Mission type | Astrobiology |
---|---|
Operator | NASA |
Website | jpl.nasa.gov |
Mission duration | ≤ 22 days on the surface [1] |
Spacecraft properties | |
Launch mass | 16.6 metric tons [1] |
Power | 50 kWh (from batteries only) [1] |
Start of mission | |
Launch date | 2025–2030 (proposed) [2] |
Rocket | Space Launch System or a commercial rocket |
Flyby of Earth | |
Closest approach | 2027–2032 |
Jupiter orbiter | |
Orbital insertion | 2030–2035 |
Europa lander | |
Landing date | 2032–2037 |
Large Strategic Science Missions Planetary Science Division |
The Europa Lander is an astrobiology mission concept by NASA to send a lander to Europa,an icy moon of Jupiter. [3] [4] If funded and developed as a large strategic science mission,it would be launched in 2027 to complement the studies by the Europa Clipper orbiter mission and perform analyses on site. [5]
The objectives of the mission are to search for biosignatures at the subsurface ≈10 cm,to characterize the composition of non-ice near-subsurface material,and determine the proximity of liquid water and recently erupted material near the lander's location.
NASA had previously evaluated a Europa Lander concept in 2005 with the Europa Lander Mission concept. [6] Also,a lander was evaluated in 2012. [7] There was continued support for Europa missions,including in 2014,when the U.S. Congress House Appropriations Committee announced a bipartisan bill that included US$80 million in funding to continue the Europa mission concept studies. [8] [9]
The United States Congress issued a congressional directive on a Europa Lander,and NASA initiated a study in 2016,assessing and evaluating the concept. [3] The mission concept is being supported by the Ocean Worlds Exploration Program. [10] NASA's Planetary Science Division delivered its report in early February 2017. [3] This was a six-month-long study by a Science Definition Team. [11] [12] The study assesses the science value and engineering design of a potential Europa lander mission. [12]
NASA's 2021 fiscal year budget in Congress's Omnibus Spending Bill did not include any language mandating or funding the Europa Lander as previous bills,making the mission's future uncertain. [13]
The Europa Lander was considered by the Planetary Science Decadal Report of 2023─2032 but rejected in favor of the Uranus Orbiter and Probe and Enceladus Orbilander. [14]
The primary mission goal is detection of organic indicators of past or present life,called biosignatures. [15] [3] [16] The lander was described as a logical follow-up to the Galileo orbiter and probe mission in the 1990s,for which a major result was the discovery of a large sub-surface ocean that may offer habitable aquatic conditions. [11]
On Earth,life can be found in essentially all locations where water is present. It follows that Europa is an excellent candidate in the search for life elsewhere in the Solar System. [17] This subsurface water may not only be warmed by geological activity,but likely also enriched with dissolved minerals and organic compounds. [18]
Various ecosystems exist on Earth without any access to sunlight relying instead on hydrothermal vents or other sources of chemicals suitable to energy production by extremophiles [19] (see chemosynthesis). Measurements to date indicate that Europa has an ocean approximately twice the volume of Earth's oceans. This water layer below the ice may be in contact with the moon's interior allowing ready access to hydrothermal energy and chemistry. [3] A surface mission can take advantage of the relatively young,active surface of Europa as this activity may allow deep subsurface materials to regularly relocate to the surface. [20]
In 18 July 2017,the House Space Subcommittee held hearings on the Europa Clipper as a scheduled large strategic science mission and to discuss this lander as a possible follow up. [21] The president's 2018 and 2019 federal budget proposals do not fund the Europa Lander,but they did assign US$195 million [22] for concept studies [23] [24] and research on the required science instruments. [25] The 2022 omnibus spending bill allocates $14.2 million to Icy Satellites Surface Technology for a future Ocean Worlds lander mission (NASA had requested $5 million for the Europa Lander). [26]
The lander mission would have three main science objectives: [27]
The key phases of the flight are:launch,cruise,de-orbit,descent and landing. [28] The spacecraft would consist of several modules that would be discarded at different phases of its deorbiting and landing sequence. The complete stack would be propelled by the Carrier Stage,that also features the solar panels. [1] After orbit injection around Jupiter,the spacecraft would spend about two years adjusting its orbit and velocity before attempting to land on Europa. [1]
