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Wednesday, 25 April 2007 |
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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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Monday, 09 April 2007 |
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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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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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