This Solicitation opportunity from Government of Canada was posted on February 12, 2026. The submission period has ended. Browse the details below for market research, or find similar active opportunities.

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Development of the Martian Atmospheric Gas Evolution Experiment – Inter-Cavity Optical Spectroscopy (MAGE-ICOS)

Closed

9F063-20250304Canada

Submission Closed02/27/2026, 07:00:00 PM UTC

Contract Overview

Solicitation details, issuing organization, response deadlines, documents, and interested companies for this government contract opportunity.

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NAICS: 541715

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Marshall Space Flight Center

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Armstrong Flight Research Center

POSTED

in 6 months

DEADLINE

N/A

General Info

Agency

Government of Canada → Canadian Space AgencyView Agency

NAICS

541715 - Research and Development in the Physical, Engineering, and Life Sciences (except Nanotechnology and Biotechnology) View NAICS

Place of Performance

Longueuil, CAN

Set-Aside

NONE

Documents

(2)

ACAN for MAGE-ICOS_20250304.pdf

PDF

PAC pour MAGE-ICOS_20250304.pdf

PDF

AI Contract Breakdown

Uniform Contract Format

Timeline

PhaseClosed

PostedFeb 12

Solicitation

Response DeadlineFeb 27

Deadline has passed

Submission Closed

02/27/2026, 07:00:00 PM UTC

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Organization & Contact Information

AgencyGovernment of Canada → Canadian Space Agency

Contacts1 person available

OfficeN/A

Organization / Agency

Government of Canada → Canadian Space Agency

View Agency Profile

Office AddressN/A

Contacts

R&D ProcurementContracting Authority

contact@example.gov

Full Description

The Canadian Space Agency (CSA) requires specialized research and development services to advance the Martian Atmospheric Gas Evolution Experiment – Inter-Cavity Optical Spectroscopy (MAGE-ICOS). The work will focus on maturing ICOS technology for in-situ detection of methane on Mars, including: • development and optimization of low-pressure ICOS instrumentation; • miniaturization of instrument mass and volume relative to commercial ICOS systems; • environmental testing under simulated Martian atmospheric conditions (100–130 Torr); • performance characterization at trace methane detection thresholds; • delivery of engineering reports, design updates, and prototype hardware as detailed in Annex A.