John Batchelor Show Hotel Mars, Wednesday, 11-4-15 November 5, 2015Posted by The Space Show in Uncategorized.
Tags: : John Batchelor, chemical signatures, Dr. Ashwin Vasavada, Dr. David Livingston, flowing water on Mars, ice on Mars, liquid water on mars, magnetic field, Mars, Mars climate history., Martian atmosphere, signs of Martian life
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John Batchelor Show Hotel Mars, Wednesday, 11-4-15
Special Guest: Dr. Ashwin Vasavada
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Guests: John Batchelor, Dr. Ashwin Vasavada, Dr. David Livingston. Topics: Liquid flowing water on Mars and more. You are invited to comment, ask questions, and discuss the Space Show program/guest(s) on the Space Show blog. Comments, questions, and any discussion must be relevant and applicable to Space Show programming. Written Transcripts of Space Show programs are not permitted without prior written consent from The Space Show (even if for personal use) & are a violation of the Space Show copyright. We do not permit the commercial use of any Space Show program or part thereof, nor do we permit Space Show programs to be edited, placed on YouTube, or other private channels & websites. Space Show programs can be quoted in news articles, papers, academic & research work but must be cited or referenced in the proper citation format. Contact Dr. Livingston for questions about our copyright and trademark policies which we do enforce. This program is archived on The Space Show website, podcasting, and blog sites with permission from John Batchelor. Please visit the John Batchelor Show website for more information about this fine program, www.johnbatchelorshow.com. Remember, your Amazon Purchases Can Help Support The Space Show/OGLF (www.onegiantleapfoundation.org/amazon.htm). For those of you listening to archives on live365.com & rating the programs, please email me the reasons for your rating. This will definitely help improve Space Show programming. Thank you. Please note that audio and transition issues are a result of copying the John Batchelor broadcast & are not within my control as they originate in the Batchelor studio.
John Batchelor and I welcomed back Dr. Ashwin Vasavada to discuss NASAs recent announcement about flowing liquid water on Mars. We also talked about other locations for water on Mars including ice which could be converted to rocket fuel were there sufficient energy available for such a conversion by those on Mars wanting the fuel. Dr. Vasavada explained the liquid flowing water and answered questions about the Martian atmosphere. We also talked about Curiosity and its examination of the early Martian climate history through its work in Gale Crater. We talked about the possibility of finding signs of life. With respect to this question, our guest said that the odds for finding signs of life are improving all the time. They odds “keep going up.”
You can email Mr. Batchelor or Dr. Ashwin Vasavada through me at email@example.com.
Dr. David Lawrence, Friday, 12-28-12 December 29, 2012Posted by The Space Show in Uncategorized.
Tags: " Mercury, Crater naming process., data embargo, Dawn Mission, Dr. David Lawrence, Earth, Gamma Ray and Neutron Spectrometer (GRNS), Johns Hopkins Applied Physics Lab, magnetic field, Mars, Mercury craters, Mercury density, Mercury flyby's, Mercury Hollows, Mercury orbital dynamics, Mercury tectonic activity, Messenger, Moon, NASA, NASA budget, NASA Discovery Program, NASA Planetary Portal System, neutron spectroscopy, organic molecules, Venus, Vesta, volatile elements, water ice at the poles
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Dr. David Lawrence, Friday, 12-28-12
Guest: Dr. David Lawrence. Topic: The planet Mercury & the NASA Messenger Mission. Please direct all comments & questions regarding Space Show programs/guest(s) to the Space Show blog, https://thespaceshow.wordpress.com. Comments & questions should be relevant to the specific Space Show program. Written Transcripts of Space Show programs are a violation of our copyright & are not permitted without prior written consent, even if for your own use. We do not permit the commercial use of Space Show programs or any part thereof, nor do we permit editing, YouTube clips, or clips placed on other private channels & websites. Space Show programs can be quoted, but the quote must be cited or referenced using the proper citation format. Contact The Space Show for further information. We welcomed Dr. David Lawrence to the program to discuss the planet Mercury & the NASA Messenger Mission’s latest finding. For more information, visit the Messenger websites, http://www.nasa.gov/mission_pages/messenger/main/index.html & http://messenger.jhuapl.edu. We started our discussion by describing the Mercury & the Messenger mission. For example, it took over six years to get to Mercury because of the difficulty in slowing the spacecraft down given the close proximity to the sun. Dr. Lawrence explained this process to us & the Venus, Mercury, & Earth flyby program used by the spacecraft to orbit around Mercury. We talked about the spacecraft health, the instruments on board & the problem with the gamma ray spectrometer which worked for about 9,000 hours on an expected life of 8,000 hours. However, data from this instrument is still being analyzed & will be for some time to come. Other instruments on Messenger are fine & the spacecraft has a life expectancy to 2015. Our guest explained mission nominal life & the process for mission extensions with additional NASA funding. We talked about funding issues for Messenger & other planetary missions in light of NASA budget issues & the overall U.S. economy. Dr. Lawrence told us how the missions compete for extension & additional funding, plus the requirements they must meet to be extended. Listeners wanted to know about the application of Messenger & Mercury science to Earth & other solar system missions, our Moon, a NEO, even Mars. Other listeners wanted to know Mercury’s distances from the sun & Earth, as well as more about possible tectonic activity on Mercury. We discussed basic chemical elements found on Mercury as well as volatile elements.
In our second segment, Dr. Lawrence was asked to identify the biggest surprise so far which he said had to do with the composition of the planet & volatile elements with high concentrations of sulfur & sodium, among others. A listener asked about Mercury radiation levels & another listener wanted to know how Mercury crater’s got their names. Dr. Lawrence then took us through the crater naming process which you can also read about on the Messenger websites. We talked about Messenger’s discovery of Hollows (see, http://science.nasa.gov/science-news/science-at-nasa/2011/24oct_sleepyhollows). One listener asked our guest how one gets on a science team like Messenger. Dr. Lawrence explained the paths to joining these teams. Mercury’s high density came up & our guest talked about most all of the iron on the planet being concentrated in its core. We also talked about data analysis, archives, embargos, & availability. Our guest directed us to the NASA Planetary Portal System for more information. Near the end, we talked about the NASA Discovery Program & other successful Discovery missions including Dawn.
Please post your comments/questions on The Space Show blog. You can email Dr. Lawrence through me or the APL Messenger website.