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Giant Magellan Telescope

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uuid004hpva

Namestring
Giant Magellan Telescope
Legal namestring
GMTO Corporation
Company typeenum
Private
Founded yearint
2015
Descriptiontext

The Giant Magellan Telescope (GMT) is a ground-based astronomical research facility being constructed by GMTO Corporation, a U.S. nonprofit entity headquartered in Pasadena, California, and operated as an international scientific endeavor led by a consortium of 16 universities and research institutions spanning the United States, Chile, Australia, Brazil, Israel, South Korea, and Taiwan. The facility is being built at Las Campanas Observatory in Chile's Atacama Desert and is currently 40% complete, with first light projected around 2029. Its primary purpose is to provide next-generation observational capability to astronomers for studies including exoplanet detection and atmospheric biosignature characterization, galaxy formation and evolution, dark matter and dark energy research, and first-light observations of the early universe.

The telescope's core technology is a 25.4-meter effective aperture formed by seven 8.4-meter off-axis primary mirror segments (polished to 25-nanometer surface accuracy), employing a Gregorian optical design with seven deformable secondary mirrors that reshape up to 2,000 times per second to counteract atmospheric turbulence. The first-generation instrument suite includes the G-CLEF visible echelle spectrograph (the only high-resolution visible spectrograph planned for the first decade of any ELT), the GMTNIRS near-infrared echelle spectrograph, the GMTIFS integral field spectrograph, the GMag AO-X extreme adaptive optics coronagraph for direct Earth-like exoplanet imaging, and the MANIFEST multi-object fiber positioning system. The architecture delivers imaging 4-16x sharper than JWST from the ground, a 13x larger wide-field field of view than competing ELTs, and instruments up to 27x more compact than alternative ELT designs.

GMT's business model is a nonprofit consortium structure in which member institutions contribute capital and receive observing time proportional to their investment. To date, $1 billion in private funding has been secured (65% from U.S. institutions), supplemented by a $500M commitment from 11 founding partners in 2015, a $205M private raise in August 2022, and a $15M NSF grant in 2020, against a total $2.6 billion project value. The organization is actively pursuing National Science Foundation consortium membership following its June 2025 Final Design Phase advancement, which could accelerate construction from 40% to 90% completion within two years. Access for U.S. astronomers is also planned through the federally-funded US Extremely Large Telescope Program (US-ELTP), with philanthropic donations supplementing capital funding under the GMTO Corporation's 501(c)-equivalent nonprofit status.

Short descriptiontext

The Giant Magellan Telescope is a U.S. nonprofit-led international project constructing a 25.4-meter ground-based extremely large telescope in Chile's Atacama Desert, operated by a 16-member university consortium to provide astronomers with next-generation observational capabilities for exoplanet research and cosmology.

Operating statusenum
Operating
Ownership categoryenum
Headcount rangeband
51–100
akta.pro rankint
HeadquartersPasadena, United States
HQ citystring
Pasadena
HQ countrystring
United States
HQ regionstring
North America
Markets served

Serves global market

Offices3 records

Each record includes

City, Country, Type, Description, Source

Keyword5 values
ground-based telescopes, astronomical observatory construction, adaptive optics systems, exoplanet imaging instruments, scientific research consortium
SIC code1 code
  • Optical Instruments & Lenses3827
Product category
Ground-based Astronomical Observatory
Social media profiles2 records
GTM motion1 record

Each record includes

Type, Description, Source

Revenue model3 records
1Consortium Membership Contributions
TypeLicensing Royalties
Description

International consortium of 16 universities and research institutions fund the construction and operation of the telescope through membership contributions. The project is backed by $1 billion in private funding, with 65% coming from U.S. institutions and investors. An additional ~$500M was committed by the original 11 founding international partners at the start of construction.

giantmagellan.org
2National Science Foundation Funding
TypeLicensing Royalties
Description

Federal funding from the National Science Foundation (NSF) as a prospective consortium member. NSF budget requests to Congress advancing the telescope represent a major potential revenue stream. NSF support could bring the telescope from 40% to 90% completion within two years.

giantmagellan.org
3Philanthropic Donations
TypeLicensing Royalties
Description

Philanthropic giving from individuals and foundations supporting the telescope project. The GMTO Corporation is a nonprofit entity that accepts charitable contributions.

