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Vehicle: Angara 1.2 | Antares 330 | Ariane 62 | Ariane 64 | Ariane 64 Block 2 | Astra Rocket 4 | Atlas V 551 | Electron | Falcon 9 Block 5 | Falcon Heavy | Firefly Alpha Block 2 | H3-24 | H3-30 | HANBIT-Nano | KSLV-2 Nuri | Launch Vehicle Mark-3 (GSLV Mk III) | Long March 10B | Long March 12B | Long March 2D | Long March 2F/G | Long March 6 | Long March 7A | Nebula-1 | Neutron | New Glenn | Pegasus XL | RFA One | South Korean ADD Solid-Fuel SLV | Soyuz 2.1a | Soyuz 2.1b | Soyuz-5 | Spectrum | Starship V3 | Themis Demonstrator | Vega-C | Vulcan VC4L | Zhuque-2E

Orbit: Elliptical Orbit | Geostationary Transfer Orbit | Low Earth Orbit | Lunar Orbit | Mars Orbit | Medium Earth Orbit | Polar Orbit | Suborbital | Sun-Earth L2 | Sun-Synchronous Orbit | Unknown

Apr 2026
Month
launch status: TBD
πŸ‡¬πŸ‡« Vega-C – Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) – Avio S.p.A (Commercial) — Elliptical Orbit (Elliptical) — Astrophysics
Ariane Launch Area 1 (ELV) — Guiana Space Centre, French Guiana
Chinese Academy of Sciences πŸ‡¨πŸ‡³ (Government) , European Space Agency πŸ‡ͺπŸ‡Ί (Multinational)

Joint mission between the European Space Agency and the Chinese Academy of Sciences to investigate the interaction between Earth’s protective shield – the magnetosphere – and the supersonic solar wind.

15 Aug 2026
Day
launch status: TBD
πŸ‡³πŸ‡Ώ Electron – Aspera – Rocket Lab (Commercial) — Low Earth Orbit (LEO) — Astrophysics
Unknown Pad — Rocket Lab Launch Complex 1, Mahia Peninsula, New Zealand
National Aeronautics and Space Administration πŸ‡ΊπŸ‡Έ (Government)

Aspera houses an ultraviolet telescope and will examine hot gas in the intergalactic medium, thought to be contributing to the birth of stars and planets. Aspera will be the first NASA astrophysics mission to gather and map these ultraviolet light signatures, potentially unlocking a deeper understanding of the origins of stars, planets, and life in the universe.

Sep 2026
Month
launch status: TBD
πŸ‡ΊπŸ‡Έ Falcon Heavy – Nancy Grace Roman Space Telescope – SpaceX (Commercial) — Sun-Earth L2 (L2) — Astrophysics
Launch Complex 39A — Kennedy Space Center, FL, USA

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.