MGS-1 Mars Global Simulant MGS-1

Mixed mineral powder: anorthosite (plagioclase), glass-rich basalt, pyroxene, olivine, Mg-sulfate, ferrihydrite, hydrated silica, magnetite, anhydrite, Fe-carbonate and hematite

MGS-1 Mars Global Simulant is an open-standard powder that reproduces the mineral mix of the Rocknest windblown soil at Gale crater, Mars.

8 sources · Updated 2026-11-01 · CC BY 4.0

Evidence level

2 of 5

Lab-measured

Bulk density

1.29 g/cm³

Flow behaviour

38.9 °

Particle size

60 μm

Water on heating

3.2 wt%

Volatile sulfur

> 1.27 wt%

Recipe, share of the weight

  • 27.1%Anorthosite (plagioclase)
  • 22.9%Glass-rich basalt (basaltic glass)
  • 20.3%Pyroxene
  • 13.7%Olivine
  • 4%Mg-sulfate
  • 3.5%Ferrihydrite
  • 3%Hydrated silica
  • 1.9%Magnetite
  • 1.7%Anhydrite
  • 1.4%Fe-carbonate (siderite)
  • 0.5%Hematite

Best for

Ground tests of hardware and of in-situ resource utilization on a basaltic Mars analogue, where mineral mix and volatile content matter most (Cannon et al. 2019, Section 5.1)

Weakest at

Bulk chemistry: the fact sheet and the Cannon et al. prototype give different oxide values (SiO2 42.9 wt% against 50.8 wt%), so no single bulk chemistry is settled

Risk at a glance

  • People None found. Dust is the stated hazard; use a respirator.
  • If it fails No data. No failure risks recorded
  • Corrosion Moderate. The prototype loses 3.9% of its mass on heating from 30 to 500 °C.

Why it exists

MGS-1 is an open-standard simulant of basaltic Martian regolith. Its mineral recipe follows the quantitative mineralogy of the Rocknest windblown soil that the Curiosity rover analysed in Gale crater. Cannon et al. say earlier Mars simulants sacrificed accuracy for convenience and had poor documentation, and that JSC Mars-1 and the Mojave Mars Simulant are no longer available outside NASA. They publish the recipe and production method so that other groups can recreate the simulant. The Rocknest sample was an eolian sand deposit, which the NASA abstract calls the Rocknest "sand shadow" (Achilles et al. 2016, NTRS 20160002646). Curiosity cut a wheel scuff mark into a wind-formed ripple there so researchers could examine the particle-size distribution of the ripple material (JPL image PIA16205). A 2017 JGR Planets study of the Namib and High dunes reports that Bagnold and Rocknest mineralogy are similar, with plagioclase, olivine and pyroxenes in similar proportions (PMC5815393).

Where it's used

Hardware testing

Cannon et al. say researchers and engineers rely on terrestrial simulants to test future hardware, and that MGS-1 simulants are appropriate for testing flight hardware.

In-situ resource utilization

Cannon et al. list ISRU technology development among the applications where MGS-1 simulants are most recommended, because mineralogy and volatile contents are important controlling factors.

Recipe

Mixed mineral powder: anorthosite (plagioclase), glass-rich basalt, pyroxene, olivine, Mg-sulfate, ferrihydrite, hydrated silica, magnetite, anhydrite, Fe-carbonate and hematite

MGS-1 is a mixture of mineral powders, not one compound. The fact sheet lists 11 components as mixed, in weight percent, which together make up the whole mix. Cannon et al. made their prototypes by mixing plagioclase, pyroxene, olivine, basaltic glass and magnetite with water and a sodium metasilicate binder, drying the paste into hard cobbles, grinding the cobbles and mixing them with the secondary phases.

