- Hunting for the Mysterious Origins of Fast Radio Bursts28 Sep, 2020
- Girls Educating Girls 28 Sep, 2020
- Cassini Data Solves Mystery of Arecibo Radar Signals on Titan28 Sep, 2020
- How to Build an Asteroid11 Sep, 2020
- A Holistic Approach to Understanding Asteroids: Laboratory Experiments, Theoretical Models, & Radar Observations 11 Sep, 2020
- Sharing the Connection: Arecibo’s Planetary Radar & NASA’s OSIRIS-REx Mission to Bennu10 Sep, 2020
- Analyzing Gravitational Fields Around Small Bodies in Support of Future Spacecraft Missions09 Sep, 2020
- Broken Cable Damages Arecibo Observatory11 Aug, 2020
- Open Position: Research Intern06 Aug, 2020
- Recorded Session: Arecibo Observatory Virtual Town Hall30 Jul, 2020
- The Arecibo Observatory congratulates Dr. Martha P. Haynes, recipient of the Janksy Lectureship 2020! 23 Jul, 2020
- AO Adapts: Continued Workshops, Training, and Education06 Jul, 2020
- Annoucing the Arecibo Observatory Town Hall01 Jul, 2020
- AO Features: Former AO Postdoctoral Researcher Kristen Jones30 Jun, 2020
- New AO Lidar Observations of Ca+ in the Mesosphere and Thermosphere29 Jun, 2020
- Breaking Assumptions on the Excitation Temperatures in Molecular Clouds29 Jun, 2020
In the 2030’s, two spacecrafts - NASA’s Europa Clipper and the European Space Agency’s Jupiter Icy Moons Explorer (JUICE) missions - will enter orbit around Jupiter to study the planet’s largest moons. Until then, observations of the Galilean satellites - named for their discoverer - are restricted to observations from Earth.
Precise knowledge of the moons’ orbits around Jupiter is key. In a recent study published in The Astronomical Journal, scientists used radar observations from the Arecibo Observatory spanning 17 years, from 1999 - 2016, to determine the satellites’ positions and motions over time.
“Arecibo is the only facility that can do these types of observations. You need the world’s most powerful radar system to reach all the way to Jupiter,” explained Dr. Marina Brozovic, a radar scientist at the Jet Propulsion Laboratory and lead author of the publication.
“Arecibo is the only facility that can do these types of observations. You need the world’s most powerful radar system to reach all the way to Jupiter,..” - Dr. Marina Brozovic, Radar scientist at NASA's Jet Propulsion Laboratory
“We were able to obtain some very high-precision measurements of the line-of-sight positions of the Galilean satellites. Only a spacecraft can do better,” Dr. Brozovic added. The team also obtained the very first radar images of Jupiter’s volcanic moon, Io.
Radar image of Jupiter’s largest moon, Ganymede, obtained at Arecibo Observatory on Jan 31, 2015 with 10.5 km resolution.
The new, precise astrometric measurements of the moons enabled high-precision estimates of their orbits, which were described in the study. Dr. Brozovic elucidated, “We are hoping that this work will lead to a better understanding of the orbital changes that the Galilean satellites experience due to their tidal interaction with Jupiter.”
Among the co-authors of the paper are current AO analyst Ms. Luisa Zambrano-Marin and former AO staff Dr. Michael Nolan, Dr. Patrick Taylor, Dr. James Richardson, and Ms. Linda Rodriguez-Ford.
The Arecibo Planetary Radar Program is funded by NASA’s Near-Earth Object Observations Program. The Arecibo Observatory is operated by the University of Central Florida (UCF) in partnership with Universidad Ana G. Mendez - Universidad Metropolitana and Yang Enterprises Inc., under a cooperative agreement with the National Science Foundation (NSF).
Article written by Dr. Tracy Becker - AO Collaborator / SwRI
Group Lead for Arecibo Planetary Radar
For more information about NASA Planetary Defense program please check out the following links:
Keywords: arecibo, observatory, virkki, NASA, radio , lunar, telescope, radio, telescope, Research, NEO, taylor, Brozovic,Moons ,NASA , Jet, Propulsion, Laboratory, Nolan, Richardson, Rodriguez, Ganymede