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USGS Open-File Report 2005-1190, Appendix A
USGS Open-File Report 2005-1190 APPENDIX B Detailed listing of personnel changes for the Branch of Astrogeology from 1960 through 1972. In the early 1960’s, the Branch of Astrogeology grew slowly. Growth was rapid during and after 1964 with a maximum of 250 employees being reached in 1970 when design and training for the Apollo missions were at their peaks. [Authors Note: The Branch of Astrogeology in 2006 consisted of approximately 80 employees.] Table 1. Number of Employee with the U.S. Geological Survey, Branch of Astrogeology from 1960 through 1987 [Author’s Note: Although Monthly Reports for Astrogeology were submitted to the USGS and NASA through 1977, new personnel and personnel changes were only documented in these reports through 1970.] Year Number of employees 1960 18 1961 26 1962 40 1963 59 1964 143 1965 154 1966 221 1967 239 1968 244 1969 234 1970 250 1960 The following personnel joined the Astrogeologic Studies Unit at Menlo Park during 1960 (see main text and Appendix A) (various sources): Henry J. Moore II (Geologist, September) Charles H. “Chuck” Marshall (Geologist/Lunar mapper; September) Richard E. Eggleton (Geologist, October) Richard V. Lugn (August) 1961 The following personnel came on duty with the Branch of Astrogeology at Menlo Park, California during 1961 (see main text and Appendix A) (various sources): David J. Roddy (Geologist; January/February) Martin L. Baker (Scientific Photographer; October) Jacquelyn H. Freeberg (Research Librarian and Bibliographer; December) Daniel J. Milton (Geologist; August) Carl H. Roach (Geophysicist; August) 1 Maxine Burgess (Secretary) 1962 The following was taken from the Branch of Astrogeology Monthly Report for April 1962 from Chief, Branch of Astrogeology to V.E. -
Astro2020 Science White Paper Unlocking the Secrets of Late-Stage Stellar Evolution and Mass Loss Through Radio Wavelength Imaging
Astro2020 Science White Paper Unlocking the Secrets of Late-Stage Stellar Evolution and Mass Loss through Radio Wavelength Imaging Thematic Areas: Planetary Systems Star and Planet Formation Formation and Evolution of Compact Objects Cosmology and Fundamental Physics 7 Stars and Stellar Evolution Resolved Stellar Populations and their Environments Galaxy Evolution Multi-Messenger Astronomy and Astrophysics Principal Author: Name: Lynn D. Matthews Institution: Massachusetts Institute of Technology Haystack Observatory Email: [email protected] Co-authors: Mark J Claussen (National Radio Astronomy Observatory) Graham M. Harper (University of Colorado - Boulder) Karl M. Menten (Max Planck Institut fur¨ Radioastronomie) Stephen Ridgway (National Optical Astronomy Observatory) Executive Summary: During the late phases of evolution, low-to-intermediate mass stars like our Sun undergo periods of extensive mass loss, returning up to 80% of their initial mass to the interstellar medium. This mass loss profoundly affects the stellar evolutionary history, and the resulting circumstellar ejecta are a primary source of dust and heavy element enrichment in the Galaxy. However, many details concerning the physics of late-stage stellar mass loss remain poorly understood, including the wind launching mechanism(s), the mass loss geometry and timescales, and the mass loss histories of stars of various initial masses. These uncertainties have implications not only for stellar astrophysics, but for fields ranging from star formation to extragalactic astronomy and cosmology. Observations at centimeter, millimeter, and submillimeter wavelengths that resolve the radio surfaces and extended atmospheres of evolved arXiv:1903.05592v1 [astro-ph.SR] 13 Mar 2019 stars in space, time, and frequency are poised to provide groundbreaking new insights into these questions in the coming decade. -
Cometary Panspermia a Radical Theory of Life’S Cosmic Origin and Evolution …And Over 450 Articles, ~ 60 in Nature
35 books: Cosmic origins of life 1976-2020 Physical Sciences︱ Chandra Wickramasinghe Cometary panspermia A radical theory of life’s cosmic origin and evolution …And over 450 articles, ~ 60 in Nature he combined efforts of generations supporting panspermia continues to Prof Wickramasinghe argues that the seeds of all life (bacteria and viruses) Panspermia has been around may have arrived on Earth from space, and may indeed still be raining down some 100 years since the term of experts in multiple fields, accumulate (Wickramasinghe et al., 2018, to affect life on Earth today, a concept known as cometary panspermia. ‘primordial soup’, referring to Tincluding evolutionary biology, 2019; Steele et al., 2018). the primitive ocean of organic paleontology and geology, have painted material not-yet-assembled a fairly good, if far-from-complete, picture COMETARY PANSPERMIA – cultural conceptions of life dating back galactic wanderers are normal features have argued that these could not into living organisms, was first of how the first life on Earth progressed A SOLUTION? to the ideas of Aristotle, and that this of the cosmos. Comets are known to have been lofted from the Earth to a coined. The question of how from simple organisms to what we can The word ‘panspermia’ comes from the may be the source of some of the have significant water content as well height of 400km by any known process. life’s molecular building blocks see today. However, there is a crucial ancient Greek roots ‘sperma’ meaning more hostile resistance the idea of as organics, and their cores, kept warm Bacteria have also been found high in spontaneously assembled gap in mainstream understanding - seed, and ‘pan’, meaning all. -