- Management Update (October 12, 2020) by Director Eng. Francisco Cordova13 Oct, 2020
- Summer Student Assists in Development of Newest AO Facility01 Oct, 2020
- STAR Academy: Training the Next Generation of STEM Professionals 29 Sep, 2020
- Management Update (August 11, 2020) by Director Eng. Francisco Cordova29 Sep, 2020
- Management Update (August 28, 2020) by Director Eng. Francisco Cordova29 Sep, 2020
- Arecibo STAR Teachers29 Sep, 2020
- 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 Asteroids11 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
Byadmin28 December 2018 Comets
Observ-a-thon reveals comet nucleus, holiday asteroid, and more!
Team radar from across several institutions were busy this month observing many targets of interest, including Comet 46P/Wirtanen, near-Earth asteroid 2003 SD220, and 7 other NEAs. The cross-institution teams used the NASA-funded Arecibo S-band planetary radar to study these objects in order to measure their astrometry, size, and characterize their surfaces.
Arecibo radar was able to pierce through the dust and gases that surround Comet 46P/Wirtanen to reveal for the first time its diameter and shape. The observing campaign was led by Dr. Ellen Howell, researcher at the University of Arizona's Lunar and Planetary Laboratory (LPL). Dr. Howell was also a staff scientist at Arecibo for many years prior to moving to LPL. Her radar observing team included Dr. Mike Nolan, also from LPL, Drs. Edgard G. Rivera-Valentin and Patrick Taylor, USRA scientists at LPI, and members of the UCF/Arecibo planetary radar group, Drs. Anne Virkki, Sean Marshall, and Flaviane Venditti.
Range-Doppler image sequence of Comet 46P/Wirtanen taken on 17 December 2018 UT. Here the range (veritcal axis) resolution is 20 m/pxl and Doppler frequency (horizontal axis) resolution is 0.05 Hz/pxl. This set of images reveals the comet to be elongated, with a visible extent of some 540 m, which suggests a diameter > 1km. Several radar bright spots, which could be boulders or other structures, including one at the center of the image that barely moves, can be tracked as the body rotates.
To learn more about these comet observations, click here!
(163899) 2003 SD220
Arecibo also observed near-Earth asteroid (163899) 2003 SD220 using the largest radio telescopes in the nation. For these runs, Arecibo used its powerful transmitter while the echoes were received at the Green Bank Telescope in West Virginia. This observing campaign was co-led by Drs. Edgard G. Rivera-Valentin and Patrick Taylor, USRA scientists at LPI who both worked at Arecibo for many years. Arecibo observers included members of the UCF/Arecibo planetary radar group, Drs. Anne Virkki and Sean Marshall. Observers at Green Bank included Amber Bonsall and Drs. Frank Ghigo and Andrew Seymour. Another experiment, called speckle, was carried out where Arecibo transmited and several radio telescopes of the VLBA received the echoes. The speckle experiment was led by Dr. Michael Busch, SETI scientist.
To learn more about these asteroid observations, click here!
More NEAs!Additionally, the UCF/Arecibo planetary radar group, Drs. Anne Virkki, Flaviane Venditti, and Sean Marshall, detected several near-Earth asteroids: 2003 NW1, 2018 XC4, 2014 JU54, 2018 XS4, 2010 GT7, 2012 MS4, and 2018 XJ1. For all of these objects, the team submitted valuable astrometry, which will help in determining their orbits precisely.
The Arecibo Planetary Radar Program is funded by NASA’s Near-Earth Object Observations Program. The Arecibo Observatory is a facility of the National Science Foundation operated under cooperative agreement by University of Central Florida, Yang Enterprises, and Universidad Metropolitana.
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