In preparation to its landing,the Carrier Stage would be discarded,leaving the spacecraft stack in a configuration called Deorbit Vehicle (DOV) that would decelerate and initiate the descent. The engine module for this phase,called Deorbit Stage (DOS) would be discarded after the burn,leaving what is called the Powered Descent Vehicle (PDV) –which comprises the lander and the sky crane system. The sky crane system would lower the lander with a tether to a soft landing with a 100 m (330 ft) accuracy. [1]
The lander would feature a robotic arm with 5 degrees of freedom,that would enable it to dig out several shallow sub-surface samples at a maximum depth of 10 cm (3.9 in) and deliver them to its onboard laboratory. [1]
Once landed,the lander would operate for up to 22 days by using chemical battery power,rather than a radioisotope thermoelectric generator (RTG) or solar power. [1] [12] [24] The 2019 concept proposes four batteries,which would provide three times the needed energy for safety margin during its ≈22-day surface operations. [1] The baseline is 7 days to complete its surface mission,the additional 15 days are for contingencies. [1]
Regardless of the power source,one of the limiting factors for the lifetime of the mission would be enduring intense radiation;the surface of Europa is estimated to experience 540 rem per day,whereas a typical Earth surface dose is about 0.14 rem/year. [29] It is estimated that the probe would receive a total ionizing dose of 2.3 Mrad over the 30 day mission. [1] Radiation damaged the electronics of the Galileo orbiter during its mission. [30]
The launcher would be the Space Launch System (SLS),with a suggested launch between 2025-2030. [1] [31] The SLS is proposed[ needs update ] given the spacecraft's mass of 16.6 metric tons,including the solid propellant to place the spacecraft into orbit around Jupiter,and the sky crane landing system. [32] One calculated trajectory would see a launch aboard SLS in 2025,Earth gravity assist in 2027,and Jupiter/Europa arrival in 2030. [12] It would spend some time orbiting around Jupiter over the next year to maneuver for its landing on Europa. [12] The landing would be performed two years after orbit insertion around Jupiter. [1]
At Europa,it would have to land on the surface,matching its velocity,but with essentially no atmosphere there is no "entry",it is just a descent and landing. [28] The Planetary Society noted that NASA called this DDL — de-orbit,descent,and landing. [28] In 1995,astronomers using the Hubble Space Telescope discovered that Europa has a very tenuous exosphere composed of oxygen. [33] Compared to Earth,its atmosphere is thin to the extreme,with pressure at the surface predicted to be 0.1 μPa,or 10−12 times that of the Earth. [34]
The lander would communicate directly to Earth,but the Europa Clipper ,if still operational,could function as an additional communications relay for the lander. [28] To ensure communication,there is a suggestion to include a telecomm orbiter with the lander mission. [35]
A study published in October 2018 suggests that most of Europa's surface may be covered with closely spaced ice spikes,called penitents,as tall as 15 meters (50 ft). [36] [37] Although the imaging available from the Galileo orbiter does not have the resolution needed to confirm this,radar and thermal data are consistent with this interpretation. [37] This supports the need to first perform high-definition reconnaissance with the ESA's Jupiter Icy Moons Explorer (JUICE) and Europa Clipper,launching in 2023 and 2024 respectively,before planning a lander mission. [37] [38]
The mission concept would require funding and further development to be launched. One of the key requirements is to operate in the radiation environment at the moon's surface. [11] [1] The radiation environment at Europa is extreme,so the lander may need as much additional protection as the Juno Radiation Vault in the Juno Jupiter orbiter. [39] The vault helped reduce radiation exposure to vulnerable systems,especially electronics on the orbiter.
NASA announced in May 2017 to the scientific community to think on possible Europa Lander instruments. [40] The concept study reports were made available in June 2019. [41]
NASA selected 14 potential instruments for maturation under Instrument Concepts for Europa Exploration 2 (ICEE-2) awarding approximately US$2 million each for two years. [25] The ICEE-2 project would allow the maturation of novel instrument approaches to meet the science goals and objectives of the mission.