giantmagellan.org
Marketing channels7 records

Each record includes

Title, Type, Stage, Description, Source

Distribution channels2 records

Each record includes

Title, Type, Scope, Target buyer, Description, Source

Cost components5 values
Technology or R&D, Infrastructure, Personnel, Operations, Supply Chain
GTM typeB2B
B2B
Offering typeServices
Services
Core offering1 text field

GMTO Corporation is constructing the Giant Magellan Telescope, a 25.4-meter effective aperture ground-based extremely large telescope at Las Campanas Observatory in Chile's Atacama Desert, on behalf of an international consortium of 16 universities and research institutions. Once operational, the telescope will deliver astronomical observation capabilities to consortium members and U.S. astronomers through the US Extremely Large Telescope Program, supporting research in exoplanet detection, early-universe cosmology, dark matter, and spectroscopy.

Differentiator
Functional benefit
Problem solved
Quantifiable outcome1 of 6 values shown
  • 200x more powerful than today's best telescopes
+5 more records
Product and service2 records
1Giant Magellan Telescope (GMT)
CategoryGround-based astronomical telescope
Description

A 25.4-meter effective aperture ground-based extremely large telescope under construction at Las Campanas Observatory in Chile's Atacama Desert. Will deliver astronomical observation services to consortium member institutions and U.S. astronomers for research in exoplanet detection, early-universe cosmology, dark matter, and spectroscopy.

2GMTNIRS Near-Infrared Echelle Spectrograph
CategoryScientific instrument
Description

Single-object near-infrared to mid-infrared echelle spectrograph providing simultaneous coverage of full JHKLM bands with spectral resolutions of 65,000 (JHK) and 85,000 (LM) across a 1.1-5.4 micrometer wavelength range. Used by astronomers for detailed spectroscopic studies of celestial objects.

Scale indicator11 records

Each record includes

Type, Value, Description, Source

Partnership31 partners
Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2026-04-01
Description

Strategic partnership signed in April 2026 to strengthen the astronomy industry in Chile's Coquimbo region, supporting the local astronomical ecosystem around the telescope.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2025-09-01
Description

Joined the international consortium in September 2025 as its newest partner, expanding the American university consortium supporting the telescope.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2024-12-01
Description

Joined the international consortium in December 2024. Northwestern's CIERA center and Dr. Vicky Kalogera contribute expertise in multi-messenger astronomy and gravitational wave follow-up.

4Taiwan (National Science and Technology Council)
Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2024-02-01
Description

Joined the consortium in February 2024 as a new partner, expanding global scientific impact and bringing Taiwan's astronomical community into the GMT program.

giantmagellan.org
Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner from Australia. Contributed to the $500M founding commitment in 2015 and participates in telescope construction, mirror development, and scientific instrument programs.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Key founding partner developing the GMTIFS (Integral Field Spectrograph). ANU's Research School of Astronomy & Astrophysics contributes to the instrument suite and scientific program.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner providing the Las Campanas Observatory site in Chile where the telescope will be constructed and operated. Host institution for the project.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner through the Center for Astrophysics | Harvard & Smithsonian. Leads development of the G-CLEF (Large Earth Finder) first-light instrument. Dr. Andrew Szentgyorgyi is the principal investigator.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Joint founding partner with Harvard University through the Center for Astrophysics. Contributes to G-CLEF development and the GMACS instrument program.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner from South Korea. Increased investment announced in July 2026. Actively involved in synergies with ALMA, Rubin Observatory, and NASA's SPHEREx Telescope.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner. Worked on cleaning, assembling, and testing the support actuators for the primary mirror support system at the University of Arizona Mirror Lab.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner responsible for manufacturing all seven 8.4-meter primary mirrors at the Richard F. Caris Mirror Laboratory. Mirrors are polished to 25 nanometer accuracy.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner contributing to the international construction effort and scientific program.

Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Founding consortium partner through the McDonald Observatory. Dr. Taft Armandroff serves/served as Board Chair. Daniel T. Jaffe named President in January 2026. UT Austin leads GMTNIRS instrument development.

15São Paulo Research Foundation (FAPESP) / Brazil
Strategic tierCoreTypeStrategic or Co-development PartnerAnnounced on2015-01-01
Description

Brazilian founding partner providing data connection to the telescope from Chile and ensuring Brazilian astronomical community participation in science collaborations including Rubin Observatory and GMT.

giantmagellan.org
Strategic tierCoreTypeStrategic or Co-development Partner
Description

NSF is being asked to become a consortium member to keep America globally competitive in space science. NSF's external evaluation panel expressed confidence in GMT's path to completion. NSF budget requests to Congress for GMT final design phase funding represent a major milestone. Federal support could bring construction from 40% to 90% completion within two years.

