As the 1.8 meter (60 inch) Pan-STARRS 1 telescope (PS1), one of the most powerful current survey telescopes, scans the night sky, its 1400 Megapixel digital camera takes more than 500 exposures per night. Between October 25 and December 21, 2010, some of this data found its way into classrooms in the USA and in Germany, where high-school students have used it to track known asteroids, and also to discover candidate objects that could be previously unknown asteroids. When Hawaiian skies were overcast, schools also received data taken with a telescope operated by the Astronomical Research Institute (ARI) in Westfield, Illinois.
The PS1 telescope on Hawaii
Image credit: Rob Ratkowski
Over the Internet, the participating schools received series of astronomical images. Each series included images of one specific region of the sky, taken an hour apart. During this hour, the image of a main belt asteroid would have moved noticeably (in the images in question: about 100 pixels) relative to the distant background stars. The students examined the images for exactly this kind of position change, carefully sorting image artifacts from moving celestial objects, and reported back to the International Astronomical Search Collaboration, whose volunteers then checked the results and arranged for follow-up observations.
Some of the most interesting student observations during the project concerned “Near-Earth Objects” (NEO), asteroids or similar objects whose orbits bring them into the inner Solar System. Some NEOs might turn out to be potential “killer asteroids” that are bound to collide with our home planet; finding these is one main goal of the PS1 telescope. In order to keep track of NEOs, at least two separate observations at different times are required. Katharina Stöckler (age 17), an 11th grade student at Gymnasium Neckargemünd near Heidelberg, explains: “We obtained a ‘NEO confirmation’ for the asteroid 2010 UR7 – the second observation ever made of that object, which confirmed the asteroid’s existence and gave crucial information about its orbit.” Three additional such “NEO confirmations” were made during the project; in addition, 64 of the students' observations amounted to the third or fourth time a specific NEO had been observed. All these observations provide important additional data to scientists studying the motion of NEOs.
In the course of the project, the students also observed 151 candidate objects in the Pan-STARRS data (plus an additional 20 candidates in the ARI/Westfield telescope data) that could be newly discovered main belt asteroids, which orbit the Sun between the orbits of Mars and Jupiter. In one case, students from Benedikt Stattler Gymnasium, a high-school in Bavaria, Germany, discovered 7 such candidate objects in a single night! Before the students' finds are confirmed as discoveries, however, and assigned provisional designation numbers, they will need to be observed again – for a number of the candidates, this is going to prove impossible; on the other hand, some are likely to turn out to have been previously known, after all. Once a newly found object has been observed over at least a whole orbit (which typically lasts 3 to 6 years), it is assigned a definite numerical identifier, and can also be given a proper name.
IASC director Dr. Patrick Miller, of Hardin-Simmons University in Abilene, Texas, says: “Pan-STARRS images contain an amazing amount of data, providing students with opportunities for literally hundreds of new discoveries. With this amount of data, we could expand our campaign to a thousand schools a year, and tens of thousands of students, which is very exciting, and is an unbelievable opportunity for high schools and colleges!”
Pan-STARRS Project Manager Dr. William Burgett adds: "It is incredibly exciting that we can use a state-of-the-art system such as Pan-STARRS to allow students around the world to learn astronomy with real research quality images. We are committed to making this a valuable and enjoyable experience for both the students and their teachers, and we hope this is only the first step in eventually involving hundreds of schools around the world."
The Pan-STARRS liaison for the IASC-Pan-Starrs campaign is Pan-STARRS Project Manager William Burgett (University of Hawaii Institute for Astronomy). The campaign is made possible by the board of the PS1 Science Consortium and by the particular efforts and support of Larry Denneau (University of Hawaii Institute for Astronomy), Matt Holman (Harvard-Smithsonian Center for Astrophysics), Robert Jedicke, Nick Kaiser, Gene Magnier and Richard Wainscoat (all UH Institute for Astronomy).
