV lander would serve as a backup for moving the samples on Mars.

### 2023 to 2024

At the start of 2023 it was revealed that a "Mars Sample Fetch Helicopter" had been envisioned since at least 2021 by the team at AeroVironment that created Ingenuity to fly in the thin atmosphere of Mars. In a public budget meeting in March, NASA noted the high cost of MSR and had begun to assemble a second independent review board (MSR IRB-2) to assess the design, schedule and required funding. The IRB-2 began working in May 2023 and released its report in September 2023.
In January 2024, a related proposed NASA plan had been challenged due to budget and scheduling considerations, and a newer overhaul plan undertaken. The American Institute of Aeronautics and Astronautics contrasted the mission cost challenge with the science value of returned samples, noting that multiple in-situ science missions could be done for the cost of MSR, but that an electron microscope for example would be too large to send to Mars. A response in March described the high mission cost as related to the size of the MAV and its huge lander, offering that innovation could lead to a smaller MAV.
In April 2024, NASA formally responded to the IRB-2 report, with a report from the MIRT (MSR IRB Response Team) which noted the cost-saving value of a smaller MAV. On April 15, 2024, NASA Administrator Bill Nelson and Science Mission Director Nicola Fox announced the organization's response to the September 2023 independent review board's investigation, notably the finding that Mars Sample Return at its current design and cost, originally estimated at $7 billion with Earth re-entry by 2033, would now cost more than an unacceptable $11 billion and end in Earth re-entry no sooner than 2040. In response, Nelson and Fox stated that NASA would make requests to industry the next day to come up with alternatives that would likely utilize more proven mission architectures with longer heritages and comply with the board's recommendations, with responses preferred by fall 2024. They also said they would spend $310 million on the program for fiscal year 2024. On April 22, a public meeting was held to explain NASA's April 16 request for proposals to revisit alternative mission architectures.

### 2024 to present

In June 2024, following the agency’s decision to open the mission to industry proposals, seven firms were selected to move forward in a 90-day mission study.
In January 2025, NASA announced they would be pursuing two potential paths forward to land the MAV. The first option would use the sky crane method used for Curiosity and Perseverance, and the second would, "capitalize on using new commercial capabilities." Both options would use the ESA's Earth Return Orbiter to receive and ferry the samples.

## Sample collection

The Mars 2020 mission landed the Perseverance rover, which is storing samples to be returned to Earth later.

### Mars 2020 Perseverance rover

The Mars 2020 mission landed the Perseverance rover in Jezero crater in February 2021. It collected multiple samples and packed them into cylinders for later return. Jezero appears to be an ancient lakebed, suitable for ground sampling.
At the beginning of August 2021, Perseverance made its first attempt to collect a ground sample by drilling out a finger-size core of Martian rock. This attempt did not succeed. A drill hole was produced, as indicated by instrument readings, and documented by a photograph of the drill hole. However, the sample container turned out to be empty, indicating that the rock sampled was not robust enough to produce a solid core.
A second target rock, judged to have a better chance to yield sufficiently robust material, was sampled at the end of August and the beginning of September 2021. After abrading the rock, cleaning away dust by puffs of pressurized nitrogen, and inspecting the resulting rock surface, a hole was drilled on September 1. A rock sample appeared to be in the tube, but it was not immediately placed in a container. A new procedure of inspecting the tube optically was performed. On September 6, the process was completed, with the first sample placed in a container.
From December 21, 2022 Perseverance started a campaign to deposit 10 of its collected samples at the backup depot, Three Forks. This work was completed on January 28, 2023.

