Time to launch another space telescope!

Scheduled for (UTC)	2026-08-30 11:26:04
Scheduled for (local)	2026-08-30 07:26:04 (EDT)
Launch site	LC-39A, Kennedy Space Center, Florida.
Launch vehicle	Falcon Heavy
Center	B1105-1 (expendable)
Booster	B1072-3 (LZ-2)
Booster	B1104-1 (LZ-40)
Customer	NASA
Payload	Nancy Grace Roman Space Telescope
Mass	9,174 kg
Target Orbit	Sun-Earth L2

Livestreams

Stream	Link
NASA	https://www.youtube.com/watch?v=9wq3VHsL_bE
NASASpaceflight	https://www.youtube.com/watch?v=-8yDQhVgypw
International Rocket Launches	https://www.youtube.com/watch?v=vj19LFKSaFw
Space Affairs	https://www.youtube.com/watch?v=5q6XP71_LYI
Everyday Astronaut	https://www.youtube.com/watch?v=J6Ww6kQN4Qw
Spaceflight Now	https://www.youtube.com/watch?v=Ab0UUfVN1w8
The Launch Pad	https://www.youtube.com/watch?v=Vj8tDhC1Rb0
Avid Space	https://www.youtube.com/watch?v=ZBcmBRrNqUw
SpaceX	https://x.com/SpaceX/status/2094006807245066584
The Space Devs	https://www.youtube.com/watch?v=1Hr08IfmvRo

Stats

Sourced from NextSpaceflight and r/SpaceX:

☑️ 2nd launch from LC-39A this year

☑️ 122 days, 21:13:04 turnaround for this pad

☑️ 2nd Falcon Heavy launch this year, 13th overall

☑️ 673rd and 674th Falcon recovery attempts

☑️ 209th consecutive successful Falcon 9 / FH launch (if successful)

☑️ 105th SpaceX mission this year, 715th overall (excluding Starship test flights)

☑️ 105th SpaceX launch this year, 724th overall (including Starship test flights)

Payload info:

• SpaceX mission page
• NextSpaceflight page

The Roman Space Telescope is a NASA observatory designed to settle essential questions in the areas of dark energy, exoplanets, and infrared astrophysics. The telescope has a primary mirror that is 2.4 meters in diameter (7.9 feet) and is the same size as the Hubble Space Telescope's primary mirror. The Roman Space Telescope will have two instruments: the Wide Field Instrument and the Coronagraph Instrument.

The Wide Field Instrument will have a field of view that is 100 times greater than the Hubble infrared instrument, capturing more of the sky with less observing time. As the primary instrument, the Wide Field Instrument will measure light from a billion galaxies over the course of the mission lifetime. It will perform a microlensing survey of the inner Milky Way to find ~2,600 exoplanets. The Coronagraph Instrument will perform high-contrast imaging and spectroscopy of individual nearby exoplanets.