Instrument | Principal investigator |
---|---|
C-LIFE:Cold-Lightweight Imagers for Europa | Shane Bryne,University of Arizona |
ELSSIE:Europa Lander Stereo Spectral Imaging Experiment | Scott L. Murchie,Johns Hopkins University Applied Physics Laboratory |
CORALS:Characterization of Ocean Residues and Life Signatures | Ricardo D. Arevalo,University of Maryland |
MASPEX-ORCA:MAss Spectrometer for Planetary EXploration–ORganic Composition Analyzer | Christopher R. Glein,Southwest Research Institute |
MOAB:Microfluidic Organic Analyzer for Biosignatures | Richard A. Mathies,University of California Berkeley |
EMILI:Europan Molecular Indicators of Life Investigation [42] | W. B. Brinckerhoff,Goddard Space Flight Center |
CIRS:Compact Integrated Raman Spectrometer | James L. Lambert,Jet Propulsion Laboratory |
ELM:Europa Luminescence Microscope | Richard Quinn,Ames Research Center |
SIIOS:Seismometer to Investigate Ice and Ocean Structure [43] | Samuel H. Bailey,University of Arizona |
ESP:Europa Seismic Package | Mark P. Panning,Jet Propulsion Laboratory |
MICA:Microfluidic Icy-World Chemistry Analyzer | Antonio J. Ricco,Ames Research Center |
MAGNET:Radiation Tolerant Magnetometer | Mark B. Moldwin,University of Michigan,Ann Arbor |
EMS:Europa Magnetotelluric Sounder | Robert E. Grimm,Southwest Research Institute |
CADMES:Collaborative Acceptance and Distribution for Measuring Europan Samples System | Charles A. Malespin,Goddard Space Flight Center |
Planetary protection guidelines require that inadvertent contamination of a Europan ocean by terrestrial organisms must be avoided,to a probability level of less than 1 in 10,000. [15] [44] The lander,and landing system components,must be assembled and tested in a clean room where all parts would have to be cleaned or sterilized before they are installed in the spacecraft. After delivering the lander,the sky crane is recommended to fly away into Jupiter for disposal. [45] At the end of the mission,the lander might self-destruct using an incendiary device. [15] That system can also be triggered if the spacecraft loses contact with the Earth. [32]
The Europa Clipper is a separately launched spacecraft that would lay a foundation for the Europa Lander mission. [3] Previously,NASA had evaluated launching the orbiter and lander together,but the strong congressional support led to an additional proposal in 2016 for a separate lander mission. [46] The Clipper orbiter will provide reconnaissance data to characterize the radiation environment and help determine a landing location. [47]
Europa, or Jupiter II, is the smallest of the four Galilean moons orbiting Jupiter, and the sixth-closest to the planet of all the 95 known moons of Jupiter. It is also the sixth-largest moon in the Solar System. Europa was discovered independently by Simon Marius and Galileo Galilei and was named after Europa, the Phoenician mother of King Minos of Crete and lover of Zeus.
The Jupiter Icy Moons Orbiter (JIMO) was a proposed NASA spacecraft designed to explore the icy moons of Jupiter. The main target was Europa, where an ocean of liquid water may harbor alien life. Ganymede and Callisto, which are now thought to also have liquid, salty oceans beneath their icy surfaces, were also targets of interest for the probe.
The Discovery Program is a series of Solar System exploration missions funded by the U.S. National Aeronautics and Space Administration (NASA) through its Planetary Missions Program Office. The cost of each mission is capped at a lower level than missions from NASA's New Frontiers or Flagship Programs. As a result, Discovery missions tend to be more focused on a specific scientific goal rather than serving a general purpose.
The New Frontiers program is a series of space exploration missions being conducted by NASA with the purpose of furthering the understanding of the Solar System. The program selects medium-class missions which can provide high science returns.
The exploration of Jupiter has been conducted via close observations by automated spacecraft. It began with the arrival of Pioneer 10 into the Jovian system in 1973, and, as of 2024, has continued with eight further spacecraft missions in the vicinity of Jupiter and two more en route. All but one of these missions were undertaken by the National Aeronautics and Space Administration (NASA), and all but four were flybys taking detailed observations without landing or entering orbit. These probes make Jupiter the most visited of the Solar System's outer planets as all missions to the outer Solar System have used Jupiter flybys. On 5 July 2016, spacecraft Juno arrived and entered the planet's orbit—the second craft ever to do so. Sending a craft to Jupiter is difficult, mostly due to large fuel requirements and the effects of the planet's harsh radiation environment.
The exploration of Saturn has been solely performed by crewless probes. Three missions were flybys, which formed an extended foundation of knowledge about the system. The Cassini–Huygens spacecraft, launched in 1997, was in orbit from 2004 to 2017.