Strategic tierMinorTypeStrategic or Co-development Partner
Description

Manufacturing partner in Rockford, Illinois that built America's largest precision gantry mill to build and assemble the telescope mount. Completed construction of a new manufacturing facility for the mount in 2022.

Strategic tierMinorTypeStrategic or Co-development Partner
Description

Italian fabrication and testing facility testing the opening and closing mechanisms on the first of 7 mirror covers for the telescope's primary mirrors.

Strategic tierMinorTypeStrategic or Co-development Partner
Description

Partnering with Ingersoll Machine Tools on fabrication of the 39-meter-tall precision moving telescope mount structure across multiple U.S. states.

20Italian National Astrophysical Institute (INAF)
Strategic tierMinorTypeStrategic or Co-development Partner
Description

Collaborating with GMT, Center for Astrophysics | Harvard & Smithsonian, and University of Arizona on testbeds to validate the wavefront-control strategy for optical performance and adaptive optics.

giantmagellan.org
Strategic tierMinorTypeStrategic or Co-development Partner
Description

Crafted the seven red camera lenses for the G-CLEF Large Earth Finder instrument, completed in 2021. Lens components are being assembled at the Harvard Smithsonian Center for Astrophysics.

Strategic tierMinorTypeStrategic or Co-development Partner
Description

Fabricated carbon-fiber-reinforced polymer optical bench components for the G-CLEF spectrograph, the same material used on the Hubble Space Telescope and James Webb Space Telescope.

Strategic tierMinorTypeStrategic or Co-development Partner
Description

Manufacturing the vacuum chamber for the G-CLEF instrument at their facility in Clearfield, Utah, providing an ultra-stable thermal environment for the spectrograph.

24U.S. Extremely Large Telescope Program (US-ELTP)
Strategic tierCoreTypeStrategic or Co-development Partner
Description

The US-ELTP is a program of NSF's NOIRLab comprising GMT and TMT, providing full-sky coverage for U.S. astronomers. GMT is a core partner alongside the Thirty Meter Telescope. Named top priority in National Academies' Astro2020 Decadal Survey.

giantmagellan.org
25Vera C. Rubin Observatory
Strategic tierCoreTypeStrategic or Co-development Partner
Description

Located less than 80 miles from GMT summit in Chile. GMT will provide spectroscopic follow-up of discoveries from Rubin's LSST survey. Rubin is a discovery engine identifying objects that have moved or changed brightness for GMT to study in detail.

giantmagellan.org
Strategic tierCoreTypeStrategic or Co-development Partner
Description

GMT complements JWST by providing optical wavelength sensitivity and extreme imaging resolution (4-16x sharper) to JWST's infrared capabilities. GMT's visible spectrum coverage is critical for detecting 'false positives' from molecular combinations that can only be produced by organic life.

27Atacama Large Millimeter/submillimeter Array (ALMA)
Strategic tierCoreTypeStrategic or Co-development Partner
Description

Located in Chile, same region as GMT. ALMA and GMT provide complementary observations: ALMA maps cold gas of circumstellar disks while GMTNIRS spectrograph is sensitive to warm gas species, enabling comprehensive planet formation studies.

giantmagellan.org
Strategic tierCoreTypeStrategic or Co-development Partner
Description

GMT will play a leading role in follow-up of gravitational wave sources detected by LIGO's global network. High-resolution spectroscopy from GMT will study electromagnetic counterparts of neutron star mergers and black hole mergers detected by LIGO.

Strategic tierCoreTypeStrategic or Co-development Partner
Description

Partner within the US-ELTP providing northern hemisphere complement to GMT's southern hemisphere coverage. Together they provide full-sky coverage for U.S. astronomers.

30European Extremely Large Telescope (E-ELT)
Strategic tierCoreTypeStrategic or Co-development Partner
Description

Located in Chile's Atacama Desert, the E-ELT is 39m and 60% complete. GMT and E-ELT are highly complementary: GMT offers wider field and bluer wavelength coverage (UV to 320nm vs 400-450nm), while E-ELT offers more mid-infrared instruments and larger diameter.

giantmagellan.org
Strategic tierMinorTypeStrategic or Co-development Partner
Description

International astronomical observatories joining forces to protect Chile's dark skies. GMT participates in this initiative to preserve the astronomical conditions that make the Las Campanas site ideal for observations.

