- Leter from Dr. Julie Brisset (Principal Investigator of the Arecibo Observatory)13 Sep, 2022
- Arecibo Deputy Principal Scientist to Explore the Cosmos with the JWST02 Sep, 2022
- Letter from the Director22 Aug, 2022
- Piercing through the Clouds of Venus with Arecibo Radar17 Aug, 2022
- Summer greetings from the Facilities and Operations Team!17 Aug, 2022
- Arecibo Observatory at the Small Bodies Assessment Group12 Aug, 2022
- Meet the 2022 Arecibo Observatory REU students!11 Aug, 2022
- Meet Luis R. Rivera Gabriel, Research Intern in the Planetary Radar Group09 Aug, 2022
- Updates from the 2022 CEDAR Workshop in Austin, TX09 Aug, 2022
- Insights into the AAS Conference from AO Analyst Anna McGilvray08 Aug, 2022
- American Astronomical Society’s 240th Meeting: Plenary Lecture Building the Future of Radio Science with the Arecibo Observatory by Dr. Héctor Arce. 28 Jul, 2022
- TRENDS 202227 Jul, 2022
- Advancing IDEA in Planetary Science 27 Jul, 2022
- The Arecibo Observatory: An Engine for Science and Scientists in Puerto Rico and Beyond27 Jul, 2022
- Cryogenic Frontend work for the 12m telescope entering phase II21 Jul, 2022
- Remote Optical Facility Updates20 Jul, 2022
Byadmin10 September 2020 Planetary
Arecibo Radar images of the asteroid (101955) Bennu and the physical model of the asteroid developed from those images.
On September 2nd, Dr. Michael Nolan presented a Solar System Ambassadors and Museum Alliance Professional Development Training Webinar titled “Twenty Years of Bennu: From Arecibo to Orbit (and Home Again).”
The webinar highlighted the importance of the Arecibo Observatory for characterizing the near-Earth asteroid (101955) Bennu, the target of NASA’s OSIRIS-REx mission. The spacecraft, currently in orbit around Bennu, is slated to pick up a sample of the asteroid next month and send the piece back to Earth by September 2023.
Dr. Nolan is the Science Team Chief of the OSIRIS-REx mission and a Research Professor at the University of Arizona’s Lunar and Planetary Laboratory. He worked at the Arecibo Observatory for twenty years, from 1995 - 2015, and served as the Head of Planetary Radar program and the Observatory Director.
“Whenever I give a talk about Bennu, I like to give my own personal perspective, which begins at Arecibo,” Dr. Nolan said.
The Arecibo Observatory hosts the most powerful planetary radar system in the world. Observations of Bennu were obtained in 1999, 2005, and 2011. From those, Dr. Nolan created the highly-accurate physical model of the asteroid that was necessary for planning the OSIRIS-REx mission.
“One of my specific goals arriving at Arecibo was to use radar to help plan space missions, and here we are!” - Dr. Michael Nolan, Science Team Chief of the OSIRIS-REx mission
Series of images of the asteroid (101955) Bennu taken from the OSIRIS-REx spacecraft.
In his webinar for the Solar System Ambassadors, Dr. Nolan shared updates from the OSIRIS-REx mission, including the incredible images that the spacecraft has sent back to Earth.
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 Research Scientist
Head of Planetary Radar team
Keywords: arecibo, observatory, planetary,