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Nongalactic Astrophysics">astro-ph.CO</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Earth and Planetary Astrophysics">astro-ph.EP</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Astrophysics of Galaxies">astro-ph.GA</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Solar and Stellar Astrophysics">astro-ph.SR</span> </div> </div> <p class="title is-5 mathjax"> Advanced Technology Large-Aperture Space Telescope (ATLAST): A Technology Roadmap for the Next Decade </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/astro-ph?searchtype=author&query=Postman%2C+M">Marc Postman</a>, <a href="/search/astro-ph?searchtype=author&query=Argabright%2C+V">Vic Argabright</a>, <a href="/search/astro-ph?searchtype=author&query=Arnold%2C+B">Bill Arnold</a>, <a href="/search/astro-ph?searchtype=author&query=Aronstein%2C+D">David Aronstein</a>, <a href="/search/astro-ph?searchtype=author&query=Atcheson%2C+P">Paul Atcheson</a>, <a href="/search/astro-ph?searchtype=author&query=Blouke%2C+M">Morley Blouke</a>, <a href="/search/astro-ph?searchtype=author&query=Brown%2C+T">Tom Brown</a>, <a href="/search/astro-ph?searchtype=author&query=Calzetti%2C+D">Daniela Calzetti</a>, <a href="/search/astro-ph?searchtype=author&query=Cash%2C+W">Webster Cash</a>, <a href="/search/astro-ph?searchtype=author&query=Clampin%2C+M">Mark Clampin</a>, <a href="/search/astro-ph?searchtype=author&query=Content%2C+D">Dave Content</a>, <a href="/search/astro-ph?searchtype=author&query=Dailey%2C+D">Dean Dailey</a>, <a href="/search/astro-ph?searchtype=author&query=Danner%2C+R">Rolf Danner</a>, <a href="/search/astro-ph?searchtype=author&query=Doxsey%2C+R">Rodger Doxsey</a>, <a href="/search/astro-ph?searchtype=author&query=Ebbets%2C+D">Dennis Ebbets</a>, <a href="/search/astro-ph?searchtype=author&query=Eisenhardt%2C+P">Peter Eisenhardt</a>, <a href="/search/astro-ph?searchtype=author&query=Feinberg%2C+L">Lee Feinberg</a>, <a href="/search/astro-ph?searchtype=author&query=Fruchter%2C+A">Andrew Fruchter</a>, <a href="/search/astro-ph?searchtype=author&query=Giavalisco%2C+M">Mauro Giavalisco</a>, <a href="/search/astro-ph?searchtype=author&query=Glassman%2C+T">Tiffany Glassman</a>, <a href="/search/astro-ph?searchtype=author&query=Gong%2C+Q">Qian Gong</a>, <a href="/search/astro-ph?searchtype=author&query=Green%2C+J">James Green</a>, <a href="/search/astro-ph?searchtype=author&query=Grunsfeld%2C+J">John Grunsfeld</a>, <a href="/search/astro-ph?searchtype=author&query=Gull%2C+T">Ted Gull</a>, <a href="/search/astro-ph?searchtype=author&query=Hickey%2C+G">Greg Hickey</a> , et al. (43 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0904.0941v2-abstract-short" style="display: inline;"> The Advanced Technology Large-Aperture Space Telescope (ATLAST) is a set of mission concepts for the next generation of UVOIR space observatory with a primary aperture diameter in the 8-m to 16-m range that will allow us to perform some of the most challenging observations to answer some of our most compelling questions, including "Is there life elsewhere in the Galaxy?" We have identified two d… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0904.0941v2-abstract-full').style.display = 'inline'; document.getElementById('0904.0941v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0904.0941v2-abstract-full" style="display: none;"> The Advanced Technology Large-Aperture Space Telescope (ATLAST) is a set of mission concepts for the next generation of UVOIR space observatory with a primary aperture diameter in the 8-m to 16-m range that will allow us to perform some of the most challenging observations to answer some of our most compelling questions, including "Is there life elsewhere in the Galaxy?" We have identified two different telescope architectures, but with similar optical designs, that span the range in viable technologies. The architectures are a telescope with a monolithic primary mirror and two variations of a telescope with a large segmented primary mirror. This approach provides us with several pathways to realizing the mission, which will be narrowed to one as our technology development progresses. The concepts invoke heritage from HST and JWST design, but also take significant departures from these designs to minimize complexity, mass, or both. Our report provides details on the mission concepts, shows the extraordinary scientific progress they would enable, and describes the most important technology development items. These are the mirrors, the detectors, and the high-contrast imaging technologies, whether internal to the observatory, or using an external occulter. Experience with JWST has shown that determined competitors, motivated by the development contracts and flight opportunities of the new observatory, are capable of achieving huge advances in technical and operational performance while keeping construction costs on the same scale as prior great observatories. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0904.0941v2-abstract-full').style.display = 'none'; document.getElementById('0904.0941v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 8 May, 2009; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 6 April, 2009; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2009. