Titan In-situ Resource Utilization (ISRU) Sample Return (TISR)

التفاصيل البيبلوغرافية
العنوان: Titan In-situ Resource Utilization (ISRU) Sample Return (TISR)
المؤلفون: Steven Oleson, Geoffrey Landis, Ralph Lorenz, Elizabeth Turnbull, Thomas Packard, Anthony Colozza, David Smith, Jeffrey Pekosh, Steven McCarty, Zachary Zoloty, Laura Burke, James Fittje, John Gyekenyesi, Paul Schmitz, Lucia Tian, Steven Korn, Nick Uguccini, Brent Faller, Christine Schmid, Christopher Heldman, W Peter Simon, Onoufrios Theofylaktos
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 2022.
سنة النشر: 2022
مصطلحات موضوعية: Launch Vehicles And Launch Operations, Lunar And Planetary Science And Exploration, Spacecraft Design, Testing And Performance, Spacecraft Propulsion And Power
الوصف: Titan is unique in the outer solar system in that it is the only moon with a thick atmosphere, and the only body in the solar system outside the Earth with liquid seas on its surface. The Titanian oceans, however, are seas of liquid hydrocarbons, and the rocks on the surface are solid water ice. Like other icy Moons of the outer solar system, beneath the ice crust, Titan also has a subsurface ocean. Rodriguez et al. refer to it as the “world with two oceans”, an organic-rich body with interior-surface-atmosphere interactions that are comparable in complexity to the Earth. [1] Titan is scientifically fascinating in many ways [2], [3], [4]. The Compass Team will emphasize just one here: Titan is a high priority target for astrobiology [4] [5] [6] [7] [8] [9] [10] [11]. It is a world with a surface and atmosphere rich in the complex organic compounds known as tholins. A detailed understanding of the nature of these complex compounds will require an analysis using a full laboratory on Earth. Because of its value to understanding the organic compounds of the outer solar system which may be the primordial building-blocks of life, return of samples from Titan to laboratories on Earth will be the primary goal of this mission. While this would give unprecedented science return, returning even a small sample from Titan using conventional technology would be tremendously difficult. Saturn is almost a billion miles from the Earth, about thirteen times farther than Mars. A return mission to Saturn requires such a large total-mission ∆V that, with conventional technology, the mass ratios required are prohibitive. Such a sample return would truly be “mission incredible.” But to date, a sample return mission from so distant a target has been assumed to be, not merely incredible, but mission impossible. The Compass Team has proposed [2] [12] that by manufacturing the propellant for the return to Earth using the resources available on Titan, such a mission becomes possible. The task of this report is to show that it is reasonable with credible space technology.
نوع الوثيقة: Report
اللغة: English
URL الوصول: https://ntrs.nasa.gov/citations/20220016292
ملاحظات: 371544.01.21.01.22.01
رقم الأكسشن: edsnas.20220016292
قاعدة البيانات: NASA Technical Reports