## List of samples cached
### Sample Tube Status

Sample Details :
| Sampling Attempt | Date | Tube No. | Seal No. | Ferrule Prefix | Ferrule No. | Contents | Sample Name and Image during Caching | Sample Depot Deposit Date, Spot and Image | Rock Name | Core Length | Estimated Martian Atmosphere Headspace Gas | Location | Notes |
| 1 | June 22, 2021 (Sol 120) | SN061 | SN147 | 10464848-7 | SN090 | Witness Tube (Empty) | WB-1 | | N/A | N/A | 2.2 x 10$^{−6}$ mol | North Séítah Unit | This was taken as a dry-run in preparation for later sampling attempts, and did not aim to sample a rock. During final pre-launch activities, this witness tube was activated (the inner seal was punctured to begin accumulation) and placed in the Bit Carousel. This tube will therefore have accumulated contaminants for the entire duration of exposure from a few months before launch through cruise and EDL until it was sealed on the surface of Mars. Given its long exposure, it is likely that the inner surfaces of WB1 will be saturated with organic contaminants, i.e., they will be in adsorption equilibrium with their immediate surroundings in the rover (and or the entire spacecraft prior to landing). WB1 is therefore expected to have higher concentrations of contaminants, and potentially different contaminants, than the sample tubes. |
| 2 | August 6, 2021 (Sol 164) | SN233 | SN025 | 10464848-7 | SN062 | Atmospheric Gas | Roubion (failed attempt of caching rock sample) | January 4, 2023 (Sol 666) at Three Forks Sample Spot "4" | Roubion 18°25′40″N 77°27′06″E﻿ / ﻿18.42767°N 77.45167°E﻿ / 18.42767; 77.45167 | N/A | 4.9x10$^{−6}$ mol | Polygon Valley, Cratered Floor Fractured Rough Unit | Attempted to sample a rock consisting of Basaltic lava flow or sandstone or Microgabbro but did not succeed, as they didn't reach the bit carousel, and the caching system stored and sealed an empty tube. However, in this process, it collected atmospheric samples. |
| 3 | September 6, 2021 (Sol 194) | SN266 | SN170 | 10464848-6 | SN099 | Basalt (or possibly basaltic sandstone) Rock Sample | Montdenier | January 10, 2023 (Sol 672) at Three Forks Sample Spot "6" | Rochette 18°25′51″N 77°26′40″E﻿ / ﻿18.43074°N 77.44433°E﻿ / 18.43074; 77.44433 | 5.98 cm (2.35 in) | 1.2x10$^{−6}$ mol | Arturby Ridge, Citadelle, South Séítah Unit | Successful sample. |
| 4 | September 8, 2021 (Sol 196) | SN267 | SN170 | 10464848-6 | SN074 | Basalt (or possibly basaltic sandstone) Rock Sample | Montagnac | | Rochette 18°25′51″N 77°26′40″E﻿ / ﻿18.43074°N 77.44433°E﻿ / 18.43074; 77.44433 | 6.14 cm (2.42 in) | 1.3x10$^{−6}$ mol | Arturby Ridge, Citadelle, South Séítah Unit | Sampled from same rock as previous sample. |
| 5 | November 15, 2021 (Sol 262) | SN246 | SN194 | 10464848-5 | SN107 | Olivine cumulate Rock Sample | Salette | | Brac 18°26′02″N 77°26′35″E﻿ / ﻿18.43398°N 77.44305°E﻿ / 18.43398; 77.44305 | 6.28 cm (2.47 in) | 1.1 x10$^{−6}$ mol | Brac Outcrop, South Séítah Unit | |
| 6 | November 24, 2021 (Sol 271) | SN284 | SN219 | 10464848-6 | SN189 | Olivine cumulate Rock Sample | Coulettes | January 6, 2023 (Sol 668) at Three Forks Sample Spot "5" | Brac 18°26′02″N 77°26′35″E﻿ / ﻿18.43398°N 77.44305°E﻿ / 18.43398; 77.44305 | 3.30 cm (1.30 in) | 2.5 x10$^{−6}$ mol | Brac Outcrop, South Séítah Unit | |
| 7 | December 22, 2021 (Sol 298) | SN206 | SN184 | 10464848-7 | SN064 | Olivine cumulate Rock Sample | Robine | | Issole 18°25′58″N 77°26′29″E﻿ / ﻿18.43264°N 77.44134°E﻿ / 18.43264; 77.44134 | 6.08 cm (2.39 in) | 1.0 x10$^{−6}$ mol | Issole, South Séítah Unit | |