What MGS-1 is made of
IngredientShare of the weightWhat it does
Anorthosite (plagioclase) 27.1% Largest crystalline component. The fact sheet calls it anorthosite; Cannon et al. call it plagioclase.
Glass-rich basalt (basaltic glass) 22.9% Amorphous basaltic glass, an X-ray amorphous phase in the mix.
Pyroxene 20.3% Crystalline silicate. Cannon et al. used a bronzite-variety pyroxene from Brazil.
Olivine 13.7% Crystalline silicate. Cannon et al. used highly forsteritic San Carlos olivine.
Mg-sulfate 4% Sulfate. Its breakdown releases SO2 and O2 near 950 °C on heating.
Ferrihydrite 3.5% Iron oxyhydroxide. Cannon et al. say ferrihydrite and hematite act as strong pigments. Table 1 gives 1.7 wt%.
Hydrated silica 3% Secondary phase. Cannon et al. Table 1 lists it as hydrated silica (opal) at 5.0 wt%.
Magnetite 1.9% Magnetic iron oxide. Cannon et al. say magnetite matters for the magnetic properties.
Anhydrite 1.7% Sulfate. Cannon et al. use anhydrite for sulfur content. Table 1 gives 0.9 wt%.
Fe-carbonate (siderite) 1.4% Iron carbonate. Its breakdown gives a sharp CO2 release on heating.
Hematite 0.5% Iron oxide and pigment. Cannon et al. Table 1 gives 1.1 wt%.

Weight shares are as printed in the sources.

What it can do

Bulk density

1.29 g/cm³

measured

The uncompressed bulk density is 1.29 g/cm3 per the fact sheet, and Cannon et al. report the same value for their prototype.

Flow behaviour

38.9 °

measured

The fact sheet gives an average angle of repose of 38.9° and a maximum of 43.6°.

Particle size

60 μm

measured

The fact sheet gives a mean particle size of 90 μm and a median of 60 μm from laser diffraction. Cannon et al.'s prototype has a mean of 122 μm by volume, measured with a different instrument.

Water on heating

3.2 wt%

measured

Heated from 30 to 500 °C, the prototype released water equal to 3.2 wt% of MGS-1 (Cannon et al. 2019, Section 4.4).

Volatile sulfur

> 1.27 wt%

measured

The fact sheet gives SO3 of at least 1.27 wt%, measured by XRF.

How it compares

Cannon et al. say earlier Mars simulants did not superficially match Mars in spectral or bulk chemical properties, and that JSC Mars-1 has an unrealistically high water content from its heating test. MGS-1 is designed as a mineralogical match to Rocknest instead. The prototype's bulk density of 1.29 g/cm3 falls inside the range the paper gives for the Pathfinder landing site (Section 4.1). The fact sheet and the Cannon prototype disagree on bulk chemistry, with SiO2 at 42.9 wt% on the fact sheet and 50.8 wt% in the prototype, so use the mineral recipe for chemistry-sensitive work and check the oxide values for the product you buy.

The same measurements for each material, so you can compare them. Each row names the key condition under the value; the full conditions and methods are in the numbered notes under Technical details.

Benchmarks
MeasurementMGS-1
Physical and electrical
Uncompressed bulk density1.29 g/cm³1
Other measurements
Average angle of repose38.9 °2
Maximum angle of repose43.6 °3
Mean particle size (fact sheet)90 μm4
Median particle size (fact sheet)Printed on the fact sheet header block60 μm
Particle size range (fact sheet)Printed range on the fact sheet0.04 to 600 μm5
Fraction finer than 53 μm by mass (sieve)3.6 % by mass6
Mean grain size by volume (Cannon prototype)122 μm7
SiO2, XRF (fact sheet)42.9 wt%8
SiO2, XRF (Cannon prototype)50.8 wt%9
MgO, XRF (fact sheet)14.6 wt%10
MgO, XRF (Cannon prototype)16.7 wt%11
FeO, XRF (fact sheet)11.2 wt%12
FeOT (total iron as FeO, Cannon prototype)13.3 wt%13
Al2O3, XRF (fact sheet)12.8 wt%14
Al2O3, XRF (Cannon prototype)8.9 wt%15
Loss on ignition (LOI), fact sheetPrinted on the fact sheet, footnote LOI5.3 wt%
Mass loss on heating, 30 to 500 °C (prototype)3.9 %16
Water (H2O) equivalent from mass loss, 30 to 500 °C3.2 wt%17
Sulfur trioxide (volatile), XRFPrinted in the Volatiles table on the fact sheet> 1.27 wt%
Fluorine (volatile), XRFPrinted in the Volatiles table on the fact sheet> 0.1 wt%
Chlorine (volatile), XRFPrinted in the Volatiles table on the fact sheet> 0.005 wt%
Anorthosite (plagioclase), as mixed27.1 wt%18
Glass-rich basalt (basaltic glass), as mixed22.9 wt%19
Pyroxene, as mixed20.3 wt%20
Olivine, as mixed13.7 wt%21
Mg-sulfate, as mixed4 wt%22
Ferrihydrite, as mixed (fact sheet)3.5 wt%23
Ferrihydrite, Cannon et al. Table 1 prototype recipePrinted in Table 1 of Cannon et al. 20191.7 wt%24
Hydrated silica, as mixed (fact sheet)3 wt%25
Hydrated silica (opal), Cannon et al. Table 1 prototype recipe5 wt%26
Magnetite, as mixed1.9 wt%27
Anhydrite, as mixed (fact sheet)1.7 wt%28
Anhydrite, Cannon et al. Table 1 prototype recipePrinted in Table 1 of Cannon et al. 20190.9 wt%29
Fe-carbonate (siderite), as mixed1.4 wt%30
Hematite, as mixed (fact sheet)0.5 wt%31
Hematite, Cannon et al. Table 1 prototype recipePrinted in Table 1 of Cannon et al. 20191.1 wt%32

