Mass Spectrometer for Planetary Exploration

Last updated
MASPEX
Europa Clipper's Mass Spectrometer.jpg
Operator NASA
Manufacturer Southwest Research Institute
Instrument type mass spectrometer
Functionchemical analyzer
Mission durationCruise: 3-6 years
Science phase: ≥ 3 years
Properties
Mass8 kg
Dimensions40 cm
Resolution1 ppt
Host spacecraft
Spacecraft Europa Clipper
Operator NASA
Launch date≈ 2025 [1]
Rocket SLS
Launch site Kennedy Space Center

The MAss Spectrometer for Planetary EXploration (MASPEX) is a mass spectrometer capable of high-resolution and high-sensitivity that allows the determination of a wide variety of chemical compounds in complex mixtures. This instrument will fly on board the planned Europa Clipper orbiter to explore Jupiter's moon Europa. This astrobiology mission will analyse the composition of Europa's surface while in orbit, and will directly assess its internal ocean habitability by flying through Europa's tenuous atmosphere.

Contents

On 27 May 2016 it was announced that MASPEX was selected to fly on the mission. [2] The launch is planned for approximately 2025. The instrument has also been proposed to fly on three Discovery program missions: Enceladus Life Finder (ELF), comet Hartley 2 (PRIME), and to the main belt comet Read (Proteus). [3] It also has applications for probes, landers, and sample return missions. The original Principal Investigator was Jack Waite, and the Technical Lead is Tim Brockwell, from the Southwest Research Institute. In 2020 NASA announced that Jim Burch of Southwest Research Institute would become the Principal Investigator and that some instrument capabilities might be reduced due to technical and financial limitations.

Overview

MASPEX is a next generation spectrometer with significantly improved performance over existing instruments, [4] that was developed over 10 years by the Southwest Research Institute. Development of the MASPEX was born out of the need to separate and analyze the unexpectedly rich volatile mixtures discovered by the Cassini INMS instrument at Titan and Enceladus. The instrument is a high-resolution, high-sensitivity mass spectrometer developed for planetary applications. Its high-resolution allows the unambiguous determination of volatile isotopes of methane, water, ammonia, carbon monoxide, molecular nitrogen (N2), carbon dioxide (CO
2
), and small organic compounds (C2, C3, and C4) in complex mixtures. [3] [4] MASPEX can also measure compounds in trace amounts (ppt), including the noble gases argon, krypton, xenon, and their isotopes. [3] [4]

The MASPEX can operate in a heavy radiation environment, and can be baked to 300 °C for planetary protection against forward biological contamination in case the probe impacts any potentially habitable moon of Jupiter. [4] MASPEX can observe spatial features as small as 400 km of orbital track at high scan rates, and can operate at 5 kHz across full mass range. [4] Other areas of enhanced performance over existing instruments include: [4]

ParameterPerformance
Extended mass range
for heavy organic molecules
>1000 amu
Enhanced mass resolution>30,000 M/dM
Enhanced dynamic range109 in a 1s period
Improved sensitivitybetter than 1ppt with cryotrapping
High throughput>5000 samples/s
Length and mass40 cm and < 8 kg

See also

Related Research Articles

<span class="mw-page-title-main">Astrobiology</span> Science concerned with life in the universe

Astrobiology is a scientific field within the life and environmental sciences that studies the origins, early evolution, distribution, and future of life in the universe by investigating its deterministic conditions and contingent events. As a discipline, astrobiology is founded on the premise that life may exist beyond Earth.

<span class="mw-page-title-main">Enceladus</span> Natural satellite orbiting Saturn

Enceladus is the sixth-largest moon of Saturn. It is about 500 kilometers in diameter, about a tenth of that of Saturn's largest moon, Titan. It is mostly covered by fresh, clean ice, making it one of the most reflective bodies of the Solar System. Consequently, its surface temperature at noon reaches only −198 °C, far colder than a light-absorbing body would be. Despite its small size, Enceladus has a wide variety of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrain.

A biosignature is any substance – such as an element, isotope, molecule, or phenomenon that provides scientific evidence of past or present life. Measurable attributes of life include its complex physical or chemical structures, its use of free energy, and the production of biomass and wastes.

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.

<span class="mw-page-title-main">Habitability of natural satellites</span> Measure of the potential of natural satellites to have environments hospitable to life

The habitability of natural satellites is the potential of moons to provide habitats for life, though it is not an indicator that they harbor it. Natural satellites are expected to outnumber planets by a large margin and the study of their habitability is therefore important to astrobiology and the search for extraterrestrial life. There are, nevertheless, significant environmental variables specific to moons.

