Sarah Greenstreet, Zhuofu Li, Dmitrii Vavilov, Devanshi Singh, Mario Jurić, Željko Ivezić, Siegfried Eggl, Alec Koumjian, Joachim Moeyens, V. Carruba, Maria Womack, Mikael Granvik, A. Alexov, P. Antilogus, B̌rian J. Baumanć, Eric C. Bellm, Alexandre Boucaud, Andrew Bradshaw, Jeffrey L. Carlin, Hsin‐Fang Chiang, Philip N. Daly, Felipe Daruich, Guillaume Daubard, Erik Dennihy, Stephanie Jh Deppe, H. Drass, É. Gangler, L. Le Guillou, L. P. Guy, Patrick A. Hascall, Patrick Ingraham, M. James Jee, Tim Jenness, S. M. Kahn, Arun Kannawadi, L. S. Kelvin, Jacob A. Kurlander, Didier Laporte, Nate B. Lust, Mostafa Lutfi, Lauren A. MacArthur, G Mainetti, Moniez Marc, A. A. Plazas, David Jiménez Mejías, F. Menanteau, David Mills, William O’Mullane, Angelo Fausti Neto, J. Neveu, Erfan Nourbakhsh, HyeYun Park, Maria T. Patterson, J. R. Peterson, Bruno Quint, Tiago Ribeiro, Stephen T. Ridgway, Wouter van Reeven, Jacques Sebag, Nima Sedaghat, Richard A. Shaw, Alan L. Strauss, Krzysztof Suberlak, Ian Sullivan, J. Swinbank, Sandrine Thomas, Adam Thornton, W. M. Wood-Vasey, C. W. Walter, Charlotte Ward, Beth Willman
Abstract We present lightcurves, rotation periods, and colors for the first asteroid discoveries made with the NSF-DOE Vera C. Rubin Observatory. These are the first science results derived from the 2103 asteroid discoveries released as part of the Rubin First Look (RFL) media event on 2025 June 23, in which the first LSST Camera commissioning images were released. The ∼340,000 observations in which the discoveries were made span nine nights between 2025 April 21 and May 5. With a limiting single-epoch 5 σ depth of ∼23–25 mag and dense temporal sampling under an irregular, commissioning-driven cadence, the RFL observations provide an ideal test bed for determination of rotation periods, including sensitivity to rapid rotation. We model lightcurves and derive rotation periods and colors for the ∼2000 objects. We find 75 main-belt asteroids (MBAs) and one near-Earth object (NEO) with reliable rotation periods spanning 0.031–21.3 hr and a photometric precision in the range of 0.05–0.15 mag. We find 19 superfast rotators with periods shorter than the 2.2 hr spin barrier. Rubin-discovered MBA 2025 MN 45 is the fastest-rotating d > 0.5 km known asteroid with a rotation period of 1.9 minutes; along with NEO 2025 MJ 71 (1.9 minutes) and Rubin-discovered MBAs 2025 MK 41 (3.8 minutes), 2025 MV 71 (13 minutes), and 2025 MG 56 (16 minutes), these five super- to ultrafast rotators join a couple of NEOs as the fastest-spinning subkilometer asteroids known. As this study demonstrates, even in early commissioning, Rubin is successfully probing a previously sparsely sampled region of the subkilometer size−spin rate regime for MBAs.