Why choose it, and why not

Good for

  • Hardware and ISRU tests where mineralogy and volatile content matter. Cannon et al. recommend MGS-1 for those uses.
  • Tests that need a documented, reproducible recipe. Cannon et al. publish the recipe and production method.

Watch out for

  • Bulk chemistry: the fact sheet and the Cannon prototype disagree (SiO2 42.9 wt% against 50.8 wt%; MgO 14.6 wt% against 16.7 wt%).
  • Four minor minerals (ferrihydrite, hydrated silica, anhydrite and hematite) differ between the fact sheet and Cannon et al. Table 1.
  • Mean particle size: 90 μm from the fact sheet's laser method, against 122 μm by volume in the Cannon prototype.
  • The Cannon values come from a lab-made prototype. The commercial product may differ.

MGS-1 is a published, open recipe for basaltic Martian regolith with sourced density, particle-size and mineral-mix values. Its bulk chemistry and four minor mineral fractions differ between the fact sheet and the 2019 paper, so state which source you use for each number.

Technical details

For scientists and researchers. Everything above comes from the record below: every number with its method, its conditions and its source.

Notes

The method, full conditions and any caveat for the numbered rows above.

Notes for the numbered rows
#MeasurementMethodConditionsCaveat
1Uncompressed bulk densityPrinted value on the fact sheet; Cannon et al. 2019 report the same 1.29 g/cm3 for their prototype (Section 4.1)state uncompressed bulk powder, as mixedbasis value printed on the fact sheetCannon et al. 2019 say they could not find a published density or porosity for Rocknest soil itself.
2Average angle of reposePrinted on the fact sheet, Geotechnical Properties blockbasis average angle of repose as printed; test method not stated—
3Maximum angle of reposePrinted on the fact sheet, Geotechnical Properties blockbasis maximum angle of repose as printed; test method not stated—
4Mean particle size (fact sheet)Printed on the fact sheet; the volumetric distribution slide names the CILAS 1190 analyzerdistribution volumetric, laser diffractioninstrument CILAS 1190 laser diffraction particle size analyzer—
5Particle size range (fact sheet)—bound note the fact sheet prints the lower limit as greater than 0.04 μmThe lower limit is printed as greater than 0.04 μm, so 0.04 μm is a bound, not a measured minimum.
6Fraction finer than 53 μm by mass (sieve)Printed under Sieve Analysis; the fact sheet notes that sieving skews sizes larger because fines cling to coarse grainsmethod sieve analysis following ASTM E11 with RO-TAP RX-30 shakerbasis mass—
7Mean grain size by volume (Cannon prototype)Measured at Johnson Space Center ARES facilities (Section 3.3); the paper reports the mean by volumebasis prototype sieved below 1 mm; volume meanmedium isopropyl alcoholinstrument Microtrac S3500 particle size analyzerreplicates measured in triplicateDifferent instrument and sample preparation from the fact sheet's 90 μm mean, so the two means are not directly comparable.
8SiO2, XRF (fact sheet)Printed in the Bulk Chemistry table as Oxide Wt.%method XRF on fused bead, relative abundances, Hamilton Analytical Labbasis oxide wt%—
9SiO2, XRF (Cannon prototype)Measured by Cannon et al. (Section 3.3) and printed in Table 2, MGS-1 prototype columnbasis prototype MGS-1 simulant, measured by XRF in oxides mode at the UCF Materials Characterization FacilityDisagrees with the fact sheet's 42.9 wt%. Cannon et al. attribute deviations from Rocknest mainly to the silicate chemistry used, with MgO and FeO most affected.
10MgO, XRF (fact sheet)Printed in the Bulk Chemistry table as Oxide Wt.%method XRF on fused bead, relative abundances, Hamilton Analytical Labbasis oxide wt%—
11MgO, XRF (Cannon prototype)Measured by Cannon et al. (Section 3.3) and printed in Table 2, MGS-1 prototype columnbasis prototype MGS-1 simulant, measured by XRF in oxides mode at the UCF Materials Characterization FacilityDisagrees with the fact sheet's 14.6 wt%.
