Uranus Stellar Occultation Campaign 2025
Project Concept
On April 7, 2025, Planetary scientists at NASA Langley Research Center led an international team of over 30 astronomers, using 15 professional observatories, to observe a Uranus stellar occultation event. A stellar occultation occurs when a planet such as Uranus passes in front of, or occults, a distant star. Observations of special alignments of Uranus and a bright star like that on April 7, 2025 are used by scientists to study the temperature and density of the upper atmosphere of Uranus in detail, which is a key step toward preparing future missions to the planet.
At the beginning of a stellar occultation, starlight reaching the observers on Earth is gradually dimmed by the atmosphere of Uranus; the process reverses at the end of the occultation and the starlight brightens when it is no longer obstructed by Uranus. The animation below illustrates this process. Detailed measurements of the dimming over time allows scientists to determine the properties of the atmosphere of Uranus. Specifically, we use the April 7 stellar occultation to measure temperature, density, and pressure at many different altitudes in the upper atmosphere of Uranus, which allow examining how the planet has changed in the past three decades and how its atmosphere functions today. These measurements help enable a future mission to Uranus that includes dropping a probe into the planet’s atmosphere.
This campaign was supported by the Planetary Science Division's Solar System Observations program within NASA's Science Mission Directorate.
Observatories and Telescopes Involved
- McDonald Observatory: Struve Telescope (Texas)
- Lowell Discovery Telescope (Arizona)
- NASA Infrared Telescope Facility (Hawaii)
- Large Binocular Telescope (Arizona)
- Apache Point Observatory: ARC Telescope (New Mexico)
- Steward Observatory: Bok Telescope (Arizona)
- MMT (Arizona)
- Io Input/Output Observatory (Arizona)
- Bruneau Dunes Observatory (Idaho)
- Centennial Observatory (Idaho)
- Apache Point Observatory: NMSU 1-meter Telescope (New Mexico)
- Tortugas Mountain Observatory (New Mexico)
- Michael Skrutskie Telescope (Colorado)
- San Pedro Martir National Astronomical Observatory (Baja California, Mexico)
- Universidad Autonoma De Nuevo Leon: Observatorio Astronómico Universitario (Nuevo Leon, Mexico)
- University of Idaho Telescope
- McDonald Observatory: Chow Telescope (Texas)
- Apache Point Observatory: ARCSAT (New Mexico)
Team Members
Principal Investigator
- Kunio Sayanagi, NASA Langley Research Center
Science Principal Investigator & Analysis Lead
- William Saunders, NASA Langley Research Center, Analytical Mechanics Associates
Team members (organized alphabetically by institution)
- Matthew Lehner, Academia Sinica Institute of Astronomy and Astrophysics, Taiwan
- Zhi-Wei Zhang, Academia Sinica Institute of Astronomy and Astrophysics, Taiwan
- Jack Dembicky, Apache Point Observatory & New Mexico State University
- Brian Jackson, Boise State University
- Hailey Stubbers, Boise State University
- Emma Dahl, Caltech
- Geoffrey Blake, Caltech
- James Dull, College of Idaho
- Chris Anderson, College of Southern Idaho
- Brian McLeod, Harvard-Smithsonian Center for Astrophysics
- Gregory Harmon, Idaho Department of Parks and Recreation
- Stephen Levine, Lowell Observatory
- Katie Breeland-Newcomb, Lowell Observatory
- Michael J. Person, MIT
- Joel Castro-Chacón, National Autonomous University of Mexico
- Nancy Chanover, New Mexico State University
- Mark Croom, New Mexico State University
- Jason Jackiewicz, New Mexico State University
- Damya Souami, Paris Observatory
- Jeffrey P. Morgenthaler, Planetary Science Institute
- Leslie Young, Southwest Research Institute
- Erika Cook, Texas A&M University
- Darren DePoy, Texas A&M University
- Ryan Oelkers, The University of Texas Rio Grande Valley
- Donald W. McCarthy Jr., University of Arizona
- Bill Hubbard, University of Arizona
- Craig Kulesa, University of Arizona
- Matthew Hedman, University of Idaho
- Stephen C. Hummel, University of Texas at Austin & McDonald Observatory
- Mike Skrutskie, University of Virginia
- Anne Verbiscer, University of Virginia
- Richard G. French, Wellesley University & Space Science Institute
- Luke Schmidt, Yerkes Observatory
2025 Observatories Map
Map showing the locations of observatories utilized in the April 7, 2025 Uranus Stellar Occultation.
2024 Campaign
Observatories and telescopes involved in the November 12, 2024 Uranus occultation campaign
- Devasthal Optical Telescope
- Himalayan Chandra Observatory
- Hokkaido University Observatory
- Kyoto Sangyo University Observatory
- Thai National Observatory
Team Members (India)
- Principle Investigators:
- Damya Souami, LIRA, CNRS, Paris Observatory
- Richard G. French, Wellesley University & Space Science Institute
- Team Members:
- Anandmayee Tej, Indian Institute of Space Science and Technology, India
- Saurabh Sharma and Tarak Chand, Aryabhatta Institute of Observational Sciences, India
- Joe Ninan, Devendra Ojha, and Pramod Kumar, Indian Institute of Astrophysics, India
- NM Ashok, Physical Research Laboratory, India
Team Members (Thailand)
- Puji Irawati, Saran Poshyachinda, Supachai Awiphan, Somsawat Rattanasoon, Orarik Tasuya, Thail National Observatory & National Astronomical Research Institute of Thailand
Team Members (Japan)
- Seiko Takagi, Kotaro Amada, Hokkaido University
- Hideo Sagawa, Kyoto Sangyo University
- Jun Kimura, Osaka University