Peter Jenniskens

Peter Jenniskens
Senior Research Scientist
Degree/Major: 
Physics and Astronomy
Curriculum Vitae: 
Discipline: 
Planetary Astronomy
We live in space, and with passion and persistence we may one day understand what that means.

If you ever spend a night under the stars watching for meteors and saw something unusual, you may want to meet astronomer Dr. Peter Jenniskens. He’s an expert on meteor showers and author of Meteor Showers and their Parent Comets, a 790 page book containing predictions on what unusual meteor showers to expect in the next 50 years.

Peter is best known for his recovery of fragments of asteroid 2008 TC3 in the Nubian Desert of northern Sudan with Sudanese astronomer Muawia Shaddad and his students from the University of Khartoum. This was the first time that an asteroid was spotted in space, observed by telescopes, then samples retrieved for study. More: http://asima.seti.org/2008TC3/ 

Peter currently runs the NASA sponsored Cameras for Allsky Meteor Surveillance (CAMS) project  in northern California, which aims to confirm some of the 300+ meteor showers in the IAU Working List that need confirmation. Sixty video security cameras film the skies over the San Francisco Bay Area. Each confirmed shower identifies past activity from one of the many Near Earth Asteroids that are being discovered in recent years. He is famous for identifying the parent body of the Quadrantid shower, a minor planet called 2003 EH1, which led to a small rennaiscance in finding parent bodies of our meteor showers. CAMS already confirmed several showers and discovered a new shower, the February eta Draconids, caused by the trail of dust from a potentially hazardous long-period comet. More: http://cams.seti.org

Peter is a meteor storm chaser, who likes to watch meteor showers where they are at their most spectacular: high above clouds in an airplane. His NASA sponsored multi-instrument aircraft campaigns have brought teams of researchers to Japan, Israel, and Spain to study the 1998 – 2002 Leonid meteor storms. In 2007 and 2008, he studied from the air an encounter with the dust of long-period comet C/1911 N1 (Kiess) and the Quadrantid shower. More: http://airborne.seti.org

He has used the same techniques to study artificial meteors during the return of NASA's Genesis and Stardust missions over Utah, the re-entry of ESA's first Automated Transfer Vehicle over the Pacific Ocean and, most recently, the return of JAXA's Hayabusa spacecraft over Australia. These missions gathered data on the physical conditions during entry for clues about the performance of the sample return capsule's thermal protection system and about the manner of breakup during controlled re-entries of spacecraft lacking such thermal protection. One result has been some incredible video footage. More: http://airborne.seti.org

 

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Rapid Response to Announced Small Asteroid Impacts

This project is to establish a program to prepare for and execute a rapid and effective response to a predicted Earth impactor, the next asteroid 2008 TC3. The objective is to fully characterize the asteroid before entry, to measure its internal strength and internal composition during entry, and to recover meteorites for extensive ground-based analysis. The ultimate goal is to forge links between meteorite mineralogy, meteoroid internal strength, and their parent asteroid spectral types, important data needed for the implementation of mitigation actions against a detected impact threat and characterize small Near Earth Objects of the type that are targets for recovery and manned missions.

A spectroscopic survey of meteoroid elemental compositions

This project is to develop and deploy the first automated survey of meteoroid elemental compositions (Mg, Na, Fe, Ca, ...), by simultaneously measuring meteoroid orbits and meteor spectra in large numbers on both the northern and southern hemisphere. The survey will shed light on the diversity of meteor shower parent bodies. This data will be used to test recent planet formation models and improve the first dynamical model of the formation and evolution of the zodiacal cloud.