| 8 | December 29, 2021 (Sol 306) | SN261 | SN053 | 10464848-6 | SN062 | Olivine cumulate Rock Sample | Pauls (Abandoned sample from this site due to Core Bit Dropoff.) | December 21, 2022 (Sol 652) at Three Forks Sample Spot "1" | Issole 18°25′58″N 77°26′29″E﻿ / ﻿18.43264°N 77.44134°E﻿ / 18.43264; 77.44134 | N/A | N/A | Issole, South Séítah Unit | Pebble-sized debris from the first sample fell into the bit carousel during transfer of the coring bit, which blocked the successful caching of the sample. It was decided to abandon this sample and do a second sampling attempt again. Subsequent tests and measures cleared remaining samples in tube and debris in caching system The tube was reused for second sample attempt, which was successful. It was the first sample tube to be deposited at a Sample Depot (in this case the depot is Three Forks). |
| 9 | January 31, 2022 (Sol 337) | SN261 | SN053 | 10464848-6 | SN062 | Olivine cumulate Rock Sample | Malay (During Caching) | December 21, 2022 (Sol 652) at Three Forks Sample Spot "1" | Issole 18°25′58″N 77°26′29″E﻿ / ﻿18.43264°N 77.44134°E﻿ / 18.43264; 77.44134 | 3.07 cm (1.21 in) | 2.7 x10$^{−6}$ mol | Issole, South Séítah Unit | Pebble-sized debris from the first sample fell into the bit carousel during transfer of the coring bit, which blocked the successful caching of the sample. It was decided to abandon this sample and do a second sampling attempt again. Subsequent tests and measures cleared remaining samples in tube and debris in caching system The tube was reused for second sample attempt, which was successful. It was the first sample tube to be deposited at a Sample Depot (in this case the depot is Three Forks). |
| 10 | March 7, 2022 (Sol 371) | SN262 | SN172 | 10464848-6 | SN129 | Basaltic andesite Rock Sample | Ha'ahóni (aka "Hahonih") | | Sid 18°27′09″N 77°26′38″E﻿ / ﻿18.45242°N 77.44386°E﻿ / 18.45242; 77.44386 | 6.50 cm (2.56 in) | 0.98 x10$^{−6}$mol | Ch'ał outcrop(100 m (330 ft) east of Octavia E. Butler Landing), Séítah Unit | |
| 11 | March 13, 2022 (Sol 377) | SN202 | SN168 | 10464848-4 | SN074 | Basaltic andesite Rock Sample | Atsá (aka "Atsah") | January 20, 2023 (Sol 682) at Three Forks Sample Spot "9" | Sid 18°27′09″N 77°26′38″E﻿ / ﻿18.45242°N 77.44386°E﻿ / 18.45242; 77.44386 | 6.00 cm (2.36 in) | 1.3 x10$^{−6}$ mol | Ch'ał outcrop(100 m (330 ft) east of Octavia E. Butler Landing), Séítah Unit | |
| 12 | July 7, 2022 (Sol 490) | SN186 | SN188 | 10464848-4 | SN101 | Clastic Sedimentary Rock Sample | Swift Run | | Skinner Ridge 18°24′22″N 77°27′32″E﻿ / ﻿18.40617°N 77.45893°E﻿ / 18.40617; 77.45893 | 6.69 cm (2.63 in) | 1.23 x 10$^{−6}$ mol | Skinner Ridge, Delta Front | First Deltaic and First sedimentary sample cached by Perseverance. |
| 13 | July 12, 2022 (Sol 495) | SN272 | SN192 | 10464848-6 | SN068 | Clastic Sedimentary Rock Sample | Skyland | January 18, 2023 (Sol 680) at Three Forks Sample Spot "8" | Skinner Ridge 18°24′22″N 77°27′32″E﻿ / ﻿18.40617°N 77.45893°E﻿ / 18.40617; 77.45893 | 5.85 cm (2.30 in) | 1.7 x 10$^{−6}$ mol | Skinner Ridge, Delta Front | |
| 14 | July 16, 2022 (Sol 499) | SN205 | SN119 | 10464848-6 | SN170 | Witness Tube (Empty) | WB2 | | N/A | N/A | 2.7 x 10$^{−6}$ mol | Hogwallow Flats, Delta Front | This may have been done to clean out any leftover debris during the previous sampling attempts. On sol 495, a string-like piece of foreign object debris (FOD) similar to materials released during EDL was observed in the workspace images. On sol 499 this object was no longer observed, presumably because it blew out of the scene. This observation suggests the possibility of FOD in tubes sealed in this general area. |