12FeO, XRF (fact sheet)Printed in the Bulk Chemistry table as Oxide Wt.%method XRF on fused bead, relative abundances, Hamilton Analytical Labbasis oxide wt%—
13FeOT (total iron as FeO, Cannon prototype)Measured by Cannon et al. (Section 3.3) and printed in Table 2, MGS-1 prototype columnbasis total iron expressed as FeO, prototype MGS-1 simulantTotal iron as FeO in the paper; the fact sheet prints FeO. Disagrees with the fact sheet's 11.2 wt%.
14Al2O3, XRF (fact sheet)Printed in the Bulk Chemistry table as Oxide Wt.%method XRF on fused bead, relative abundances, Hamilton Analytical Labbasis oxide wt%—
15Al2O3, XRF (Cannon prototype)Measured by Cannon et al. (Section 3.3) and printed in Table 2, MGS-1 prototype columnbasis prototype MGS-1 simulant, measured by XRF in oxides mode at the UCF Materials Characterization FacilityDisagrees with the fact sheet's 12.8 wt%.
16Mass loss on heating, 30 to 500 °C (prototype)Thermogravimetric analysis, reported by Cannon et al. (Section 4.4)range 30 to 500 °Csample MGS-1 prototype, not the fact-sheet productbasis relative mass—
17Water (H2O) equivalent from mass loss, 30 to 500 °CValue stated by Cannon et al. from the thermogravimetry data (Section 4.4)basis H2O-related mass loss expressed as wt% of MGS-1assumption siderite assumed to decompose completelysample MGS-1 prototype—
18Anorthosite (plagioclase), as mixedPrinted in the Mineralogy table. The fact sheet calls this anorthosite; Cannon et al. Table 1 calls it plagioclase at the same 27.1 wt%basis as mixed, share of the mineral components—
19Glass-rich basalt (basaltic glass), as mixedPrinted in the Mineralogy table; Cannon et al. Table 1 gives basaltic glass at the same 22.9 wt%basis as mixed, share of the mineral components—
20Pyroxene, as mixedPrinted in the Mineralogy table; Cannon et al. Table 1 gives the same 20.3 wt%basis as mixed, share of the mineral components—
21Olivine, as mixedPrinted in the Mineralogy table; Cannon et al. Table 1 gives the same 13.7 wt%basis as mixed, share of the mineral components—
22Mg-sulfate, as mixedPrinted in the Mineralogy table; Cannon et al. Table 1 gives the same 4.0 wt%basis as mixed, share of the mineral components—
23Ferrihydrite, as mixed (fact sheet)Printed in the Mineralogy table; Cannon et al. Table 1 gives a different value (see next entry)basis as mixed, share of the mineral componentsDisagrees with Cannon et al. Table 1 (1.7 wt%).
24Ferrihydrite, Cannon et al. Table 1 prototype recipe—basis prototype recipe, share of the mineral componentsDisagrees with the fact sheet's 3.5 wt%.
25Hydrated silica, as mixed (fact sheet)Printed in the Mineralogy table; Cannon et al. Table 1 gives a different value (see next entry)basis as mixed, share of the mineral componentsDisagrees with Cannon et al. Table 1 (5.0 wt%, labelled hydrated silica (opal)).
26Hydrated silica (opal), Cannon et al. Table 1 prototype recipePrinted in Table 1 of Cannon et al. 2019, amorphous phasesbasis prototype recipe, share of the mineral componentsDisagrees with the fact sheet's 3.0 wt%.
27Magnetite, as mixedPrinted in the Mineralogy table; Cannon et al. Table 1 gives the same 1.9 wt%basis as mixed, share of the mineral components—
28Anhydrite, as mixed (fact sheet)Printed in the Mineralogy table; Cannon et al. Table 1 gives a different value (see next entry)basis as mixed, share of the mineral componentsDisagrees with Cannon et al. Table 1 (0.9 wt%).
29Anhydrite, Cannon et al. Table 1 prototype recipe—basis prototype recipe, share of the mineral componentsDisagrees with the fact sheet's 1.7 wt%.
30Fe-carbonate (siderite), as mixedPrinted in the Mineralogy table; Cannon et al. Table 1 gives the same 1.4 wt%, named Fe-carbonated therebasis as mixed, share of the mineral components—
31Hematite, as mixed (fact sheet)Printed in the Mineralogy table; Cannon et al. Table 1 gives a different value (see next entry)basis as mixed, share of the mineral componentsDisagrees with Cannon et al. Table 1 (1.1 wt%).
32Hematite, Cannon et al. Table 1 prototype recipe—basis prototype recipe, share of the mineral componentsDisagrees with the fact sheet's 0.5 wt%.

