Collaborative Research: An Ultrastable Blue Astro Comb for Exoplanet and Cosmology Research

合作研究：用于系外行星和宇宙学研究的超稳定蓝色 Astro 梳

• 批准号: 0905214
• 负责人: Ronald Walsworth
• 金额: $ 33万
• 依托单位: Harvard University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-09-15 至 2012-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0905214&HistoricalAwards=false
• 关键词: Collaborative; Research; Ultrastable; Blue; Astro

This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).Great progress has been made in recent years in detecting massive planets orbiting other stars. These exciting discoveries are an important step toward understanding the evolution of other solar systems and whether or not they may harbor life. Tantalizing as these discoveries are, however, they are not conclusive. Astronomers have yet to find a planet in another solar system that could support life as we know it. To do so would require finding smaller solid (not gaseous) earth-like planets orbiting a star within the "habitable zone" where the distance of the planet from the star is such that the surface temperature of the planet can sustain liquid water. There are at least four ways to detect a planet orbiting a star. By far the most successful means to date has been to very carefully monitor the velocity of the star. If the velocity tends to vary regularly about its average value, then it is possible that some celestial body is in orbit around it and we are measuring the reflex velocity of the star due to the changes in the position of the planet in its orbit. This is a very exacting measurement to make and it relies on extremely accurate velocity measurements made with a spectrograph. Large planets create the biggest velocity wiggle and are therefore easiest to detect. But detecting smaller earth like planets in the habitable zone requires much higher precision than is currently available. Dr. Franz Kaertner of the Massachusetts Institute of Technology is designing a very stable and accurate calibration mechanism to improve the radial velocity measurements. He is working with a number of scientific colleagues and several students to design and build the device over the next two years. This new scheme uses a very rapidly pulsed laser to imprint a regularly spaced calibration "comb" of lines of precisely known wavelengths through the spectrograph and onto the spectrum of the star. This new technique will improve the velocity determination from the current standard by about a factor of 100, enough to detect earth-like planets in the habitable zone.

该奖项是根据 2009 年美国复苏和再投资法案（公法 111-5）资助的。近年来，在探测绕其他恒星运行的大质量行星方面取得了巨大进展。 这些令人兴奋的发现是了解其他太阳系演化以及它们是否可能存在生命的重要一步。尽管这些发现很诱人，但它们并不是决定性的。 天文学家尚未在另一个太阳系中找到一颗可以支持我们所知的生命的行星。 要做到这一点，需要在“宜居带”内找到围绕恒星运行的较小固体（而非气态）类地行星，其中行星与恒星的距离使得行星的表面温度可以维持液态水。至少有四种方法可以检测绕恒星运行的行星。 迄今为止，最成功的方法是非常仔细地监测恒星的速度。 如果速度趋于围绕其平均值有规律地变化，则可能有某个天体在其周围的轨道上运行，并且我们正在测量恒星的反射速度，这是由于行星在其轨道上的位置的变化而引起的。 这是一项非常严格的测量，它依赖于用摄谱仪进行的极其精确的速度测量。 大行星产生最大的速度摆动，因此最容易被发现。 但探测宜居带内较小的类地行星需要比目前更高的精度。 麻省理工学院的 Franz Kaertner 博士正在设计一种非常稳定且精确的校准机制，以改进径向速度测量。 他正在与一些科学同事和几名学生合作，在未来两年内设计和建造该设备。这种新方案使用非常快速的脉冲激光，通过光谱仪将精确已知波长的规则间隔的校准“梳”印刻到恒星的光谱上。 这项新技术将使当前标准的速度测定提高约 100 倍，足以探测位于宜居带的类地行星。