| 15 | July 27, 2022 (Sol 509) | SN172 | SN157 | 10464848-7 | SN099 | Fine grained, well-sorted sedimentary rock sample, sulphate-bearing coarse mudstone | Hazeltop | | Wildcat Ridge 18°24′21″N 77°27′31″E﻿ / ﻿18.40589°N 77.45863°E﻿ / 18.40589; 77.45863 | 5.97 cm (2.35 in) | 1.63 x 10$^{−6}$ mol | Wildcat Ridge, Delta Front | |
| 16 | August 3, 2022 (Sol 516) | SN259 | SN177 | 10464848-5 | SN110 | Fine grained, well-sorted sedimentary rock sample, sulphate-bearing coarse mudstone | Bearwallow | January 13, 2023 (Sol 675) at Three Forks Sample Spot "7" | Wildcat Ridge 18°24′21″N 77°27′31″E﻿ / ﻿18.40589°N 77.45863°E﻿ / 18.40589; 77.45863 | 6.24 cm (2.46 in) | 1.43 x 10$^{−6}$ mol | Wildcat Ridge, Delta Front | |
| 17 | October 2, 2022 (Sol 575) | SN264 | SN068 | 10464848-5 | SN085 | Fine grained, well-sorted sedimentary rock, olivine-bearing coarse mudstone | Shuyak | | Amalik outcrop 77°24′05″N 18°27′03″E﻿ / ﻿77.40144°N 18.45073°E﻿ / 77.40144; 18.45073 | 5.55 cm (2.19 in) | 1.73 x 10$^{−6}$ mol | Amalik outcrop, Delta Front | |
| 18 | October 6, 2022 (Sol 578) – November 16, 2022 (Sol 588) | SN184 | SN587 | 10464848-4 | SN030 | Fine grained, well-sorted sedimentary rock, olivine-bearing coarse mudstone | Mageik | December 23, 2022 (Sol 654) at Three Forks Sample Spot "2" | Amalik outcrop 77°24′05″N 18°27′03″E﻿ / ﻿77.40144°N 18.45073°E﻿ / 77.40144; 18.45073 | 7.36 cm (2.90 in) | 0.63 x 10$^{−6}$ mol | Amalik outcrop, Delta Front | The anomaly first appeared on Oct 5 after the successful coring of the mission's 14th sample, called "Mageik," when the seal assigned to cap the rock-core-filled sample tube did not release as expected from its dispenser. The process of sealing a sample happens in the rover's Sampling and Caching System. During sealing, a small robotic arm moves the rock-core-filled tube to one of seven dispensers and presses its open end against a waiting seal. On the 17 previous occasions when a sample tube had been sealed during the mission, the seal was pressed fully into the tube. That allowed the seal to be extracted from the dispenser and the arm to move the seal-tube combination to a different station where they are pressed together, creating a hermetic seal. However, when the sample handling system attempted to dispense a seal in the tube of the Mageik sample, the seal encountered too much resistance and did not come free. The sampling system automatically detected the lack of seal and stored the unsealed tube safely so the tube and sample hardware remain in a stable configuration. One of the possible causes of the seal's nondeployment may be that Martian dust adhered to a location on the tube's interior surface where the dust could impede successful coupling and extraction. To ensure a hermetic seal, the tolerances between tube and seal are, by necessity, extremely small: 0.00008 inches (0.002 mm). The rover's CacheCam captured images showing light deposits of dust on the tube's lip, but the camera's imaging capabilities along the tube's inner surface are quite limited. Sealing which was tried again and again was finally completed on November 16, 2022 (Sol 588) successfully. |