Recent move7 records

Each record includes

Date, Type, Title, Description, Source

Expansion highlight6 records

Each record includes

Type, Description

Market position
Weaknesses5 records

Each record includes

Headline, Details, Source

Competitive moat6 records

Each record includes

Type, Details

Customer concentration

Classification, Details

Named customers2 records

Each record includes

Name, Industry, Type, Use case, Source, UUID

Segment1 record

Each record includes

Title, Type, Primary, Description, Pain point addressed, Use case, Source

Ideal customer profile2 records

Each record includes

Profile, Firmographic size, Sales motion, Sales cycle length, Buying structure, Purchase trigger, Buyer persona, Geography, Industry vertical, Primary use case, Description, Pain points, Evidence proof points, Target buyer

Technology focused
Yes
API detail
Has APIbool
No

Docs URL, Description

AI maturity
App detail

Has app

Feature9 records

Each record includes

Title, Differentiator, Description, Source

Core technology
Revenue estimate
Valuation estimate
Number of profiles
Profiles9 records

Each record includes

Name, Designation, Designation category, Overview, Profile commentary, Source

No data
No data
Funding overview

Funding stage, Last funding date, Total funding USD

Funding rounds

Each record includes

Round, Amount USD, Date, Pre money valuation, Total investors, Investors, News

Investors

Each record includes

Name, Type, Date of entry, Rounds participated, Website

Funding detail is available on the Subscription and Enterprise plan.Contact sales →

M&A

Each record includes

Name, Acquisition type, Announced date, Completed date, Status, Website, News

Investment

Each record includes

Name, Round, Announced date, Lead investor, Website, News

M&A and investment is available on the Subscription and Enterprise plan.Contact sales →

Giant Magellan Telescope

Ground-based Astronomical Observatorygiantmagellan.org

The Giant Magellan Telescope is a U.S. nonprofit-led international project constructing a 25.4-meter ground-based extremely large telescope in Chile's Atacama Desert, operated by a 16-member university consortium to provide astronomers with next-generation observational capabilities for exoplanet research and cosmology.

What Giant Magellan Telescope does

The Giant Magellan Telescope (GMT) is a ground-based astronomical research facility being constructed by GMTO Corporation, a U.S. nonprofit entity headquartered in Pasadena, California, and operated as an international scientific endeavor led by a consortium of 16 universities and research institutions spanning the United States, Chile, Australia, Brazil, Israel, South Korea, and Taiwan. The facility is being built at Las Campanas Observatory in Chile's Atacama Desert and is currently 40% complete, with first light projected around 2029. Its primary purpose is to provide next-generation observational capability to astronomers for studies including exoplanet detection and atmospheric biosignature characterization, galaxy formation and evolution, dark matter and dark energy research, and first-light observations of the early universe.

The telescope's core technology is a 25.4-meter effective aperture formed by seven 8.4-meter off-axis primary mirror segments (polished to 25-nanometer surface accuracy), employing a Gregorian optical design with seven deformable secondary mirrors that reshape up to 2,000 times per second to counteract atmospheric turbulence. The first-generation instrument suite includes the G-CLEF visible echelle spectrograph (the only high-resolution visible spectrograph planned for the first decade of any ELT), the GMTNIRS near-infrared echelle spectrograph, the GMTIFS integral field spectrograph, the GMag AO-X extreme adaptive optics coronagraph for direct Earth-like exoplanet imaging, and the MANIFEST multi-object fiber positioning system. The architecture delivers imaging 4-16x sharper than JWST from the ground, a 13x larger wide-field field of view than competing ELTs, and instruments up to 27x more compact than alternative ELT designs.

GMT's business model is a nonprofit consortium structure in which member institutions contribute capital and receive observing time proportional to their investment. To date, $1 billion in private funding has been secured (65% from U.S. institutions), supplemented by a $500M commitment from 11 founding partners in 2015, a $205M private raise in August 2022, and a $15M NSF grant in 2020, against a total $2.6 billion project value. The organization is actively pursuing National Science Foundation consortium membership following its June 2025 Final Design Phase advancement, which could accelerate construction from 40% to 90% completion within two years. Access for U.S. astronomers is also planned through the federally-funded US Extremely Large Telescope Program (US-ELTP), with philanthropic donations supplementing capital funding under the GMTO Corporation's 501(c)-equivalent nonprofit status.

