... 2004 April 25 . D. rad Bacteria: Candidate Astronauts . ... Explanation: These bacteria could survive on another planet. ... Amazingly, they even have the ability to repair their own DNA , usually with 48 hours. Known as an extremophile , bacteria such as D. rad are of interest to NASA partly because they might be adaptable to help human astronauts survive on other worlds. ... About APOD | ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ...

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• APOD: 2006 January 22 - D.rad Bacteria: Candidate Astronauts
• APOD: 2002 September 30 - D rad Bacteria: Candidate Astronauts
• APOD: 2002 July 20 - Footprints on Another World

... D rad Bacteria: Candidate Astronauts . ... 22.01.2006 . ... Credit: Michael Daly ( Uniformed Services University of the Health Sciences ), DOE Explanation: These bacteria could survive on another planet. ... Amazingly, they even have the ability to repair their own DNA , usually with 48 hours. Known as an extremophile , bacteria such as D. rad are of interest to NASA partly because they might be adaptable to help human astronauts survive on other worlds. ... January 2006 . ... 2005 2006 . ...

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• D. rad Bacteria: Candidate Astronauts
• Астронет > D rad Bacteria: Candidate Astronauts
• GRB 990510: Another Unusual Gamma Ray Burst

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. November 19, 1999 . Mercury And The Sun . ... TRACE Project . Explanation: Just days before the peak of the Leonid meteor shower , skywatchers were offered another astronomical treat as planet Mercury crossed the face of the Sun on November 15. Viewed from planet Earth, a transit of Mercury is not all that rare. ... About APOD > . ...

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• APOD: August 30, 1998 - The Sun Erupts
• APOD: June 9, 1999 - NGC 4414: A Telling Spiral
• APOD: May 3, 1997 - Giant Cluster Bends, Breaks Galaxy Images

... To avoid extensive numerical calculations in the statistical simulations, we treat the continuous evolution of each binary component as a sequence of a finite number of basic evolutionary states (for example, main sequence, red (super)giant, helium (Wolf-Rayet) star,     hot WD), in which stellar parameters significantly differ from each other. ... Figure 2: Schematic representation of the typical evolutionary track of a massive binary system with normal and compact star stages indicated. ...

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• Concluding Remarks and Future Prospects

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