| 19 | October 14, 2022 (Sol 585) | SN188 | SN153 | 10464848-5 | SN073 | Witness Tube (Empty) | WB3 | January 28, 2023 (Sol 689) at Three Forks Sample Spot "10" | N/A | N/A | 2.31 x 10$^{−6}$ mol | Amalik outcrop, Delta Front | The witness tubes do not collect samples but are opened near the sampling location to "witness" the Martian environment. The witness tubes go through the motions of sample collection without collecting rock or soil samples and are sealed and cached like Martian samples. Witness tubes aim to ensure that any potential Earth contaminants are detected during sample collection. This is to provide the validity of the samples once returned to Earth for analysis. During the processing of the WTA, two faults occurred. On sol 584 there was a fault during the simulated coring which resulted in only 5 of the normally 7 spindle/percuss motions being performed, and no percuss-to-ingest motion was executed. While anomaly recovery was being undertaken, the tube remained in the corer and exposed to the Martian environment about 10 times longer than normal WTA/sample exposure time. A second fault occurred after the sealing of the tube on sol 586, and left the hermetically sealed WTA sitting in the sealing station at an elevated temperature (up to 40 °C) until sol 591. The witness tube was successfully sealed on October 14, 2022 (Sol 586) and placed into storage on October 19, 2022 (Sol 591). |
| 20 | November 24, 2022 (Sol 626) – November 29, 2022 (Sol 631) | SN242 | SN151 | 10464848-5 | SN113 | Fine grained, moderately-sorted sedimentary rock, sulphate-bearing coarse sandstone | Kukaklek | | Hidden Harbor 77°23′57″N 18°27′13″E﻿ / ﻿77.39911°N 18.45364°E﻿ / 77.39911; 18.45364 | 4.97 cm (1.96 in) | 1.78 x 10$^{−6}$ mol | Hidden Harbor, Delta Front | First Sample from an abrasion patch, abraded earlier on the rock. It was sampled on November 29, 2022 (Sol 631) |
| 21 | December 2, 2022 (Sol 634) | SN059 | SN098 | 10464848-5 | SN063 | Regolith Sand Sample, likely containing mixed sedimentary and igneous grains | Atmo Mountain | | Observation Mountain 77°24′04″N 18°27′05″E﻿ / ﻿77.40122°N 18.45131°E﻿ / 77.40122; 18.45131 | 5.30 cm (2.09 in) | 1.87 x 10$^{−6}$ mol | Observation Mountain, Delta Front | First Regolith Sample. |
| 22 | November 7, 2022 (Sol 639) | SN173 | SN191 | 10464848-6 | SN106 | Regolith Sand Sample, likely containing mixed sedimentary and igneous grains | Crosswind Lake | December 29, 2022 (Sol 660) at Three Forks Sample Spot "3" | Observation Mountain 77°24′04″N 18°27′05″E﻿ / ﻿77.40122°N 18.45131°E﻿ / 77.40122; 18.45131 | 5.30 cm (2.09 in) | 1.88 x 10$^{−6}$ mol | Observation Mountain, Delta Front | |
| 23 | March 30, 2023 (Sol 749) | SN214 | SN066 | 1064848-5 | SN150 | Sedimentary Rock Sample | Melyn | | Berea Outcrop 77°23′02″N 18°28′13″E﻿ / ﻿77.383946°N 18.470216°E﻿ / 77.383946; 18.470216 | 6.04 cm (2.38 in) | | Berea, Tenby, Upper Fan | First Sample taken after completion of sample depot and the first taken under the new mission campaign. |
| 24 | May 23, 2023 (Sol 801) | | SN094 | 10464848-3 | | Conglomerate Sedimentary Rock Sample | N/A (Abandoned sample from this site due to small sample collection.) | | Onahu outcrop 77°22′07″N 18°26′00″E﻿ / ﻿77.368526°N 18.433455°E﻿ / 77.368526; 18.433455 | 1.30 cm (0.51 in) (Non-Cached) | N/A | Onahu, Upper Fan | The first attempt yielded a sample that was unfortunately too small, and the second attempt was unsuccessful and caching would have resulted in another empty Roubion atmospheric sample tube. A conglomerate rock is of special interest to the Science Team because they are made up of many clasts of rocks. These distinct clasts become cemented together over time to form the conglomerate. Importantly, these clasts were likely transported to Jezero crater from much farther away. Analyzing the distinct clasts and cements captured in a sample of the conglomerate would give insights into where these materials were sourced, how far they traveled, and what the martian environment was like, both when the clasts first formed and when the conglomerate rock formed. |