Giant Magellan Telescope firmographics

Firmographics
Name
Giant Magellan Telescope
Legal name
GMTO Corporation
Website
https://giantmagellan.org
Company type
Private
Founded year
2015
Operating status
Operating
Headcount range
51–100 employees
Short description
The Giant Magellan Telescope is a U.S. nonprofit-led international project constructing a 25.4-meter ground-based extremely large telescope in Chile's Atacama Desert, operated by a 16-member university consortium to provide astronomers with next-generation observational capabilities for exoplanet research and cosmology.
Ownership category
akta.pro rank

Where Giant Magellan Telescope is headquartered

Location

Headquarters

HQ city
Pasadena
HQ country
United States
HQ region
North America

Offices3 records

Markets served

Giant Magellan Telescope business model

Business model
GTM type
B2B
Offering type
Services
Cost components
Technology or R&D, Infrastructure, Personnel, Operations, Supply Chain

Revenue model

  1. Consortium Membership Contributions: International consortium of 16 universities and research institutions fund the construction and operation of the telescope through membership contributions. The project is backed by $1 billion in private funding, with 65% coming from U.S. institutions and investors. An additional ~$500M was committed by the original 11 founding international partners at the start of construction.
  2. National Science Foundation Funding: Federal funding from the National Science Foundation (NSF) as a prospective consortium member. NSF budget requests to Congress advancing the telescope represent a major potential revenue stream. NSF support could bring the telescope from 40% to 90% completion within two years.
  3. Philanthropic Donations: Philanthropic giving from individuals and foundations supporting the telescope project. The GMTO Corporation is a nonprofit entity that accepts charitable contributions.

Go-to-market motion1 record

Distribution channels2 records

Marketing channels7 records

Giant Magellan Telescope product offering

Product offering

Core offering

GMTO Corporation is constructing the Giant Magellan Telescope, a 25.4-meter effective aperture ground-based extremely large telescope at Las Campanas Observatory in Chile's Atacama Desert, on behalf of an international consortium of 16 universities and research institutions. Once operational, the telescope will deliver astronomical observation capabilities to consortium members and U.S. astronomers through the US Extremely Large Telescope Program, supporting research in exoplanet detection, early-universe cosmology, dark matter, and spectroscopy.

Differentiator

Problem solved

Functional benefit

Products and services

  • Giant Magellan Telescope (GMT) A 25.4-meter effective aperture ground-based extremely large telescope under construction at Las Campanas Observatory in Chile's Atacama Desert. Will deliver astronomical observation services to consortium member institutions and U.S. astronomers for research in exoplanet detection, early-universe cosmology, dark matter, and spectroscopy.
  • GMTNIRS Near-Infrared Echelle Spectrograph Single-object near-infrared to mid-infrared echelle spectrograph providing simultaneous coverage of full JHKLM bands with spectral resolutions of 65,000 (JHK) and 85,000 (LM) across a 1.1-5.4 micrometer wavelength range. Used by astronomers for detailed spectroscopic studies of celestial objects.

Quantifiable outcome

  • 200x more powerful than today's best telescopes
  • +5 more outcomes

Companies that use Giant Magellan Telescope

Customer profile

Named customers2 records

Segments1 record

Ideal customer profiles2 records

Giant Magellan Telescope technology and API

Technology

Technology focussed Yes

API detail

Has API
No
API docs
API detail

Core technology

AI maturity

App detail

Feature9 records

Giant Magellan Telescope partnerships and signals

Strategic signal

Partnerships

31 partnerships are on record, tiered core and minor.

