- Management Update (COVID-19, Eartquakes, Transmitters)27 Mar, 2020
- NANOGrav Meeting Hosted at UCF27 Mar, 2020
- AO Colloquium: Dr. Michael Denton 27 Mar, 2020
- AO Colloquium: Dr. Alain Herique27 Mar, 2020
- REU Student Mishaal Jan Publishes Summer Research Study about Massive Star Forming Region26 Mar, 2020
- AO helps detect Magnetar in the Cow26 Mar, 2020
- Pulsar Astronomy and Physics at the Arecibo Observatory with Dr. Joanna Rankin26 Mar, 2020
- AO Science at AAS, AOGS26 Mar, 2020
- GBO/AO Single Dish and Observer Training Workshops (May 11-20, 2020)05 Feb, 2020
- Arecibo Observatory update after recent earthquakes09 Jan, 2020
- The Arecibo Observatory Congratulates Dr. Martha P. Haynes, Recipient of 2019 Bruce Gold Medal11 Dec, 2019
- Colloquium Series Recap11 Dec, 2019
- In Memoriam: Yervant Terzian, 1939 - 201906 Dec, 2019
- AO Observations of a Binary Pulsar Test the Theory of General Relativity in New Science Publication06 Dec, 2019
- The International Pulsar Timing Array: Second data release06 Dec, 2019
- Modeling Radar Albedos of Laboratory-Characterized Particles: Application to the Lunar Surface06 Dec, 2019
Byjirizarryrosario22 December 2017 Planetary
Columbia, MD and Puerto Rico — December 22, 2017. After several months of downtime since Hurricane Maria struck the island of Puerto Rico, the Arecibo Observatory Planetary Radar has returned to normal operation, providing the highest-resolution images to date of near-Earth asteroid 3200 Phaethon during its December 2017 close approach to Earth. The radar images, which are subtle at the available resolution, reveal the asteroid is spheroidal (roughly ball-shaped) and has a large concavity, or depression, at least several hundred meters in extent near its equator, and a conspicuous dark, circular feature near one of the poles. Arecibo’s radar images of Phaethon have resolutions as fine as about 250 feet (75 meters) per pixel.
“These new observations of Phaethon show it may be similar in shape to asteroid Bennu, the target of NASA's OSIRIS-REx spacecraft, but more than 1,000 Bennus could fit inside of Phaethon,” said Patrick Taylor, a Universities Space Research Association (USRA), Columbia, Maryland, scientist and group leader for Planetary Radar at Arecibo Observatory. “The dark feature could be a crater or some other topographic depression that did not reflect the radar beam back to Earth.”
"These new observations of Phaethon show it may be similar in shape to asteroid Bennu, the target of NASA's OSIRIS-REx spacecraft, but more than 1,000 Bennus could fit inside of Phaethon" - Dr. Patrick Taylor
Radar images obtained by Arecibo indicate Phaethon has a diameter of about 3.6 miles (6 kilometers) -- roughly 0.6 miles (1 kilometer) larger than previous estimates. Phaethon is the second largest near-Earth asteroid classified as "Potentially Hazardous." Near-Earth objects are classified as potentially hazardous asteroids (PHAs), based on their size and how closely they can approach Earth’s orbit. Tracking and characterizing PHAs is a primary mission of NASA’s Planetary Defense Coordination Office. Radar is a powerful technique for studying asteroid sizes, shapes, rotation, surface features and roughness, and for more precise determination of their orbital path, when they pass relatively close to Earth.
“Arecibo is an important global asset, crucial for planetary defense work because of its unique capabilities,” said Joan Schmelz of USRA and deputy director of Arecibo Observatory. “We have been working diligently to get it back up and running since Hurricane Maria devastated Puerto Rico.”
“Arecibo is an important global asset, crucial for planetary defense work because of its unique capabilities” - Dr. Joan Schmelz
The Arecibo Observatory has the most powerful astronomical radar system on Earth. On Sept. 20, the telescope suffered minor structural damage when Maria, the strongest hurricane to hit the island since 1928, made landfall. Some days after the storm, the observatory resumed radio astronomy observations, while also serving as a base for relief efforts to surrounding communities. Radar observations, which require high power and diesel fuel for generators at the site, resumed operations in early December after commercial power returned to the observatory and the generators could then be used exclusively for the radar.
Asteroid 3200 Phaethon was discovered on Oct. 11, 1983, by NASA's Infrared Astronomical Satellite (IRAS), and the planetary dust that produces the annual Geminid meteor shower originates from this asteroid. Observations of Phaethon were conducted at Arecibo from Dec. 15 through 19, 2017, using the NASA-funded planetary radar system. At time of closest approach on Dec. 16 at 3 p.m. PST (6 p.m. EST, 11 p.m. UTC) the asteroid was about 6.4 million miles (10.3 million kilometers) away, or about 27 times the distance from Earth to the moon. The encounter is the closest the asteroid will come to Earth until 2093, but it came a little closer in 1974 and about half this distance back in 1931 before its existence was known.
The Arecibo Planetary Radar Program is funded by NASA’s Near-Earth Object Observations Program through a grant to Universities Space Research Association (USRA), from the Near-Earth Object Observations program. The Arecibo Observatory is a facility of the National Science Foundation operated under cooperative agreement by SRI International, USRA, and Universidad Metropolitana.
About NASA PDCO
NASA's Planetary Defense Coordination Office is responsible for finding, tracking and characterizing potentially hazardous asteroids and comets coming near Earth, issuing warnings about possible impacts, and assisting coordination of U.S. government response planning, should there be an actual impact threat.
Founded in 1969, under the auspices of the National Academy of Sciences at the request of the U.S. Government, the Universities Space Research Association (USRA) is a nonprofit corporation chartered to advance space-related science, technology and engineering. USRA operates scientific institutes and facilities, and conducts other major research and educational programs, under Federal funding. USRA engages the university community and employs in-house scientific leadership, innovative research and development, and project management expertise. More information about USRA is available at www.usra.edu.
Arecibo Media Contact
Universidad Metropolitana (UMET)
787-878-2612 ext. 615
News Media Contact
Universities Space Research Association
Edgard G. Rivera-Valentín
Universities Space Research Association