| 25 | June 4, 2023 (Sol 813) | | SN094 | 10464848-3 | | Conglomerate Sedimentary Rock Sample | N/A (Abandoned after failed attempt of collecting rock sample) | | Onahu outcrop 77°22′07″N 18°26′00″E﻿ / ﻿77.368526°N 18.433455°E﻿ / 77.368526; 18.433455 | N/A | N/A | Onahu, Upper Fan | The first attempt yielded a sample that was unfortunately too small, and the second attempt was unsuccessful and caching would have resulted in another empty Roubion atmospheric sample tube. A conglomerate rock is of special interest to the Science Team because they are made up of many clasts of rocks. These distinct clasts become cemented together over time to form the conglomerate. Importantly, these clasts were likely transported to Jezero crater from much farther away. Analyzing the distinct clasts and cements captured in a sample of the conglomerate would give insights into where these materials were sourced, how far they traveled, and what the martian environment was like, both when the clasts first formed and when the conglomerate rock formed. |
| 26 | June 23, 2023 (Sol 832) | | SN094 | 10464848-3 | | Conglomerate Sedimentary Rock Sample | Otis Peak | | Emerald Lake 77°22′05″N 18°28′59″E﻿ / ﻿77.368179°N 18.482989°E﻿ / 77.368179; 18.482989 | 5.77 cm (2.27 in) | | Emerald Lake, Upper Fan | The first attempt yielded a sample that was unfortunately too small, and the second attempt was unsuccessful and caching would have resulted in another empty Roubion atmospheric sample tube. A conglomerate rock is of special interest to the Science Team because they are made up of many clasts of rocks. These distinct clasts become cemented together over time to form the conglomerate. Importantly, these clasts were likely transported to Jezero crater from much farther away. Analyzing the distinct clasts and cements captured in a sample of the conglomerate would give insights into where these materials were sourced, how far they traveled, and what the martian environment was like, both when the clasts first formed and when the conglomerate rock formed. |
| 27 | September 15, 2023 (Sol 913) | SN258 | SN451 | 10464848-4 | SN196 | Conglomerate Sedimentary Rock Sample | Pilot Mountain | | Dream Lake | 6.00 cm (2.36 in) | | Dream Lake, Upper Fan | |
| 28 | September 23, 2023 (Sol 921) | SN178 | SN024 | 10464848-6 | SN113 | Sedimentary Rock Sample | Pelican Point | | Hans Amundsen Memorial Workspace | 6.10 cm (2.40 in) | | Hans Amundsen Memorial Workspace, Margin Unit | |
| 29 | October 21, 2023 (Sol 948) | SN263 | SN018 | 10464848-6 | SN089 | Sedimentary Rock Sample | Lefroy Bay | | Turquoise Bay | 4.70 cm (1.85 in) | | Turquoise Bay, Margin Unit | |
| 30 | March 11, 2024 (Sol 1086) | SN174 | SN214 | 10464848-6 | SN026 | Silica-cemented Carbonate | Comet Geyser | | Bunsen Peak | 5.78 cm (2.28 in) | | Bunsen Peak, Margin Unit | |
| 31 | July 21, 2024 (Sol 1215) | | | | | Sedimentary | Cheyava Falls | | Cheyava Falls | 6.2 cm (2.4 in) | | Cheyava Falls, Neretva Vallis | |
| Sources: ||||||||||||||

