Instruments selected for Mars 2020, NASA’s latest rover

NASA is sending another rover to Mars in 2020, imaginatively named “Mars 2020.” Earlier this month, NASA announced Mars 2020’s scientific payload: seven instruments, costing roughly $130 million, all of which are, to use a technical term, super rad.

Mars 2020 is basically a souped-up version of Curiosity, the car-sized rover currently exploring Gale Crater. Copying elements of Curiosity’s design—particularly the entry, descent, and landing system—saves a lot of money and lets engineers take advantage of proven technology. (Mars 2020 will have sturdier tires than Curiosity.) If you parked Curiosity and Mars 2020 next to each other on Mars, most people wouldn’t be able to tell them apart. Well, “most people” can’t tell Mars from Arizona (there’s a strong resemblance!), but you get my point…

However, despite their physical similarities, Mars 2020 represents a completely different philosophy of planetary exploration. Whereas Curiosity is studying Mars in situ, the primary goal of Mars 2020 is preparing a cache of samples for eventual return to Earth. Curiosity aims to determine whether environments conducive to life ever existed on Mars (they did); scientists will analyze samples collected by Mars 2020 in sophisticated laboratories on Earth, which might allow them to discover whether life or its precursors actually existed on Mars.

Planetary scientists agree that sample return is crucial to answering pressing questions about Mars. But planning a sample return mission involves potential pitfalls worth knowing about.

Sample Return: Go Big and Go Home

Every ten years, the planetary science community comes together to write a report, called a decadal survey, containing a prioritized list of missions and programs for the next decade. The last decadal survey, released in 2011, went all in on Mars sample return, endorsing a rover that would prepare a sample cache (then known as “MAX-C”) as the highest priority, large-class mission—but did not recommend any alternative medium- or large-class missions to Mars.

A caching rover is only the first part of a sample return campaign. Another mission is required to pick up the cache and launch it into orbit around Mars. We’d need yet another spacecraft to bring this precious cargo back to Earth—not to mention all the specialized facilities we’d construct here to handle and analyze the samples! All of this could take ~30 years and cost more than $10 billion.

Policymakers are reluctant to commit to hugely expensive research projects that won’t yield scientific results for several decades. This is always true, but especially now given our dismal fiscal climate and the cost and schedule overruns associated with JWST and, to a lesser extent, Curiosity. However, the decadal survey offered no Plan B for Mars exploration. NASA would either need to commit to sample return or smash the crown jewel of its own exploration program. Maybe this was a strategic attempt to force NASA to commit to a more ambitious plan than they’d otherwise undertake.

Initially, it looked like this strategy, if it was a strategy, would fail. The Obama Administration’s budget request for fiscal year 2014 gutted Mars exploration, slashing hundreds of millions of dollars relative to the 2012 budget. NASA pulled out of a planned collaboration with the European ExoMars program.

Congress reinstated funding for Mars exploration after a loud outcry from planetary scientists and enthusiasts. With this funding, NASA announced that Mars 2020 would happen and, later, that Mars 2020 would indeed focus on preparing a sample cache.

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Figure 1: Example sample cache. Each sample tube is about as big as a half-used No. 2 pencil. The details of how many samples the cache will actually hold, etc. haven’t been figured out yet. (Image credit: NASA.)

Mars 2020’s Instrumental Payload

Now that we’ve discussed the overall goals and philosophy of Mars 2020, let’s admire the instruments it’ll actually use:

SuperCam — an upgrade to Curiosity’s meme-worthy ChemCam, which will analyze the chemical composition of surface material, including organic material, from afar using a laser.

Planetary Instrument for X-ray Lithochemistry (PIXL) — an X-ray fluorescence spectrometer and high-resolution imager to map samples of surface material in fine detail.

Scanning Habitable Environments with Raman & Luminescence for Organics and Chemicals (SHERLOC) — like PIXL, will map surface material at high-resolution, but using laser Raman fluorescence spectroscopy.

The Radar Imager for Mars’ Subsurface Experiment (RIMFAX) — ground-penetrating radar that can map geologic layers up to roughly half a kilometer below the surface, at 5-20 centimeter resolution, contributed by Norway.

Mars Environmental Dynamics Analyzer (MEDA) — a weather station that can measure temperature, wind velocity, pressure, relative humidity, and dust characteristics, supplied by Spain.

Mastcam-Z — two super fancy cameras that can zoom and take movies (hopefully of Mars bears or something) in twelve different wavelength bands in the visible and near infrared parts of the color spectrum.

The Mars Oxygen ISRU Experiment (MOXIE) — an engineering demonstration experiment that will produce oxygen from atmospheric carbon dioxide, which future missions would find exceedingly helpful, since oxygen is part of rocket fuel and, err, breathable.

Figure 2: Diagram of the Mars 2020 with the locations of the instruments and supporting hardware. (Image credit: NASA.)

Figure 2: Diagram of the Mars 2020 with the locations of the instruments and supporting hardware. (Image credit: NASA.)

About Joseph O'Rourke

I am a first-year graduate student in planetary science at the California Institute of Technology, where I work with Heather Knutson and David Stevenson. My research interests include the formation of gas giant planets, the internal structures of icy satellites, and the thermo-chemical evolution of terrestrial planets. My favorite planet is Venus and my favorite ice cream flavor is mint chocolate chip. I received my bachelor's degree in Astronomy & Physics and Geology & Geophysics from Yale University in May 2012.

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