Updates on the 2007 Shoemaker NEO Grant Recipients
Our 2007 Shoemaker NEO Grant winners have been extremely busy over the past two years. Take for example Quanzhi Ye of Guangzhou, China: He was only 18 when he received the award but already the principal investigator of the sky survey at the Lulin Observatory in Taiwan. In July 2007, using the new laptop he purchased with his award, Quanzhi co-discovered a comet on its way into the inner solar system. Eighteen months later, in February 2009, the "Lulin" comet made its closest approach to Earth, where it was visible to the naked eye from dark locations.
"The laptop bought with the fund from Shoemaker NEO Grant was used when discovering Comet Lulin and many other asteroids (including providing follow-up observations for NEO's)," Quanzhi Ye wrote in an e-mail message to the Society. "When I went out for travel I always bring the laptop with me, and process data on the way when internet access is available . . . [it] makes my work at Lulin much more efficient."
Only days after discovering the comet Quanzhi Ye detected another nearby space rock, designated 2007 NL1. Unfortunately an approaching Typhoon prevented him from conducting follow-up observations, so he called up Jean-Claude Pelle – another member of the Shoemaker NEO class of 2007. Pelle is based in Tahiti in the southern Pacific Ocean, where he enjoyed fine weather and clear visibility. He took over from Quanzhi and was able to confirm the NEO and track it for several nights, beginning the process of defining its orbit.
In early March 2009, when a massive space rock several dozen meters in diameter buzzed the Earth at only one fifth the distance to the Moon, Pelle was once again well-placed to observe it. 2009 DD45, as the rock was designated, made its closest approach to Earth over Tahiti, giving Pelle the opportunity to take numerous images and track its path through the sky.
Two weeks later Richard Kowalski of the Catalina Sky Survey, who received a Shoemaker-NEO grant in 2002, had a hand in the discovery of 2009 FH -- a NEO about half the size of 2009 DD45, that came almost as close to Earth. Follow-up observations were then conducted by another 2002 recipient -- James McGaha of the Sabino Canyon Observatory in Arizona -- and by Robert Holmes of the Astronomical Research Institute, a 2007 grant recipient.
Tracking Faint Objects
The magnitude of an object in the sky is a measure of its relative brightness and is a logarithmic scale. Objects that differ in magnitude by 5 differ in brightness by a factor of 100. The greater the brightness, the lower the magnitude; most stars have positive magnitudes, while the naked-eye planets, Moon, and Sun have negative magnitudes. The Sun has an apparent magnitude of -26; the brightest star in the sky, Sirius, has an apparent magnitude of -1.46. So the objects being detected at magnitudes of about 23.5 by Robert Holmes at the Astronomical Research Institute are fainter than Sirius by roughly the same factor that Sirius is fainter than the Sun.
Apart from such highlights, the chief role Shoemaker remains conducting follow-up observations of known NEO's to refine their orbits, and conducting measurements of the space rocks' physical characteristics. For this purpose several of the 2007 Shoemaker NEO Grant winners used their funds to purchase CCD cameras capable of capturing large swaths of the sky or imaging very faint objects, or both. Robert Holmes reports that with the new CCD camera purchased with NEO grant funds, 84,600 images of near-Earth objects were taken in the year from June 1, 2007 to May 31, 2008. From these, the Astronomical Research Institute reported a staggering 5,835 targeted measures of comets and near-Earth asteroids to the Minor Planet Center. The faintest object Holmes captured on camera was 2001 SD170, observed at an unfiltered magnitude of about 23.5.
Jean-Claude Pelle also used his NEO Grant award to purchase a CCD camera permitting him to capture a view of the sky 39 arcminutes square. This relatively broad field of view has facilitated Pelle's efforts to follow up on just-discovered NEOs whose orbits were only observed over a very short arc (often less than one hour) and so suffer from large uncertainties in their position. By aggressively following these recently-discovered objects, Pelle and his collaborators at Southern Stars Observatories have multiplied the length of the known arcs of some bodies by factors as large as 20. The wide field of view also brings a collateral benefit: many other objects are also often present in a single image. As a by-product of near-Earth object follow-up, Southern Stars Observatories workers have discovered 150 discoveries of main-belt asteroids.
The benefit of the NEO Grant to Giovanni Sostero and his coworkers at the Associazione Friulana di Astronomia e Meteorologia in Remanzacco, Udine, Italy has been to improve their computing power with two new PCs, speeding up their reaction times in following up new, fast-moving objects. His group now conducts astrometric and photometric follow-up from two sites in Italy, a permanent observatory at Remanzacco and a site for their portable telescopes in Comeglians, with a third position under construction at Mount Matajur, 1,320 meters above sea level. They and also observe remotely, from New Mexico and Australia. In a period of fifteen months, Sostero's group has confirmed 27 NEOs to be comets, has performed confirmation observations on the discoveries of nearly 50 NEOs (some of them very faint, at magnitudes near 21), and has recovered seven periodic comets.
Sostero's group has leveraged the $4,400 of their Shoemaker NEO Grant to win even larger support for their efforts to discover, track, and study NEOs. Sostero reports that other institutions and foundations in Italy provided further funding to refurbish their observatories after learning of the grant award; and that more collaborators joined his team after learning of the team's work from television and newspaper reports about the NEO threat and the award of the Shoemaker NEO Grant. "The benefits of the Gene Shoemaker NEO Grant has exceeded our expectations," Sostero said.
Brian Warner, at the Palmer Divide Observatory in Colorado, has put his Shoemaker NEO Grant to slightly different use. His grant allowed him to purchase a second telescope, which he employs to do photometry (studies of how the brightness of asteroids vary with the observing angle and the asteroid's rotation), which, in turn, helps to provide information on the size and shape of larger asteroids. Although these studies don't directly address the problem of whether a given asteroid will or won't hit Earth, they provide important data to the broader research into the range of sizes and shapes of the asteroid population, and into studies on YORP, the various ways that asteroid orbits change as sunlight is absorbed, reflected, and re-radiated by spinning, odd-shaped, inhomogeneously colored asteroids. As a by-product of his studies, Warner has discovered that at least a dozen asteroids are binaries. Don Pray of the Carbuncle Hill observatory has been performing similar photometric studies, helping to confirm that at least four asteroids are binaries.
Bringing the Public Along for the Ride
Many of the Shoemaker NEO Grant winners have embarked on programs to educate their communities about the night sky and the hazard of potential asteroid impact. Some also involve classrooms around the world in the work to discover and track potentially hazardous objects.
For example, the Astronomical Research Institute in Illinois is participating in the worldwide "Killer Asteroid Project," which raises awareness about the threat of near-Earth objects to teachers and students around the world. Holmes says, "Each night up to one gigabyte of data is imaged using The Planetary Society SBIG STL-1001E CCD camera, uploaded to the internet, and made available to high schools, colleges, and universities for use in their classrooms within 5 hours of acquisition. In May 2008, the Astronomical Research Institute presented more than 450 awards to schools, teachers, and students in nine countries including China, Germany, Italy, Japan, Morocco, Poland, Portugal, Russia, and the United States."
For Eric Allen of Quebec, the publicity generated by his grant award gave him the argument he needed to convince his superiors to permit him to open the observatory to the public for the first time since 2003. Now the observatory is open to the public six nights a week, and Allen educates the visitors about the night sky and NEOs. He was also interviewed for a Discovery Canada documentary on the 100th anniversary of the Tunguska impact event. His effort to automate his dome (the focus of his grant award) has been delayed because of the work involved in performing public outreach, but he expects fully automated observing runs to begin in late August.
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