  • Gobierno Regional de Coquimbo (Chile)coreStrategic or Co-development Partner · 1 April 2026Strategic partnership signed in April 2026 to strengthen the astronomy industry in Chile's Coquimbo region, supporting the local astronomical ecosystem around the telescope.
  • Massachusetts Institute of Technology (MIT)coreStrategic or Co-development Partner · 1 September 2025Joined the international consortium in September 2025 as its newest partner, expanding the American university consortium supporting the telescope.
  • Northwestern UniversitycoreStrategic or Co-development Partner · 1 December 2024Joined the international consortium in December 2024. Northwestern's CIERA center and Dr. Vicky Kalogera contribute expertise in multi-messenger astronomy and gravitational wave follow-up.
  • Taiwan (National Science and Technology Council)coreStrategic or Co-development Partner · 1 February 2024Joined the consortium in February 2024 as a new partner, expanding global scientific impact and bringing Taiwan's astronomical community into the GMT program.
  • Astronomy Australia Ltd.coreStrategic or Co-development Partner · 1 January 2015Founding consortium partner from Australia. Contributed to the $500M founding commitment in 2015 and participates in telescope construction, mirror development, and scientific instrument programs.
  • Australian National UniversitycoreStrategic or Co-development Partner · 1 January 2015Key founding partner developing the GMTIFS (Integral Field Spectrograph). ANU's Research School of Astronomy & Astrophysics contributes to the instrument suite and scientific program.
  • Carnegie Institution for SciencecoreStrategic or Co-development Partner · 1 January 2015Founding consortium partner providing the Las Campanas Observatory site in Chile where the telescope will be constructed and operated. Host institution for the project.
  • Harvard UniversitycoreStrategic or Co-development Partner · 1 January 2015Founding consortium partner through the Center for Astrophysics | Harvard & Smithsonian. Leads development of the G-CLEF (Large Earth Finder) first-light instrument. Dr. Andrew Szentgyorgyi is the principal investigator.
  • Smithsonian InstitutioncoreStrategic or Co-development Partner · 1 January 2015Joint founding partner with Harvard University through the Center for Astrophysics. Contributes to G-CLEF development and the GMACS instrument program.
  • Korea Astronomy and Space Science Institute (KASI)coreStrategic or Co-development Partner · 1 January 2015Founding consortium partner from South Korea. Increased investment announced in July 2026. Actively involved in synergies with ALMA, Rubin Observatory, and NASA's SPHEREx Telescope.
  • Texas A&M UniversitycoreStrategic or Co-development Partner · 1 January 2015Founding consortium partner. Worked on cleaning, assembling, and testing the support actuators for the primary mirror support system at the University of Arizona Mirror Lab.
  • University of ArizonacoreStrategic or Co-development Partner · 1 January 2015Founding consortium partner responsible for manufacturing all seven 8.4-meter primary mirrors at the Richard F. Caris Mirror Laboratory. Mirrors are polished to 25 nanometer accuracy.
  • University of ChicagocoreStrategic or Co-development Partner · 1 January 2015Founding consortium partner contributing to the international construction effort and scientific program.
  • University of Texas at AustincoreStrategic or Co-development Partner · 1 January 2015Founding consortium partner through the McDonald Observatory. Dr. Taft Armandroff serves/served as Board Chair. Daniel T. Jaffe named President in January 2026. UT Austin leads GMTNIRS instrument development.
  • São Paulo Research Foundation (FAPESP) / BrazilcoreStrategic or Co-development Partner · 1 January 2015Brazilian founding partner providing data connection to the telescope from Chile and ensuring Brazilian astronomical community participation in science collaborations including Rubin Observatory and GMT.
  • National Science Foundation (NSF)coreStrategic or Co-development PartnerNSF is being asked to become a consortium member to keep America globally competitive in space science. NSF's external evaluation panel expressed confidence in GMT's path to completion. NSF budget requests to Congress for GMT final design phase funding represent a major milestone. Federal support could bring construction from 40% to 90% completion within two years.
  • Ingersoll Machine Tools Inc.minorStrategic or Co-development PartnerManufacturing partner in Rockford, Illinois that built America's largest precision gantry mill to build and assemble the telescope mount. Completed construction of a new manufacturing facility for the mount in 2022.
  • OHB Italia SpAminorStrategic or Co-development PartnerItalian fabrication and testing facility testing the opening and closing mechanisms on the first of 7 mirror covers for the telescope's primary mirrors.
  • OHB Digital ConnectminorStrategic or Co-development PartnerPartnering with Ingersoll Machine Tools on fabrication of the 39-meter-tall precision moving telescope mount structure across multiple U.S. states.
  • Italian National Astrophysical Institute (INAF)minorStrategic or Co-development PartnerCollaborating with GMT, Center for Astrophysics | Harvard & Smithsonian, and University of Arizona on testbeds to validate the wavefront-control strategy for optical performance and adaptive optics.
  • NikonminorStrategic or Co-development PartnerCrafted the seven red camera lenses for the G-CLEF Large Earth Finder instrument, completed in 2021. Lens components are being assembled at the Harvard Smithsonian Center for Astrophysics.
  • Northrop Grumman Innovation SystemsminorStrategic or Co-development PartnerFabricated carbon-fiber-reinforced polymer optical bench components for the G-CLEF spectrograph, the same material used on the Hubble Space Telescope and James Webb Space Telescope.
  • Redline Chambers, Inc.minorStrategic or Co-development PartnerManufacturing the vacuum chamber for the G-CLEF instrument at their facility in Clearfield, Utah, providing an ultra-stable thermal environment for the spectrograph.
  • U.S. Extremely Large Telescope Program (US-ELTP)coreStrategic or Co-development PartnerThe US-ELTP is a program of NSF's NOIRLab comprising GMT and TMT, providing full-sky coverage for U.S. astronomers. GMT is a core partner alongside the Thirty Meter Telescope. Named top priority in National Academies' Astro2020 Decadal Survey.
  • Vera C. Rubin ObservatorycoreStrategic or Co-development PartnerLocated less than 80 miles from GMT summit in Chile. GMT will provide spectroscopic follow-up of discoveries from Rubin's LSST survey. Rubin is a discovery engine identifying objects that have moved or changed brightness for GMT to study in detail.
  • James Webb Space Telescope (JWST)coreStrategic or Co-development PartnerGMT complements JWST by providing optical wavelength sensitivity and extreme imaging resolution (4-16x sharper) to JWST's infrared capabilities. GMT's visible spectrum coverage is critical for detecting 'false positives' from molecular combinations that can only be produced by organic life.
  • Atacama Large Millimeter/submillimeter Array (ALMA)coreStrategic or Co-development PartnerLocated in Chile, same region as GMT. ALMA and GMT provide complementary observations: ALMA maps cold gas of circumstellar disks while GMTNIRS spectrograph is sensitive to warm gas species, enabling comprehensive planet formation studies.
  • Laser Interferometer Gravitational-Wave Observatory (LIGO)coreStrategic or Co-development PartnerGMT will play a leading role in follow-up of gravitational wave sources detected by LIGO's global network. High-resolution spectroscopy from GMT will study electromagnetic counterparts of neutron star mergers and black hole mergers detected by LIGO.
  • Thirty Meter Telescope (TMT)coreStrategic or Co-development PartnerPartner within the US-ELTP providing northern hemisphere complement to GMT's southern hemisphere coverage. Together they provide full-sky coverage for U.S. astronomers.
  • European Extremely Large Telescope (E-ELT)coreStrategic or Co-development PartnerLocated in Chile's Atacama Desert, the E-ELT is 39m and 60% complete. GMT and E-ELT are highly complementary: GMT offers wider field and bluer wavelength coverage (UV to 320nm vs 400-450nm), while E-ELT offers more mid-infrared instruments and larger diameter.
  • Dark Skies CouncilminorStrategic or Co-development PartnerInternational astronomical observatories joining forces to protect Chile's dark skies. GMT participates in this initiative to preserve the astronomical conditions that make the Las Campanas site ideal for observations.

