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The U.S. National Science Foundation (NSF) and the U.S. Department of Energy (DOE) Office of Science will support Rubin Observatory in its operations phase to carry out the Legacy Survey of Space and Time. They will also provide support for scientific research with the data. During operations, NSF funding is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF, and DOE funding is managed by SLAC National Accelerator Laboratory (SLAC), under contract by DOE. Rubin Observatory is operated by NSF NOIRLab and SLAC.

NSF is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.

The DOE Office of Science is the single largest supporter of basic research in the physical sciences in the United States and is working to address some of the most pressing challenges of our time.

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    • Zoom to 2026 ED138 Observations
    • 2026 ED138 orbital arc (without annotations)
    • 2026 ED138 orbital arc (with annotations)
    • 2026 ED138 3D orbit (with dwarf planets)
    • 2026 ED138 3D orbit
    • 2026 ED138 orbital arc
    • Mosaic of 2026 ED138 discovery images
    • 2026 ED138 orbital pathway during May 2026
    • 2026 ED138 3D orbit (portrait)
    • 2026 ED138 3D orbit (portrait, with dwarf planets)
    • Top-down view of 2026 ED138 orbit
    • 2026 ED138 orbit in 3D
    • Top-down view of 2026 ED138 orbit (with dwarf planets)
    • 2026 ED138 orbit in 3D (with dwarf planets)
    • Zooming into the Seagull Nebula
    • Stepping into the Seagull Nebula
    • Pan on the Seagull Nebula
    • Scale Comparison of Seagull Nebula to Trifid-Lagoon
    • Seagull Nebula captured by NSF–DOE Vera C. Rubin Observatory ComCam
    • A dense field of countless pinpoint stars fills the frame against the deep black of space, creating a fine, grainy texture like fine sand spread across a smooth table. Dozens of particularly bright stars in blue, yellow, and orange glitter across the scene like jewels.

Wispy, grayish clouds of galactic dust drift across the center and right sides of the image, appearing soft and powder-like against the dark background.

Scattered throughout the entire scene are stars and faint objects in shades of blue, yellow, and red. Some appear as sharp, solid points, while others are soft, diffuse smudges. Zooming in reveals that many of these tiny, faint smudges scattered between the stars are actually distant galaxies, varying from smooth, pebble-like blobs to faint, stretched lines.
      NSF–DOE Rubin Observatory Looks Deep Into a Famous Cosmic Field
    • Pan on NSF–DOE Rubin Observatory's Image of the COSMOS Field
    • Zoom on NSF–DOE Rubin Observatory's Image of the COSMOS Field
    • Cutout from Rubin's COSMOS
    • A composite graphic titled "Rubin's COSMOS Field" features a dense central starfield marked with ten white boxes, surrounded by ten corresponding zoomed-in panels. The central view shows a sandy scatter of distant stars and faint smudges. The numbered outer panels highlight diverse galaxy structures: bright coiled spirals, smooth golden ellipticals glowing like polished stones, and distorted merging pairs with wispy, thread-like tails of stars.
      NSF–DOE Rubin Observatory Looks Deep Into a Famous Cosmic Field (selected excerpts)
    • A scale diagram of the Rubin Observatory LSST Camera field of view. A large white circle filled with a grid of small square tiles contains a wide astronomical image across its center. Inside the image, small nested wireframe boxes show the much smaller views of the Webb, Chandra, Hubble, and Spitzer telescopes. In the bottom-right corner, a full Moon image looks tiny next to the giant circle, showing how Rubin's camera covers an area much larger than the Moon.
      Footprints on COSMOS
    • Cutout from Rubin's COSMOS
    • Cutout from Rubin's COSMOS
    • Cutout from Rubin's COSMOS
    • Cutout from Rubin's COSMOS
    • Cutout from Rubin's COSMOS
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