论文标题
NASA天体物理学任务的探测级案件
The Case for Probe-class NASA Astrophysics Missions
论文作者
论文摘要
天体物理学涵盖了从单个行星到整个宇宙的尺度上的大量问题。为了解决21世纪天体物理学的丰富性,需要跨越所有乐队和所有使者的望远镜。具有多波长的能力同时提供了很多科学利益。这些乐队大多数或测量敏感性都需要空间的任务。从历史上看,NASA一直以少量的旗舰级任务和更多的探险家任务来满足这种对广度的需求。尽管Explorer计划继续蓬勃发展,但探险家和战略任务之间存在很大的差距。新的天体物理技术与新的,高容量,每公斤低至轨道发射器的新天体物理技术的结合以及新的卫星巴士可以实现更便宜的任务,其功能可以接近战略任务水平。 NASA通过呼吁对任务研究进行调查级任务思想来认识到这些事态发展,跨越了从GEV伽马射线到远红外的大多数电磁频谱,以及中微子和超高能量宇宙射线的新使者。探针练习中的主要见解是,在500m-1b美元的范围内,总体上可以全面地估计科学绩效指标的速度提高。
Astrophysics spans an enormous range of questions on scales from individual planets to the entire cosmos. To address the richness of 21st century astrophysics requires a corresponding richness of telescopes spanning all bands and all messengers. Much scientific benefit comes from having the multi-wavelength capability available at the same time. Most of these bands,or measurement sensitivities, require space-based missions. Historically, NASA has addressed this need for breadth with a small number of flagship-class missions and a larger number of Explorer missions. While the Explorer program continues to flourish, there is a large gap between Explorers and strategic missions. A fortunate combination of new astrophysics technologies with new, high capacity, low dollar-per-kg to orbit launchers, and new satellite buses allow for cheaper missions with capabilities approaching strategic mission levels. NASA has recognized these developments by calling for Probe-class mission ideas for mission studies, spanning most of the electromagnetic spectrum from GeV gamma-rays to the far infrared, and the new messengers of neutrinos and ultra-high energy cosmic rays. The key insight from the Probes exercise is that order-of-magnitude advances in science performance metrics are possible across the board for initial total cost estimates in the range 500M-1B dollars.