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The Nancy Grace Roman Space Telescope is a NASA infrared space telescope with a 2.4 m (7.9 ft) wide field of view primary mirror and two scientific instruments. The Wide-Field Instrument (WFI) is a 300.8-megapixel multi-band visible and near-infrared camera, providing a sharpness of images comparable to that achieved by the Hubble Space Telescope over a 0.28 square degree field of view, 100 times larger than imaging cameras on the Hubble. The Coronagraphic Instrument (CGI) is a high-contrast, small field of view camera and spectrometer covering visible and near-infrared wavelengths using novel starlight-suppression technology. Roman objectives include a search for extra-solar planets using gravitational microlensing, and probing the expansion history of the Universe and the growth of cosmic structure, with the goal of measuring the effects of dark energy, the consistency of general relativity, and the curvature of spacetime.
Sun-Earth L2The Nancy Grace Roman Space Telescope is a NASA infrared space telescope with a 2.4 m (7.9 ft) wide field of view primary mirror and two scientific instruments. The Wide-Field Instrument (WFI) is a 300.8-megapixel multi-band visible and near-infrared camera, providing a sharpness of images comparable to that achieved by the Hubble Space Telescope over a 0.28 square degree field of view, 100 times larger than imaging cameras on the Hubble. The Coronagraphic Instrument (CGI) is a high-contrast, small field of view camera and spectrometer covering visible and near-infrared wavelengths using novel starlight-suppression technology. Roman objectives include a search for extra-solar planets using gravitational microlensing, and probing the expansion history of the Universe and the growth of cosmic structure, with the goal of measuring the effects of dark energy, the consistency of general relativity, and the curvature of spacetime.
Sun-Earth L2The Nancy Grace Roman Space Telescope is a NASA infrared space telescope with a 2.4 m (7.9 ft) wide field of view primary mirror and two scientific instruments. The Wide-Field Instrument (WFI) is a 300.8-megapixel multi-band visible and near-infrared camera, providing a sharpness of images comparable to that achieved by the Hubble Space Telescope over a 0.28 square degree field of view, 100 times larger than imaging cameras on the Hubble. The Coronagraphic Instrument (CGI) is a high-contrast, small field of view camera and spectrometer covering visible and near-infrared wavelengths using novel starlight-suppression technology. Roman objectives include a search for extra-solar planets using gravitational microlensing, and probing the expansion history of the Universe and the growth of cosmic structure, with the goal of measuring the effects of dark energy, the consistency of general relativity, and the curvature of spacetime.
Sun-Earth L2Demonstration flight of the Astrobotic Griffin lander and its engines, initially contracted for the cancelled NASA VIPER (Volatiles Investigating Polar Exploration Rover) mission. The vacated payload spot will now host the FLIP (FLEX Lunar Innovation Platform) lunar rover from Astrolab.
Lunar Orbit Unknown FH - Maiden Flight Unknown Unknown FH - Maiden Flight Unknown Unknown FH - Maiden Flight UnknownDemonstration flight of the Astrobotic Griffin lander and its engines, initially contracted for the cancelled NASA VIPER (Volatiles Investigating Polar Exploration Rover) mission. The vacated payload spot will now host the FLIP (FLEX Lunar Innovation Platform) lunar rover from Astrolab.
Lunar Orbit Unknown FH - Maiden Flight Unknown Unknown FH - Maiden Flight Unknown Unknown FH - Maiden Flight UnknownDemonstration flight of the Astrobotic Griffin lander and its engines, initially contracted for the cancelled NASA VIPER (Volatiles Investigating Polar Exploration Rover) mission. The vacated payload spot will now host the FLIP (FLEX Lunar Innovation Platform) lunar rover from Astrolab.