The Europa Orbiter was a planned NASA mission to Jupiter's Moon Europa, that was cancelled in 2002. Its main objectives included determining the presence or absence of a subsurface ocean and identifying candidate sites for future lander missions. Europa Orbiter received pre-project funding in 1998, and resulted from NASA's Fire and Ice project.
Io Volcano Observer (IVO) is a proposed low-cost mission to explore Jupiter's moon Io to understand tidal heating as a fundamental planetary process. The main science goals are to understand (A) how and where tidal heat is generated inside Io, (B) how tidal heat is transported to the surface, and (C) how Io is evolving. These results are expected to have direct implications for the thermal history of Europa and Ganymede as well as provide insights into other tidally heated worlds such as Titan and Enceladus. The IVO data may also improve our understanding of magma oceans and thus the early evolution of the Earth and Moon.
Laplace-P was a proposed orbiter and lander by the Russian Federal Space Agency designed to study the Jovian moon system and explore Ganymede with a lander.
The Jupiter Icy Moons Explorer is an interplanetary spacecraft on its way to orbit and study three icy moons of Jupiter: Ganymede, Callisto, and Europa. These planetary-mass moons are planned to be studied because they are thought to have significant bodies of liquid water beneath their frozen surfaces, which would make them potentially habitable for extraterrestrial life.
Europa Clipper is a space probe developed by NASA to study Europa, a Galilean moon of Jupiter. It was launched on October 14, 2024. The spacecraft will use gravity assists from Mars on March 1, 2025, and Earth on December 3, 2026, before arriving at Europa in April 2030. The spacecraft will then perform a series of flybys of Europa while in orbit around Jupiter.
The Ocean Worlds Exploration Program (OWEP) is a NASA program to explore ocean worlds in the outer Solar System that could possess subsurface oceans to assess their habitability and to seek biosignatures of simple extraterrestrial life.
The Mapping Imaging Spectrometer for Europa (MISE) is an imaging near infrared spectrometer on board the Europa Clipper mission to Jupiter's moon Europa. MISE will examine Europa's surface composition and relate it to the habitability of its internal water ocean.
The Planetary Missions Program Office is a division of NASA headquartered at the Marshall Space Flight Center, formed by the agency's Science Mission Directorate (SMD). Succeeding the Discovery and New Frontiers Program Office, it was established in 2014 to manage the Discovery and New Frontiers programs of low and medium-cost missions by third-party institutions, and the Solar System Exploration program of NASA-led missions that focus on prioritized planetary science objectives. The Discovery and New Frontiers programs were established in 1992 and 2001 respectively, and have launched fourteen primary missions together, along with two missions launched under the administration of the Planetary Missions Program Office. The Solar System Exploration Program was established alongside the office, with three missions planned for launch under the new program.
Commercial Lunar Payload Services (CLPS) is a NASA program to hire companies to send small robotic landers and rovers to the Moon. Most landing sites are near the lunar south pole where they will scout for lunar resources, test in situ resource utilization (ISRU) concepts, and perform lunar science to support the Artemis lunar program. CLPS is intended to buy end-to-end payload services between Earth and the lunar surface using fixed-price contracts. The program achieved the first landing on the moon by a commercial company in history with the IM-1 mission in 2024. The program was extended to add support for large payloads starting after 2025.
The Enceladus Orbilander is a proposed NASA Flagship mission to Saturn's moon Enceladus. The Enceladus Orbilander would spend a year and a half orbiting Enceladus and sampling its water plumes, which stretch into space, before landing on the surface for a two-year mission to study materials for evidence of life. The mission, with an estimated cost of $4.9 billion, could launch in the late 2030s on a Space Launch System or Falcon Heavy with a landing in the early 2050s. It was proposed in the 2023–2032 Planetary Science Decadal Survey as the third highest priority Flagship mission, after the Uranus Orbiter and Probe and the Mars Sample Return program.
The Europa Clipper Magnetometer (ECM) is a spacecraft magnetometer aboard the planned Europa Clipper mission. It will be used to precisely measure Europa's magnetic field during consecutive fly-bys, allowing scientists to potentially confirm the existence of Europa's hypothesised subsurface ocean. If this ocean exists, the instrument will be able to determine its depth and salinity, as well as the thickness of the moon's icy shell.