Corrosion and compatibility

What happens when it meets other materials and environments.

Corrosion and compatibility
EnvironmentConcernWhat happens
Heating from 30 to 500 °C (MGS-1 prototype) moderate The prototype loses 3.9% of its mass on heating from 30 to 500 °C.1
Corrosion details
#EnvironmentDetailsTest conditions
1 Heating from 30 to 500 °C (MGS-1 prototype) Cannon et al. report 3.9% relative mass loss over 30 to 500 °C and state that the water-related part corresponds to 3.2 wt% of MGS-1, assuming the siderite decomposes completely. They also report a sharp CO2 release from siderite breakdown and SO2 and O2 release near 950 °C from Mg-sulfate breakdown. method thermogravimetry with evolved-gas analysissample MGS-1 prototype, not the fact-sheet product

Risks and side effects

Hazards to people, what happens when a cell overheats, and how the material is handled and stored.

For people

The fact sheet's only stated hazard is dust inhalation. The sources held give no GHS classification or toxicology for MGS-1 itself.

The powder
The fact sheet names dust inhalation as the primary hazard and advises a respirator in dusty conditions. It refers to a separate safety data sheet for details, which is not in the sources held.
Fine fraction
The fact sheet gives 3.6% by mass finer than 53 μm.

If the simulant is heated

These results come from laboratory heating of the Cannon et al. prototype, not from field incidents.

Mass loss
The prototype lost 3.9% of its mass between 30 and 500 °C. Cannon et al. state that 3.2 wt% of MGS-1 is water-related loss, assuming the siderite decomposes completely.
Gas release
Cannon et al. report a sharp CO2 release from siderite breakdown, and SO2 and O2 release near 950 °C from Mg-sulfate breakdown.

Handling and storage

Storage
The sources held give no storage rule for MGS-1. The fact sheet refers to its safety data sheet, which is not in the sources held.
Dust control
The fact sheet advises a respirator in dusty conditions.

Test details
The original wording and numbers from the sources, for readers who want them.

Side effects on surrounding parts

Side effects on surrounding parts
AffectsEffect
Gas analysis and furnace or oven exhaust during heating testsOn heating the prototype, Cannon et al. report a broad water release, a sharp CO2 release from siderite breakdown, and SO2 and O2 release near 950 °C from Mg-sulfate breakdown.

Handling and storage

  • Wear a respirator in dusty conditions (fact sheet safety note).
  • Cannon et al. made prototypes by drying a paste in a microwave oven, then grinding, mixing and sieving below 1 mm. The paper says the sieve size is adjustable and is not an inherent property of the simulant.

Supply and geography

How common the raw materials are and where they come from.

MGS-1 simulant (the product)

Not applicable: a manufactured mix of Earth minerals, not a mined commodity

Recycling
Not found in the sources held.

MGS-1 simulant (current supplier)

Not applicable

Recycling
Not found in the sources held.

Mineral feedstock (plagioclase, pyroxene, olivine)

Not found in the sources held

Recycling
Not found in the sources held.

Updated