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Welcome

Carnegie Trip Map Scientists at DTM bring the perspective of several disciplines to broad questions about nature. DTM's name comes from its original role to chart the Earth's magnetic field. This goal was largely accomplished by 1929. Since then, DTM has evolved to reflect the growing multi- disciplinary nature of the Earth, planetary, and astronomical sciences. Today, the historic goal remains-to understand the physical Earth and the universe that is our home.

The above image is a map tracing the voyages that the Carnegie and the Galilee research vessels undertook, beginning in 1905.
 

News & Features

Boss Comments on Newly Discovered "Earth-Like" Planet
Wednesday, 25 April 2007

Alan Boss commented during yesterday’s NPR Morning Edition on the topic of a radio story entitled, “Earth-Like Planet Discovered in Libra.” The planet in question has a mass about fives times that of Earth and orbits around red dwarf Gliese 581, about twenty light years away in the constellation Libra. Researchers believe that it could be the first known planet outside of our solar system to contain liquid water and perhaps life. Boss remarked, “This seems to be the first discovery of an Earth-like planet. It’s not exactly an Earth, but it’s close enough that I think it does deserve the title of perhaps the first Earth-like planet.”

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MESSENGER Completes Forty Percent of Cruise Phase
Monday, 09 April 2007

On March 28, the MESSENGER spacecraft completed 40% of its 6.6 year cruise phase as measured by time traveled—and one-third of its flight distance to Mercury. DTM director Sean Solomon serves as Principal Investigator of the mission. The cruise phase has been used to commission the spacecraft systems and instruments, and to fine-tune the mission operations procedures of the team at the Johns Hopkins University Applied Physics Laboratory, ensuring that the spacecraft and its instruments will perform flawlessly at Mercury. The average speed of the spacecraft has continued to increase during the cruise phase and will reach a spacecraft record of close to 63 km per second (141,000 miles per hour) in mid-October 2008.

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Completion of CAPSCam Installation
Friday, 09 March 2007
Principal Investigator Alan Boss, Co-Investigator Alycia Weinberger, and colleagues completed installation of the CAPSCam (Carnegie Astrometic Planet Search Camera) this week on the 2.5-m du Pont telescope at Carnegie’s Las Campanas Observatory in Chile. CAPSCam is a Rockwell Hawaii-2RG HyViSI array, specialized for high-accuracy astrometry of red dwarf stars.

The highly accurate astrometric method involves observing the movement of a host star’s position in the sky as it orbits around the center of mass of the star-planet system. Knowing the mass of the star then allows the true mass of the planet, as well as its orbital parameters--including the semi-major axis, eccentricity, and inclination--to be determined. CAPSCam should yield astrometric accuracies of 0.25 millarcsec per epoch. This accuracy is sufficient to detect planets with masses as low as 1/10 the mass of Jupiter on 12-year orbits around nearby late M dwarf stars, with a signal-to-noise ratio of four.

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