Blue Ghost Mission 3 Adds Starcloud Computing to Its 2028 Lunar Science Plan
Firefly Aerospace says Blue Ghost Mission 3 has cleared critical design review, moving the NASA CLPS mission toward hardware for a 2028 trip to the Moon's Gruit
Updated October 26, 2026 Mission 3 Adds an Orbital Computing Experiment Blue Ghost Mission 3 now has a commercial computing payload alongside its lunar science campaign. In a September 30 announcement , Firefly said Starcloud's SC-1L processor will fly on the Elytra orbital vehicle supporting the Gruithuisen Domes landing. The mission remains targeted for launch no earlier than 2028. This is a payload agreement and a planned demonstration, not an operating lunar data center. The planned sequence separates NASA's surface delivery from the later commercial work. Elytra first transports Blue Ghost and provides a communications relay for the lander. After the surface mission, Firefly plans to keep Elytra in lunar orbit for customer payload and imaging operations. The company describes an operating design life of up to five years; that duration is a target, not flight performance already demonstrated at the Moon. What SC-1L is supposed to prove Starcloud's processor is intended to ingest data from Firefly's Solux vision system, perform AI computing onboard, and transmit processed results to Earth. Processing near the sensor could reduce the volume that must travel over a constrained lunar downlink. The announcement does not establish a deployed computing service, customer pricing, or measured lunar-orbit throughput. Those remain separate questions from whether the payload reaches orbit and completes its demonstration. Firefly also distinguishes this payload from the NVIDIA Jetson processing planned for its Ocula lunar imaging service. Ocula combines telescopes, onboard processing, and image delivery; SC-1L is a separate commercial computing experiment hosted on Elytra. Both depend on spacecraft power, thermal control, communications, and sustained orbital operations. Sharing an orbiter does not remove those engineering limits. The surface payload list is more specific now Firefly's current Gruithuisen mission page lists six NASA-sponsored payloads and more than 14 days of planned surface operations. Lunar-VISE combines lander cameras with rover-mounted infrared and multispectral imaging and gamma-ray and neutron measurements. That division matters: fixed cameras provide context while the rover samples changes across the Gamma Dome terrain. The other investigations broaden the mission beyond volcanic composition. Heimdall's four-camera system will study the landing environment and surface features. SAMPLR will demonstrate regolith collection and particle filtering with a robotic arm. ROLSES will characterize radio emissions and the near-surface radio environment. NMLS will measure neutrons to compare surface observations with orbital mapping, including signatures that could indicate hydrogen or water molecules. PILS will test next-generation solar-cell performance, charge buildup, and dust accumulation. None of those objectives should be mistaken for a discovery already made at the landing site. Production capacity has changed, but readiness still needs proof On September 22, Firefly announced completion of a new Cedar Park cleanroom four times the size of its existing one. The company says the two ISO Class 8 cleanrooms together can support assembly work on up to 12 lunar landers and orbital vehicles simultaneously. That is concurrent manufacturing capacity, not a claim that 12 finished spacecraft are ready to fly or that the factory delivers 12 vehicles each year. This gives the original design-review story a more concrete industrial follow-up. A new factory area and an added customer broaden the program, but they do not certify Mission 3 flight hardware. The next useful evidence is mission-specific integration and environmental testing, successful rover deployment testing, and demonstrated communications performance. Firefly's September 30 release places the preceding Blue Ghost Mission 2 launch no earlier than 2027, keeping the earlier mission's performance an important checkpoint for the shared architecture. The original design-review report is retained below for context. Launch dates, orbital service life, and payload operations described in this update are company plans as of October 26, 2026, not completed future events. Firefly Aerospace says Blue Ghost Mission 3 has cleared its critical design review, moving the company's next NASA lunar delivery toward hardware fabrication for a 2028 trip to the Gruithuisen Domes. The update is not just another checklist item. It is a sign that the commercial lunar program is starting to repeat, with the same basic lander line now moving from first landing, to far-side relay work, to rover-supported geology. The mission targets one of the Moon's strangest volcanic regions, a set of rounded domes thought to contain silica-rich material unlike the dark basalt plains that cover much of the near side. If Blue Ghost Mission 3 works, NASA gets a close look at a formation that has puzzled lunar scientists for decades, and Firefly gets another proof point that CLPS landers can become a regular logistics service instead of one-off stunts. Concept view of Blue Ghost Mission 3 surface operations at the Gruithuisen Domes. Credit: AI-generated illustration for Cislunar News The News: Design Locked, Hardware Next Firefly posted on May 28 that the Blue Ghost Mission 3 team had completed critical design review, the milestone that checks whether a mission's detailed design is mature enough to proceed toward fabrication, assembly, integration, and test. For a lunar lander mission, that review covers far more than the shape of the spacecraft. It examines payload accommodation, thermal margins, power, avionics, communications, trajectory, landing operations, software, fault protection, and how the lander, transfer vehicle, and rover work as a stack. The NASA task order behind the mission was awarded in December 2024 at roughly $179.6 million . Firefly's mission page describes a Blue Ghost lander paired with the Elytra Dark orbital vehicle and a rover supplied by Honeybee Robotics, now part of Blue Origin. The target is the Gruithuisen Domes region on the Moon's near side, with launch planned no earlier than 2028. That timing matters. CLPS has already moved through the painful first phase of commercial lunar delivery, where success and failure both arrived quickly. Firefly's first Blue Ghost mission landed successfully in Mare Crisium in 2025 and operated for a lunar day. Mission 2 is aimed at a more complex far-side and orbital communications profile. Mission 3 now pushes into a scientifically unusual site that needs both a stable landing platform and mobile surface work. $179.6M NASA CLPS task order value 2028 No earlier than launch target 6 NASA-sponsored payloads Why the CDR matters A critical design review does not guarantee launch or landing success. It does mean NASA and the company have enough design confidence to start turning the mission into flight hardware. For a CLPS provider, that is the point where credibility starts shifting from proposal to production. Why the Gruithuisen Domes Are Different Most people picture the Moon as a world of impact craters and dark basalt plains. The Gruithuisen Domes do not fit that simple picture. They are broad, rounded volcanic features near Sinus Viscositatis that appear to be rich in silica. On Earth, silica-rich volcanic rocks are often linked to water, plate tectonics, and complex crustal recycling. The Moon has none of that in the same way, which makes the domes a geologic problem worth visiting. Remote sensing has suggested that the domes may contain material closer to granite-like compositions than ordinary mare basalt. That raises a direct scientific question: how did such material form on a dry, one-plate body that cooled quickly compared with Earth? A rover-supported mission can measure texture, composition, and local context in ways orbital data cannot. Blue Ghost Mission 3 is expected to carry instruments tied to imaging, spectroscopy, regolith analysis, and geophysical co