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- 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
- Modifying the Earth’s Ionosphere from Arecibo29 Jun, 2020
- AO radar measurements of Jupiter’s Moons29 Jun, 2020
- A New Approach for Understanding the Occurrence Rate of MSTIDs in the Caribbean Nighttime Ionosphere29 Jun, 2020
Byjirizarryrosario14 March 2019 Astronomy
|Astronomy||March 8th, 2019|
Alex Wolszczan discusses Arecibo’s potential in the field of exoplanets- written by Nipuni Palliyaguru
Dr. Alex Wolszczan, who is a professor at Penn State and a long-term user, visited the Arecibo Observatory during the week of March 4th, 2019 as part of an observing campaign to search for radio emission from cool brown dwarfs.
During this visit, Alex spoke about the possibility of detecting such planets via flaring radio emission and about detecting planets around pulsars through precision timing. He also talked about Jupiter-Io like emission from compact planetary systems, and plans to search for such flaring events from low-mass stars, brown dwarfs, and white dwarfs.
Dr. Alex Wolszczan with Dr. Abel Mendez and his undergraduate students and faculty from University of PR at Arecibo, who are performing exoplanet searches with the Arecibo telescope.
The measurement of magnetic fields is key in probing the internal structure of exoplanets and has important implications for habitability. He spoke about how Arecibo’s sensitivity is crucial in detecting these faint systems and the need to observe at frequencies from below 1 GHz to at least 10 GHz. Arecibo telescope can observe up to 10 GHz and is the largest single dish telescope, currently operational, capable of observing at frequencies above 1.4 GHz.
At the February 2019 Arecibo Futures meeting, aimed at discussing a science blueprint for the next decade, exoplanet research was identified as a key area that the Arecibo observatory could be a leader in. The seminar was attended by current and former observatory staff, faculty and students from UPR Arecibo. This effort is part of an initiative to involve undergraduate and graduate students of Puerto Rican universities in the activities conducted at the Observatory.
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About Arecibo Observatory
The Arecibo Observatory is operated by the University of Central Florida (UCF) in partnership with Sistema Ana G. Mendez Universidad Metropolitana and Yang Enterprises Inc., under a cooperative agreement with the National Science Foundation (NSF).
Keywords: astronomy, observatory, arecibo, planetary, systems, exoplanets, jupiter, dwarfs