Scale indicators11 records

Recent moves7 records

Expansion highlights6 records

Giant Magellan Telescope competitors and assessment

Company assessment

Market position

Weaknesses5 records

Competitive moat6 records

Customer concentration

Giant Magellan Telescope social profiles

Digital presence

Giant Magellan Telescope financial estimates

Financial estimate

Revenue estimate

Valuation estimate

Giant Magellan Telescope leadership team

Management profile

Number of profiles

Profiles9 records

Giant Magellan Telescope funding detail

Funding detail

Funding overview

Funding rounds

Investors

Funding detail is available on the Subscription and Enterprise plan.Contact sales →

Giant Magellan Telescope M&A and investment

M&A and investment

M&A

Investments

M&A and investment is available on the Subscription and Enterprise plan.Contact sales →

Frequently asked questions about Giant Magellan Telescope

What does Giant Magellan Telescope do?

GMTO Corporation is constructing the Giant Magellan Telescope, a 25.4-meter effective aperture ground-based extremely large telescope at Las Campanas Observatory in Chile's Atacama Desert, on behalf of an international consortium of 16 universities and research institutions. Once operational, the telescope will deliver astronomical observation capabilities to consortium members and U.S. astronomers through the US Extremely Large Telescope Program, supporting research in exoplanet detection, early-universe cosmology, dark matter, and spectroscopy.