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">22 pages, RFI submitted to Astro2010 Decadal Committee</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/astro-ph/0609799">arXiv:astro-ph/0609799</a> <span> </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics">astro-ph</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1089/ast.2006.0124">10.1089/ast.2006.0124 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A Re-appraisal of the Habitability of Planets Around M Dwarf Stars </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/astro-ph?searchtype=author&query=Tarter%2C+J+C">Jill C. Tarter</a>, <a href="/search/astro-ph?searchtype=author&query=Backus%2C+P+R">Peter R. Backus</a>, <a href="/search/astro-ph?searchtype=author&query=Mancinelli%2C+R+L">Rocco L. Mancinelli</a>, <a href="/search/astro-ph?searchtype=author&query=Aurnou%2C+J+M">Jonathan M. Aurnou</a>, <a href="/search/astro-ph?searchtype=author&query=Backman%2C+D+E">Dana E. Backman</a>, <a href="/search/astro-ph?searchtype=author&query=Basri%2C+G+S">Gibor S. Basri</a>, <a href="/search/astro-ph?searchtype=author&query=Boss%2C+A+P">Alan P. Boss</a>, <a href="/search/astro-ph?searchtype=author&query=Clarke%2C+A">Andrew Clarke</a>, <a href="/search/astro-ph?searchtype=author&query=Deming%2C+D">Drake Deming</a>, <a href="/search/astro-ph?searchtype=author&query=Doyle%2C+L+R">Laurance R. Doyle</a>, <a href="/search/astro-ph?searchtype=author&query=Feigelson%2C+E+D">Eric D. Feigelson</a>, <a href="/search/astro-ph?searchtype=author&query=Freund%2C+F">Friedmann Freund</a>, <a href="/search/astro-ph?searchtype=author&query=Grinspoon%2C+D+H">David H. Grinspoon</a>, <a href="/search/astro-ph?searchtype=author&query=Haberle%2C+R+M">Robert M. Haberle</a>, <a href="/search/astro-ph?searchtype=author&query=Hauck%2C+S+A">Steven A. Hauck II</a>, <a href="/search/astro-ph?searchtype=author&query=Heath%2C+M+J">Martin J. Heath</a>, <a href="/search/astro-ph?searchtype=author&query=Henry%2C+T+J">Todd J. Henry</a>, <a href="/search/astro-ph?searchtype=author&query=Hollingsworth%2C+J+L">Jeffery L. Hollingsworth</a>, <a href="/search/astro-ph?searchtype=author&query=Joshi%2C+M+M">Manoj M. Joshi</a>, <a href="/search/astro-ph?searchtype=author&query=Kilston%2C+S">Steven Kilston</a>, <a href="/search/astro-ph?searchtype=author&query=Liu%2C+M+C">Michael C. Liu</a>, <a href="/search/astro-ph?searchtype=author&query=Meikle%2C+E">Eric Meikle</a>, <a href="/search/astro-ph?searchtype=author&query=Reid%2C+I+N">I. Neill Reid</a>, <a href="/search/astro-ph?searchtype=author&query=Rothschild%2C+L+J">Lynn J. Rothschild</a>, <a href="/search/astro-ph?searchtype=author&query=Scalo%2C+J+M">John M. Scalo</a> , et al. (7 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="astro-ph/0609799v2-abstract-short" style="display: inline;"> Stable, hydrogen-burning, M dwarf stars comprise about 75% of all stars in the Galaxy. They are extremely long-lived and because they are much smaller in mass than the Sun (between 0.5 and 0.08 MSun), their temperature and stellar luminosity are low and peaked in the red. We have re-examined what is known at present about the potential for a terrestrial planet forming within, or migrating into,… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/0609799v2-abstract-full').style.display = 'inline'; document.getElementById('astro-ph/0609799v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="astro-ph/0609799v2-abstract-full" style="display: none;"> Stable, hydrogen-burning, M dwarf stars comprise about 75% of all stars in the Galaxy. They are extremely long-lived and because they are much smaller in mass than the Sun (between 0.5 and 0.08 MSun), their temperature and stellar luminosity are low and peaked in the red. We have re-examined what is known at present about the potential for a terrestrial planet forming within, or migrating into, the classic liquid-surface-water habitable zone close to an M dwarf star. Observations of protoplanetary disks suggest that planet-building materials are common around M dwarfs, but N-body simulations differ in their estimations of the likelihood of potentially-habitable, wet planets residing within their habitable zones, which are only ~ 1/5 to 1/50 of the width of that for a G star. Particularly in light of the claimed detection of the planets with masses as small as 5.5 and 7.5 MEarth orbiting M stars, there seems no reason to exclude the possibility of terrestrial planets. Tidally locked synchronous rotation within the narrow habitable zone doesn't necessarily lead to atmospheric collapse, and active stellar flaring may not be as much of an evolutionarily disadvantageous factor as has previously been supposed. We conclude that M dwarf stars may indeed be viable hosts for planets on which the origin and evolution of life can occur. A number of planetary processes such as cessation of geothermal activity, or thermal and non-thermal atmospheric loss processes may limit the duration of planetary habitability to periods far shorter than the extreme lifetime of the M dwarf star. Nevertheless, it makes sense to include M dwarf stars in programs that seek to find habitable worlds and evidence of life. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/0609799v2-abstract-full').style.display = 'none'; document.getElementById('astro-ph/0609799v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 November, 2006; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 28 September, 2006; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2006. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">To be published in Astrobiology. approx. 34 pages</span> </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span 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