Lunar Orbit Unknown FH - Maiden Flight Unknown Unknown FH - Maiden Flight Unknown Unknown FH - Maiden Flight UnknownDragonfly is NASA's 4th New Frontiers program mission that will send a robotic rotorcraft to fly within the atmosphere of Saturn's moon Titan to sample materials and determine surface composition in different geologic settings, advancing humanity's search for the building blocks of life. The craft is a large quadcopter with double rotors with mass of about 875 kg, featuring rotors of 1.35 m in diameter. It can fly through several kilometers within an hour and will perform 1 flight per Titan day (~16 Earth days). During the planned 3.3-year mission, Dragonfly is expected to cover distance up to several hundred km. Dragonfly will use a Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) to power its instruments. The planned science instrument suite is: * DragonCam: Camera Suite * DrACO: Drill for Acquisition of Complex Organics * DraMS: Mass Spectrometer * DraGNS: Gamma-ray and Neutron Spectrometer * DraGMet: Geophysics and Meteorology
Heliocentric N/ADragonfly is NASA's 4th New Frontiers program mission that will send a robotic rotorcraft to fly within the atmosphere of Saturn's moon Titan to sample materials and determine surface composition in different geologic settings, advancing humanity's search for the building blocks of life. The craft is a large quadcopter with double rotors with mass of about 875 kg, featuring rotors of 1.35 m in diameter. It can fly through several kilometers within an hour and will perform 1 flight per Titan day (~16 Earth days). During the planned 3.3-year mission, Dragonfly is expected to cover distance up to several hundred km. Dragonfly will use a Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) to power its instruments. The planned science instrument suite is: * DragonCam: Camera Suite * DrACO: Drill for Acquisition of Complex Organics * DraMS: Mass Spectrometer * DraGNS: Gamma-ray and Neutron Spectrometer * DraGMet: Geophysics and Meteorology
Heliocentric N/ADragonfly is NASA's 4th New Frontiers program mission that will send a robotic rotorcraft to fly within the atmosphere of Saturn's moon Titan to sample materials and determine surface composition in different geologic settings, advancing humanity's search for the building blocks of life. The craft is a large quadcopter with double rotors with mass of about 875 kg, featuring rotors of 1.35 m in diameter. It can fly through several kilometers within an hour and will perform 1 flight per Titan day (~16 Earth days). During the planned 3.3-year mission, Dragonfly is expected to cover distance up to several hundred km. Dragonfly will use a Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) to power its instruments. The planned science instrument suite is: * DragonCam: Camera Suite * DrACO: Drill for Acquisition of Complex Organics * DraMS: Mass Spectrometer * DraGNS: Gamma-ray and Neutron Spectrometer * DraGMet: Geophysics and Meteorology
Heliocentric N/AExoMars 2028 is a second mission of two-part European Space Agency astrobiology project to search for evidence of life on Mars. The primary objective is to land the rover at a site with high potential for finding well-preserved organic material, particularly from the very early history of the planet. The rover is expected to travel several kilometers during its mission. The European rover will be the first mission to combine the capability to move across the surface and to study Mars at depth. It will collect samples with a drill down to a depth of 2 m and analyze them with next-generation instruments in an onboard laboratory. Underground samples are more likely to include biomarkers, since the tenuous martian atmosphere offers little protection from radiation and photochemistry at the surface.
Heliocentric N/AExoMars 2028 is a second mission of two-part European Space Agency astrobiology project to search for evidence of life on Mars. The primary objective is to land the rover at a site with high potential for finding well-preserved organic material, particularly from the very early history of the planet. The rover is expected to travel several kilometers during its mission. The European rover will be the first mission to combine the capability to move across the surface and to study Mars at depth. It will collect samples with a drill down to a depth of 2 m and analyze them with next-generation instruments in an onboard laboratory. Underground samples are more likely to include biomarkers, since the tenuous martian atmosphere offers little protection from radiation and photochemistry at the surface.
Heliocentric N/AExoMars 2028 is a second mission of two-part European Space Agency astrobiology project to search for evidence of life on Mars. The primary objective is to land the rover at a site with high potential for finding well-preserved organic material, particularly from the very early history of the planet. The rover is expected to travel several kilometers during its mission. The European rover will be the first mission to combine the capability to move across the surface and to study Mars at depth. It will collect samples with a drill down to a depth of 2 m and analyze them with next-generation instruments in an onboard laboratory. Underground samples are more likely to include biomarkers, since the tenuous martian atmosphere offers little protection from radiation and photochemistry at the surface.
Heliocentric N/A18 Low Earth Orbit communication satellites with Ku, Q and V band payloads for the G60 constellation operated by Shanghai Spacesail Technologies with…
Thirteenth batch of satellites for a reconnaissance satellite constellation built by SpaceX and Northrop Grumman for the National Reconnaissance Offi…
Ninth cargo delivery mission to the Chinese space station.
A batch of 24 satellites for the Starlink mega-constellation - SpaceX's project for space-based Internet communication system.
Ride-share of 45 satellites including: * CAS500-2 (KASA, South Korea) The South Korean CAS500-1 and -2 satellites will image the Earth in pan-chr…