### Type Of Cached Samples

* Witness (3) (10.71%)
* Atmospheric (1) (3.57%)
* Igneous (8) (28.57%)
* Sedimentary (13) (46.43%)
* Regolith (2) (7.14%)
* Silica-cemented Carbonate (1) (3.57%)

### Sample Depot at Three Forks
## Three Forks Sample Depot

After nearly a Martian year of NASA's Perseverance Mars rover's science and sample caching operations for MSR campaign, the rover is currently tasked to deposit ten samples that it has cached from beginning at Three Forks Sample Depot as NASA aims to eventually return them to Earth starting from December 19, 2022. This depot will serve as a backup spot, in case Perseverance cannot deliver its samples. Perseverance is depositing the samples at a relatively flat terrain known as Three Forks so that NASA and ESA could recover them in its successive missions in the MSR campaign. It is even selected as the backup landing spot for the Sample Retrieval Lander. It is a relatively benign place. It is as flat and smooth as a table top.
Perseverance's complex Sampling and Caching System takes almost an hour to retrieve the metal tube from inside the rover's belly, view it one last time with its internal Cachecam, and drop the sample ~0.89 m (2 ft 11 in) onto a carefully selected patch of Martian surface.
The tubes will not be piled up at a single spot. Instead, each tube-drop location will have an "area of operation" ~5.5 m (18 ft) in diameter. To that end, the tubes will be deposited on the surface in an intricate zigzag pattern of 10 spots for 10 tubes, with each sample ~5 m (16 ft) to ~15 m (49 ft) apart from one another near the proposed Sample retrieval lander's landing site. There are various reasons for this plan, most significantly the design of the sample recovery helicopters. They are designed to interact with only one tube at a time. Alongside, they will perform takeoffs and landings, and driving in that spot. To ensure a helicopter could retrieve samples without any problem, the plan is to be executed properly and would span over more than two months.
Before and after Perseverance drops each tube, mission controllers will review a multitude of images from the rover's SHERLOC WATSON camera. Images by the SHERLOC WATSON camera are also used to check for surety that the tube had not rolled into the path of the rover's wheels. They also look to ensure the tube had not landed in such a way that it was standing on its end (each tube has a flat end piece called a "glove" to make it easier to be picked up by future missions). That occurred less than 5% of the time during testing with Perseverance's Earthly twin OPTIMISM in JPL's Mars Yard. In case it does happen on Mars, the mission has written a series of commands for Perseverance to carefully knock the tube over with part of the turret at the end of its robotic arm.
These SHERLOC WATSON camera images will also give the Mars Sample Return team the precise data necessary to locate the tubes in the event of the samples becoming covered by dust or sand before they are collected. Mars does get windy, but not like on Earth, as the atmosphere on Mars is 100 times less dense than that of Earth's atmosphere, so winds on Mars can pick up speed (the fastest are Dust devils), but they don't pick up a lot of dust particles. Martian wind can certainly lift fine dust and leave it on surfaces, but even if significant dust is accumulated these images the depositing pattern will help to recover them back. A lucky encounter with a dust devil could remove dust over the samples as in case with the solar panels of the Spirit and Opportunity rovers.
Once the task of depositing the 10 samples is completed, Perseverance will carry on with its mission, traversing to the crater floor and scaling Delta's summit. The rover traverse along the edge of the crater and caching more tubes while following the plan of taking single sample at one rock. Until now, several pairs of samples were taken and one sample from each pair will be placed at the depot and the other pair will stay on board the rover.

## Sample retrieval

The Mars Sample Return mission earlier in its design process consisted of the ESA Sample Fetch Rover and its associated second lander, alongside the Mars ascent vehicle and its lander that will take the samples to it, from where the samples will be launched back to Earth. But after consideration and cost overruns, it was decided that given Perseverance's expected longevity, the extant rover will be the primary means of transporting samples to the Sample Retrieval Lander (SRL).

### Sample Retrieval Lander

The sample retrieval mission involves launching a 5-solar array sample return lander in 2028 with the Mars Ascent Vehicle and two sample recovery helicopters as a backup for Perseverance. The SRL lander is about the size of an average two-car garage weighing ~3,375 kg (7,441 lb); tentatively planned to be 7.7 m (25 ft) wide and 2.1 m (6.9 ft) high when fully deployed. The payload mass of the lander is double that of the Perseverance rover, that is, ~563 kg (1,241 lb). The lander needs to be close to the Perseverance rover to facilitate the transfer of Mars samples. It must land within 60 m (200 ft) of its target site – much closer than previous Mars rovers and landers. Thus, it will have a secondary battery to power the lander to land on Mars. The lander would take advantage of an enhanced version of NASA's successful Terrain Relative Navigation that helped land Perseverance safely. The new Enhanced Lander Vision System would, among other improvements, add a second camera, an altimeter, and better capabilities to use propulsion for precision landing. It is planned to land near at Three Forks in 2029.
The Mars 2020 rover and helicopters will transport the samples to the SRL lander. SRL's ESA-built ~2.40 m (7.9 ft) long, Sample Transfer Arm will be used to extract the samples and load them into the Sample Return Capsule in the Ascent Vehicle.

### Mars Sample Recovery Helicopters

The MSR campaign includes Ingenuity-class helicopters, both of which will collect the samples with the help of a tiny robotic arm and move them to the SRL, in case the Perseverance rover runs into problems.

