
ALT Artemis II commander Reid Wiseman (left) stands next to Artemis II mission specialist Christina Koch (right) in front of the T-38 planes they used to fly to NASA's Kennedy Space Center ahead of the launch of the Artemis II mission. They are wearing blue flight suits, sunglasses, and smile at someone off-camera. Credit: NASA/Brandon Hancock

ALT Canadian Space Agency astronaut Joshua Kutryk stands beside NASA's T-38 aircraft. NASA astronaut Jessica Watkins sits in the backseat. Both wear blue flight suits. Photo: NASA/Luna Posadas Nava

ALT From left to right, NASA astronaut Jessica Watkins, Roscosmos cosmonaut Sergey Teteryatnikov, NASA astronaut Luke Delaney, and Canadian Space Agency astronaut Joshua Kutryk walk carrying green bags and wearing blue flight suits ahead of departing aboard T-38 aircraft for NASA's Kennedy Space Center. Photo: NASA/Luna Posadas Nava

ALT Pictured from left to right in this photo are NASA Administrator James D. Fletcher, DeForest Kelley (who played Dr. “Bones” McCoy in the original Star Trek series), George Takei (Mr. Sulu), James Doohan (Chief Engineer Montgomery “Scotty” Scott), Nichelle Nichols (Lt. Uhura), Leonard Nimoy (Mr. Spock), Star Trek creator Gene Rodenberry, U.S. Rep. Don Fuqua (D.-Fla) and Walter Koenig (Ensign Chekov). They are posed in front of space shuttle Enterprise during its rollout ceremony on Sept. 17, 1976.

ALT This test image captures the very first photons of starlight to reach the Wide Field Instrument on NASA’s Nancy Grace Roman Space Telescope. It was taken as an initial performance assessment with the detector array still stowed as it was for launch, far from best focus. Roman’s primary science instrument has opened its eyes to the universe for the first time, revealing a sea of out-of-focus stars, each spread out over many thousands of pixels. The image, which zooms into one detector and zooms again to a single star in the insets, offers a baseline the Roman team will work from to align the telescope’s optics and tune the focus. The team will soon activate the instrument’s fine-guidance system, which will mean Roman can lock onto targets. They’ll also focus the observatory, which will shrink each star’s light to appear as a crisp point, rather than the broad, donut-like features seen here (which appear as expected given the instrument’s present configuration).


