Is Giant Magellan Telescope a public or private company?

Giant Magellan Telescope is a private company. It is classified as nonprofit foundation owned and is currently operating.

When was Giant Magellan Telescope founded?

Giant Magellan Telescope was founded in 2015. It employs 51 to 100 people.

Where is Giant Magellan Telescope based?

Giant Magellan Telescope is headquartered in Pasadena, United States, in the North America region.

How does Giant Magellan Telescope make money?

Three revenue lines are on record. Consortium Membership Contributions are the primary driver. The others are national Science Foundation Funding and philanthropic Donations.

Does Giant Magellan Telescope have an API?

No public API is recorded for Giant Magellan Telescope.

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FOX 7 AustinWorld's most powerful telescope being built in Chile has Texas tiesThe Giant Magellan Telescope, being built in Chile, will be the world's largest optical-infrared telescope, completed in the 2030s. It will be nearly 80 feet in diameter, up to 200 times more powerful than existing telescopes, with UT Austin and Texas A&M involved. The telescope aims to study exoplanet atmospheres for signs of life.GlobeNewswireMIT Joins Giant Magellan Telescope International ConsortiumMIT joined the international consortium building the $2.6 billion Giant Magellan Telescope in Chile, becoming the 16th member and 10th U.S. partner. The consortium has invested $1 billion and the telescope is 40% under construction. MIT's participation strengthens U.S. leadership in astronomy, with completion expected in the 2030s.GlobeNewswireGiant Magellan Telescope Advances to National Science Foundation Final Design PhaseThe Giant Magellan Telescope received NSF approval to advance to its Final Design Phase, a step before federal construction funding. The project, backed by nearly $1 billion in private funding, is 40% under construction with components built across 36 U.S. states. The telescope is scheduled for completion in the 2030s.GlobeNewswireNorthwestern University Joins Giant Magellan Telescope International ConsortiumNorthwestern University joined the Giant Magellan Telescope consortium, becoming the 9th American institution to invest. The $2.54 billion observatory will be operational in Chile by the early 2030s. Northwestern researchers will apply AI tools to enhance the telescope's capabilities.GlobeNewswireGiant Magellan Telescope Begins Primary Mirror Support System TestingThe Giant Magellan Telescope successfully integrated a completed 8.4-meter primary mirror into a support system prototype at the University of Arizona's Mirror Lab. The six-month optical testing phase will validate the system's precision control, with production of all seven mirror cells planned for 2027. The telescope is 40% under construction and expected to be operational in Chile by the early 2030s.GlobeNewswireGiant Magellan Telescope Launches UniversoThe Giant Magellan Telescope launched Universo Expansivo, an education program for students with vision loss, featuring tactile astronomy kits and lesson plans. Developed with partners in Chile and the U.S., it was piloted with over 100 participants and is now available for free use.GlobeNewswireGiant Magellan Telescope Mount Fabrication BeginsIngersoll Machine Tools began manufacturing the Giant Magellan Telescope's 39-meter mount, weighing 2,100 metric tons. The steel structure will be assembled in Rockford, Illinois, then shipped to Chile for reassembly. The telescope is expected to be operational by the early 2030s.GlobeNewswireGiant Magellan Telescope Enclosure Ready for ConstructionThe Giant Magellan Telescope's enclosure passed its final design review and is ready for construction in Chile. The 65-meter-tall structure, weighing over 5,000 metric tons, will house the telescope and is 40% under construction. The telescope is on track to be operational by the early 2030s.GlobeNewswireGiant Magellan Telescope Expands Global Science Impact withAcademia Sinica Institute of Astronomy and Astrophysics (ASIAA) joined the Giant Magellan Telescope consortium, expanding it to 14 international institutions. ASIAA will contribute expertise in detector electronics and precision laser cutting, with construction progressing in Chile and the US. The telescope is expected to be completed in the early 2030s.GlobeNewswireGiant Magellan Telescope Expands Global Science Impact withThe Giant Magellan Telescope welcomed Academia Sinica Institute of Astronomy and Astrophysics (ASIAA) into its international consortium, expanding it to 14 institutions. ASIAA will contribute expertise in detector electronics and precision laser cutting, with construction progressing in Chile and the US. The telescope is expected to be completed in the early 2030s.