برنامهٔ مرزهای نو (به انگلیسی: New Frontiers program) شامل یک سری از ماموریتهای فضایی است که توسط ناسا با هدف کاوشگری چندین سیارهٔمنظومهٔ شمسی از جمله مشتری، زهره، و سیارهٔ کوتولهٔپلوتو برنامهریزی شدهاست. ناسا دانشمندان داخلی و نیز بینالمللی را به ارائهٔ پیشنهادهایشان در این زمینه تشویق میکند.
هم اکنون دو مأموریت از برنامهٔ مرزهای نو در فضا در جریان است. نیوهورایزنز که در ۱۹ ژانویهٔ ۲۰۰۶میلادی و فضاپیمای جونو که در ۵ اوت ۲۰۱۱ روانهٔ فضا شد. همچنین اسیریس-رکس که برای بررسی سیارکها و نمونه برداری از سوی ناسا برای پرتاب در سال ۲۰۱۶ میلادی آماده میشود سومین مأموریت برنامهٔ مرزهای نو است.
NASA is encouraging both domestic and international scientists to submit mission proposals for the program. New Frontiers was built on the innovative approach used by the Discovery and Explorer Programs of principal investigator-led missions. It is designed for medium-class missions that cannot be accomplished within the cost and time constraints of Discovery, but are not as large as Large Strategic Science Missions (Flagship missions).
There are currently three New Frontiers missions in progress: New Horizons, which was launched in 2006 and reached Pluto in 2015, Juno, which was launched in 2011 and entered Jupiter orbit in 2016, and OSIRIS-REx, launched in September 2016 towards asteroid Bennu for detailed studies from 2018 to 2021 and a sample return to Earth in 2023.
Juno views Earth in October 2013 during the spacecraft's flyby en route to Jupiter
The New Frontiers program was developed and advocated by NASA and granted by Congress in CY 2002 and 2003. This effort was led by two long-time NASA executives at Headquarters at that time: Edward Weiler, Associate Administrator of Science, and Colleen Hartman, Solar System Exploration Division Director. The mission to Pluto had already been selected before this program was successfully endorsed and funded, so the mission to Pluto, called New Horizons, was "grandfathered" into the New Frontiers program.
The 2003 Planetary Science Decadal Survey from the National Academy of Sciences identified destinations that then served as the source of the first competition for the New Frontiers program. The program name was selected by Hartman based on President John F. Kennedy's speech in 1960, in which he said "We stand, today, on the edge of a New Frontier."
Juno is a Jupiter exploration mission which launched on August 5, 2011 and arrived in July 2016. It is the first solar-powered spacecraft to explore an outer planet. The craft was placed into a polar orbit in order to study the planet's magnetic field and internal structure.
NASA's Galileo mission to Jupiter provided extensive knowledge about its upper atmosphere, however, further study of Jupiter is crucial not only to the understanding of its origin and nature of the Solar System, but also of giant extrasolar planets in general. The Juno spacecraft investigation is intended to address the following objectives for Jupiter:
Understand Jupiter's gross dynamical and structural properties through determination of the mass and size of Jupiter's core, its gravitational and magnetic fields, and internal convection;
Measure the Jovian atmospheric composition, particularly the condensable-gas abundances (H2O, NH3, CH4 and H2S), the Jovian atmospheric temperature profile, wind velocity profile, and cloud opacity to greater depths than achieved by the Galileo entry probe with a goal of 100 bar at multiple latitudes; and
Investigate and characterize the three-dimensional structure of Jupiter's polar magnetosphere.
OSIRIS-REx stands for "Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer", and was launched on 8 September 2016. This mission plan is to orbit an asteroid, at the time named 1999 RQ36 (now 101955 Bennu), by 2020. After extensive measurements, the spacecraft will collect a sample from the asteroid's surface for return to Earth in 2023. The mission, excluding the launch vehicle, is expected to cost approximately $800 million. The returned sample will help scientists answer long-held questions about the formation of the Solar System and the origin of complex organic molecules necessary for the origin of life.
The competition for the fourth mission began in January 2017. Out of 12 initial proposals, NASA selected two for additional concept studies on 20 December 2017, including Dragonfly. '
Per recommendation by the Decadal Survey, NASA's announcement of opportunity was limited to six mission themes:
Comet Surface Sample Return - a comet nucleus lander and sample return mission
Lunar South Pole Sample Return - a mission to land at the Moon's South Pole–Aitken basin and return samples to Earth
Ocean Worlds (Titan and/or Enceladus)
Saturn Probe - an atmospheric probe
Trojan Tour and Rendezvous - a mission to fly by two or more Trojan asteroids
The Decadal Survey recommended the Io Observer and Lunar Geophysical Network proposals for New Frontiers 5, in addition to the previous recommendations. NASA received and reviewed 12 proposals (with the two finalists denoted in bold):
The two finalists, CAESAR and Dragonfly, each received $4 million funding through the end of 2018 to further develop and mature their concepts, and NASA selected in June 2019 to build and launch Dragonfly.
New Frontiers 5
The Decadal Survey recommends that two New Frontiers missions be selected per decade. The 2018 Midterm Review of the 2013–2022 Decadal Survey found that NASA is falling behind on this cadence, and recommends the release of the New Frontiers 5 Announcement of Opportunity no later than December 2021.Thomas Zurbuchen, Associate Administrator for the Science Mission Directorate, responded positively to the Midterm Review's recommendation, stating that NASA is "committed to conducting two New Frontiers competitions per decade" and currently plans to release the Announcement of Opportunity in 2021 or 2022, though the Midterm Review estimates a release date as late as 2023.
^VICI: Venus In situ Composition Investigations. (PDF) L. Glaze, J. Garvin, N. Johnson, G. Arney, D. Atkinson, S. Atreya, A. Beck, B. Bezard, J. Blacksberg, B. Campbell, S. Clegg, D. Crisp, D. Dyar, F. Forget, M. Gilmore, D. Grinspoon,
Juliane Gross, S. Guzewich, N. Izenberg, J. Johnson, W. Kiefer, D. Lawrence, S. Lebonnois, R. Lorenz, P. Mahaffy, S. Maurice, M. McCanta, A. Parsons, A. Pavlov, S. Sharma, M. Trainer, C. Webster, R. Wiens, K. Zahnle, M. Zolotov. EPSC Abstracts, Vol. 11, EPSC2017-346, 2017. European Planetary Science Congress 2017.