The International Astronomical Search Collaboration (IASC, pronounced “Isaac”) is an educational outreach program for high schools and colleges, provided at no cost to the participating schools. Since the program’s foundation in fall 2006, more than 200 schools – thousands of students – per year have participated in its search campaigns, representing more than 30 countries on five continents. Over the Internet, the schools receive astronomical images taken only hours before. Students then use the software package Astrometrica to search for, discover, and measure the properties of asteroids. Overall, students have discovered more than 300 previously unknown asteroids, seven of which have received an official number and been cataloged by the Minor Planet Center at Harvard, the body in charge of keeping track of asteroid designations. (As the official numbering can take 5-10 years from the date of discovery, this number is bound to increase rapidly.) Students have also performed thousands of measurements of near-Earth objects, which pose a possible impact hazard with Earth. Centered at Hardin-Simmons University (Abilene, Texas), IASC is a collaboration of the University, Lawrence Hall of Science (University of California at Berkeley), Astronomical Research Institute (Westfield, Illinois), Global Hands-On Universe Association (Lisbon, Portugal), Tarleton State University (Stephenville, Texas), Sierra Stars Observatory Network (Markleeville, California), and Astrometrica (Linz, Austria). The present campaign builds on the Global Hands-on Universe (GHOU) collaboration. GHOU is an educational program that enables students to investigate the Universe while applying tools and concepts from science, math, and technology. GHOU has reached about 30 nations, and trained approximately 5000 teachers around the world in techniques and the use of modern astronomy in classrooms.
The German schools of the Pan-STARRS-IASC search campaign are coordinated and supported by the Center for Astronomy Education and Outreach (Haus der Astronomie) in Heidelberg (in collaboration with the Max Planck Institute for Astronomy in Heidelberg and the Starkenburg-Sternwarte Heppenheim), the Max Planck Institute for Extraterrestrial Physics in Garching, and the Technical University Munich.
The participating international teams of schools are:1. Luitpold-Gymnasium, Munich, Germany
expressed in this press release are those of the author(s), and do not necessarily reflect the views of the National Aeronautics and Space Administration.
NEO Confirmations (second observation of a specific Near-Earth Object; listed are the object identifier, the observing school, and the observation date):2010 UR7, Gymnasium Neckargemünd, 30 October 2010
Dr. Markus Pössel | Max-Planck-Institut
Astronomers find unexpected, dust-obscured star formation in distant galaxy
24.03.2017 | University of Massachusetts at Amherst
Gravitational wave kicks monster black hole out of galactic core
24.03.2017 | NASA/Goddard Space Flight Center
Astronomers from Bonn and Tautenburg in Thuringia (Germany) used the 100-m radio telescope at Effelsberg to observe several galaxy clusters. At the edges of these large accumulations of dark matter, stellar systems (galaxies), hot gas, and charged particles, they found magnetic fields that are exceptionally ordered over distances of many million light years. This makes them the most extended magnetic fields in the universe known so far.
The results will be published on March 22 in the journal „Astronomy & Astrophysics“.
Galaxy clusters are the largest gravitationally bound structures in the universe. With a typical extent of about 10 million light years, i.e. 100 times the...
Researchers at the Goethe University Frankfurt, together with partners from the University of Tübingen in Germany and Queen Mary University as well as Francis Crick Institute from London (UK) have developed a novel technology to decipher the secret ubiquitin code.
Ubiquitin is a small protein that can be linked to other cellular proteins, thereby controlling and modulating their functions. The attachment occurs in many...
In the eternal search for next generation high-efficiency solar cells and LEDs, scientists at Los Alamos National Laboratory and their partners are creating...
Silicon nanosheets are thin, two-dimensional layers with exceptional optoelectronic properties very similar to those of graphene. Albeit, the nanosheets are less stable. Now researchers at the Technical University of Munich (TUM) have, for the first time ever, produced a composite material combining silicon nanosheets and a polymer that is both UV-resistant and easy to process. This brings the scientists a significant step closer to industrial applications like flexible displays and photosensors.
Silicon nanosheets are thin, two-dimensional layers with exceptional optoelectronic properties very similar to those of graphene. Albeit, the nanosheets are...
Enzymes behave differently in a test tube compared with the molecular scrum of a living cell. Chemists from the University of Basel have now been able to simulate these confined natural conditions in artificial vesicles for the first time. As reported in the academic journal Small, the results are offering better insight into the development of nanoreactors and artificial organelles.
Enzymes behave differently in a test tube compared with the molecular scrum of a living cell. Chemists from the University of Basel have now been able to...
20.03.2017 | Event News
14.03.2017 | Event News
07.03.2017 | Event News
24.03.2017 | Materials Sciences
24.03.2017 | Physics and Astronomy
24.03.2017 | Physics and Astronomy