<span class="mw-page-title-main">Europa Clipper</span> Planned NASA space mission to Jupiter

Europa Clipper is an interplanetary mission in development by NASA comprising an orbiter. Planned for launch in October 2024, the spacecraft is being developed to study the Galilean moon Europa through a series of flybys while in orbit around Jupiter.

<span class="mw-page-title-main">Enceladus Life Finder</span> Proposed NASA mission to a moon of Saturn

Enceladus Life Finder (ELF) is a proposed astrobiology mission concept for a NASA spacecraft intended to assess the habitability of the internal aquatic ocean of Enceladus, which is Saturn's sixth-largest moon of at least 146 total moons, and seemingly similar in chemical makeup to comets. The spaceprobe would orbit Saturn and fly through Enceladus's geyser-like plumes multiple times. It would be powered by energy supplied from solar panels on the spacecraft.

Journey to Enceladus and Titan (JET) is an astrobiology mission concept to assess the habitability potential of Enceladus and Titan, moons of Saturn.

Life Investigation For Enceladus (LIFE) was a proposed astrobiology mission concept that would capture icy particles from Saturn's moon Enceladus and return them to Earth, where they could be studied in detail for signs of life such as biomolecules.

THEO is a feasibility study for a New Frontiers class orbiter mission to Enceladus that would directly sample its south pole water plumes in order to study its internal habitability and to search for biosignatures. Specifically, it would take advantage of the direct sampling opportunities of a subsurface ocean.

<span class="mw-page-title-main">Europa Lander</span> Proposed NASA lander for Europa

The Europa Lander is a proposed astrobiology mission concept by NASA to send a lander to Europa, an icy moon of Jupiter. 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.

<span class="mw-page-title-main">Oceanus (Titan orbiter)</span>

Oceanus is a NASA/JPL orbiter mission concept proposed in 2017 for the New Frontiers mission #4, but it was not selected for development. If selected at some future opportunity, Oceanus would travel to Saturn's moon Titan to assess its habitability. Studying Titan would help understand the early Earth and exoplanets which orbit other stars. The mission is named after Oceanus, the Greek god of oceans.

<span class="mw-page-title-main">Explorer of Enceladus and Titan</span> NASA/ESA Saturnian moon probe concept

Explorer of Enceladus and Titan (E2T) is a space mission concept that would investigate the evolution and habitability of the Saturnian satellites Enceladus and Titan and is proposed by the European Space Agency in collaboration with NASA.

<span class="mw-page-title-main">Ocean Worlds Exploration Program</span> NASA program for the exploration of water worlds in the Solar System

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.

Venus Origins Explorer (VOX) is a concept orbiter mission to Venus.

<span class="mw-page-title-main">Mapping Imaging Spectrometer for Europa</span> Near infrared spectrometer

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 Enceladus Icy Jet Analyzer (ENIJA) is a time-of-flight mass spectrometer developed to search for prebiotic molecules like amino acids and biosignatures in the plumes of Saturn's moon Enceladus.

<span class="mw-page-title-main">Surface Dust Analyser</span>

The SUrface Dust Analyser (SUDA) is a time-of-flight mass spectrometer of reflectron-type that employs impact ionization and is optimised for a high mass resolution. The instrument was selected in May 2015 to fly on board the Europa Clipper mission, that is planned for 2025 to Jupiter's moon Europa.

Tianwen-4, formerly known as Gan De, is a planned interplanetary mission by China to study the Jovian system and its environs, sharing a launch with a spacecraft which will make a flyby of Uranus.

<span class="mw-page-title-main">Enceladus Orbilander</span> Proposed NASA space probe to Saturns moon Enceladus

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.

References

  1. Europa Clipper passes key review. Jeff Foust, Space News. 22 August 2019.
  2. "Two Southwest Research Institute instruments selected for NASA Europa mission". SWRI. 27 May 2016. Retrieved 2017-10-24.
  3. 1 2 3 The mass spectrometer for planetary exploration (MASPEX). Tim G. Brockwell, Karen J. Meech, Keith Pickens, J. Hunter Waite, Greg Miller, John Roberts, Jonathan I. Lunine, et al. 2016 IEEE Aerospace Conference 2016; doi : 10.1109/AERO.2016.7500777; Publisher: IEEE, Conference Location: Big Sky, MT, USA; 5–12 March 2016.
  4. 1 2 3 4 5 6 MAss Spectrometer for Planetary EXploration (MASPEX).pptx The MAss Spectrometer for Planetary EXploration (MASPEX) [ dead link ] (Power Point); Mark Libardoni, et al. 10th International Planetary Probe Workshop; San Jose, CA. June 2013.