### Mars Ascent Vehicle (MAV)

Mars Ascent Vehicle (MAV) is a 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 and engines from Northrop Grumman. It is planned to be catapulted upward as high as 4.5 m (15 ft) above the lander – or 6.5 m (21 ft) above the Martian surface, into the air just before it ignites, at a rate of 5 m (16 ft) per second, to remove the odds of liftoff issues such as slipping or tilting the SRL with the rocket's sheer weight and exhaust at liftoff. The front would be tossed a bit harder than the back, causing the rocket to point upward, toward the Martian sky. Thus, the Vertically Ejected Controlled Tip-off Release (VECTOR) system adds a slight rotation during launch, pitching the rocket up and away from the surface. MAV would enter a 380-kilometre (240 mi) orbit. 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 burn for 75 seconds. The SRM1 engine can gimbal, but most gimballing solid rocket motor nozzles are designed in a way that can't handle the extreme cold MAV will experience, so the Northrop Grumman team had to come up with something that could: a state-of-the-art trapped ball nozzle featuring a supersonic split line. After SRM1 burnout, the MAV will remain in a coast period for approximately 400 seconds. During this time, the MPA aerodynamic fairing and entire first stage will separate from the vehicle. After stage separation, the second stage will initiate a spin up via side mounted small scale RCS thrusters. The entire second stage will be unguided and spin-stabilized at a rate of approximately 175 RPM. Having achieved the target spin rate, the second stage (SRM-2) will ignite and burn for approximately 18–20 seconds, raising the periapsis and circularizing the orbit. 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. Spin stabilization allows the rocket to be lighter, so it won't have to carry active control all the way to orbit. Following SRM2 burnout, the second stage will coast for up to 10 minutes while residual thrust from the SRM2 occurs. Side-mounted small de-spin motors will then fire, reducing the spin rate to less than 40 RPM. Once the target orbit has been achieved, the MAV will command the MPA to eject the Orbiting Sample Container (OS). The spent second stage of the MAV will remain in orbit, broadcasting a hosted radio beacon signal for up to 25 days. This will aid in the capture of the OS by the ERO.
MAV is scheduled to be launched in 2028 onboard the SRL lander.

## Sample return
### Earth Return Orbiter (ERO)

ERO is an ESA-developed spacecraft. It includes the NASA-built Capture and Containment and Return System (CCRS) and Electra UHF Communications Package. It will rendezvous with the samples delivered by MAV in low Mars orbit (LMO). The ERO orbiter is planned to weigh ~7,000 kg (15,000 lb) (largest Mars Orbiter) and have solar arrays resulting in a wingspan of more than 38 m (125 ft). These solar panels are some of the largest ever launched into space.
ERO is scheduled to launch on an Ariane 6 rocket in 2027 and arrive at Mars in 2029, using ion propulsion and a separate chemical propulsion element to gradually reach the proper orbit of 325 km (202 mi) and then rendezvous with the orbiting sample. The MAV's second stage's radio beacon 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. To do this, the ERO would use high-performance cameras to detect the Orbiting Sample at over 1,000 km (620 mi) distance. Once "locked on" the ERO would track it continuously using cameras and LiDARs throughout the rendezvous phase. Once aligned with the sample container, the Capture, Containment, and Return System would power on, open its capture lid, and turn on its capture sensors. ESA's orbiter would then push itself toward the sample container at about 1 to 2 inches (2.5 to 5 centimeters) per second to overtake and "swallow" it. After detecting that the sample container is safely inside, the Capture, Containment, and Return System would quickly close its lid. Thus, 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. The 600 kg (1,300 lb) CCRS would be responsible for thoroughly sterilizing the exterior of the Orbiting Sample and double sealing it inside the EES, creating a secondary containment barrier to keep the samples safely isolated and intact for maximum scientific return. It will raise its orbit, jettison the propulsion element (including ~500 kg (1,100 lb) of CCRS hardware, which is of no use after sterilizing samples), and return to Earth during the 2033 Mars-to-Earth transfer window.
The ERO will measure the total radiation dose received throughout the entire flight. Results will help monitor the health of the spacecraft and provide important information on how to protect human explorers in future trips to Mars.

### Earth Entry Vehicle (EEV)

The Capture/Containment and Return System (CCRS) would stow the sample in the EEV. The EEV would return to Earth and land passively, without a parachute. About a week before arrival at Earth, and only after successfully completing a full system safety check-out, the ERO spacecraft would be configured to perform the Earth return phase. When the orbiter is three days away from Earth, the EEV will be released from the main spacecraft and fly a precision entry trajectory to a predetermined landing site. Shortly after separation, the orbiter itself would perform a series of maneuvers to enter orbit around the Sun, never to return to Earth. The desert sand at the Utah Test and Training Range and shock absorbing materials in the vehicle are planned to protect the samples from impact forces. The EEV is scheduled to land on Earth in 2033.

## Gallery

* Potential sample-return landing site (14 April 2022)