Physics World 07月16日 00:07
Spacecraft can navigate using light from just two stars
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NASA的New Horizons探测器通过测量两颗恒星的视差,展示了简单的星际导航。国际研究团队利用地球和太空的观测数据,确定了探测器的位置和航向。这项技术未来可能用于探索太阳系外围或星际任务的航天器导航。New Horizons于2015年访问了冥王星系统,现已穿过柯伊伯带。研究人员选择了最近的恒星比邻星和狼星进行视差测量,探测器在2020年4月23日拍摄了包含这两颗恒星的星场图像,同时地球上的天文学家也进行了相同观测。虽然视差测量精度有限,但证明了仅用两颗恒星即可进行三角定位,这对未来星际导航具有重要意义。

🔭视差测量:通过比较地球和探测器对两颗近邻恒星(比邻星和狼星)的观测位置差异,计算出探测器与地球的相对距离。由于地球与探测器的距离约为47.1天文单位(7亿公里),两颗恒星相对于背景星的视差角分别为32.4和15.7角秒,结合恒星已知距离,理论上可三角定位探测器位置。

🌌观测挑战:项目实施面临COVID-19疫情带来的观测站关闭问题,团队克服困难,利用澳大利亚Siding Spring天文台的Las Cumbres望远镜观测比邻星,美国亚利桑那州Lemmon天文台的Manner望远镜观测狼星,同时探测器自身的LORRI相机也拍摄了双星图像,结合Gaia任务数据进行分析。

🚀技术意义:虽然本次测量精度有限(位置误差0.27天文单位,航向误差0.4°),但成功验证了仅用两颗恒星即可实现星际导航的概念,与需要复杂脉冲星测量设备的现有方法不同,该方法更适用于深空探测,为未来星际任务提供了创新导航方案。

🌠应用前景:该技术可能用于柯伊伯带外的深空探测或真正意义上的星际任务,尤其适用于距离地球遥远的航天器。研究团队计划在条件更优时重复实验,英国卡迪夫大学的Edward Gomez参与该项目时曾以星际导航为高中数学课题,体现了科学与科幻的奇妙联系。

🎸特别参与:Queen乐队吉他手布莱恩·梅(Brian May)也是研究团队成员,这位拥有天体物理学博士学位的艺术家为项目增添了跨界色彩。

NASA’s New Horizons spacecraft has been used to demonstrate simple interstellar navigation by measuring the parallax of just two stars. An international team was able to determine the location and heading of the spacecraft using observations made from space and the Earth.

Developed by an international team of researchers, the technique could one day be used by other spacecraft exploring the outermost regions of the solar system or even provide navigation for the first truly interstellar missions.

New Horizons visited the Pluto system in 2015 and has now passed through the Kuiper Belt in the outermost solar system.

Now, NOIRLab‘s Tod Lauer and colleagues have created a navigation technique for the spacecraft by choosing two of the nearest stars for parallax measurements. These are Proxima Centauri, which is just 4.2 light–years away, and Wolf 359 at 7.9 light–years. On 23 April 2020, New Horizons imaged star-fields containing the two stars, while on Earth astronomers did the same.

At that time, New Horizons was 47.1 AU (seven billion kilometres) from Earth, as measured by NASA’s Deep Space Network. The intention was to replicate that distance determination using parallax.

Difficult measurement

The 47.1 AU separation between Earth and New Horizons meant that each vantage point observed Proxima and Wolf 359 in a slightly different position relative to the background stars. This displacement is the parallax angle, which the observations showed to be 32.4 arcseconds for Proxima and 15.7 arcseconds for Wolf 359 at the time of measurement.

By applying simple trigonometry using the parallax angle and the known distance to the stars, it should be relatively straightforward to triangulate New Horizons’ position. In practice, however, the team struggled to make it work. It was the height of the COVID-19 pandemic, and finding observatories that were still open and could perform the observations on the required night was not easy.

Edward Gomez, of the UK’s Cardiff University and the international Las Cumbres Observatory, recalls the efforts made to get the observations. “Tod Lauer contacted me saying that these two observations were going to be made, and was there any possibility that I could take them with the Las Cumbres telescope network?” he tells Physics World.

In the end, Gomez was able to image Proxima with Las Cumbres’ telescope at Siding Spring in Australia. Meanwhile, Wolf 359 was observed by the University of Louisville’s Manner Telescope at Mount Lemmon Observatory in Arizona. At the same time, New Horizons’ Long Range Reconnaissance Imager (LORRI) took pictures of both stars, and all three observations were analysed using a 3D model of the stellar neighbourhood based on data from the European Space Agency’s star-measuring Gaia mission.

The project was more a proof-of-concept than an accurate determination of New Horizons’ position and heading, with the team describing the measurements as “educational”.

“The reason why we call it an educational measurement is because we don’t have a high degree of, first, precision, and secondly, reproducibility, because we’ve got a small number of measurements, and they weren’t amazingly precise,” says Gomez. “But they still demonstrate the parallax effect really nicely.”

New Horizons position was calculated to within 0.27 AU, which is not especially useful for navigating towards a trans-Neptunian object. The measurements were also able to ascertain New Horizon’s heading to an accuracy of 0.4°, relative to the precise value derived from Deep Space Network signals.

Just two stars

But the fact that only two stars were needed is significant, explains Gomez. “The good thing about this method is just having two close stars as our reference stars. The handed-down wisdom normally is that you need loads and loads [of stars], but actually you just need two and that’s enough to triangulate your position.”

There are more accurate ways to navigate, such as pulsar measurements, but these require more complex and larger instrumentation on a spacecraft – not just an optical telescope and a camera. While pulsar navigation has been demonstrated on the International Space Station in low-Earth orbit, this is the first time that any method of interstellar navigation has been demonstrated for a much more distant spacecraft.

Today, more than five years after the parallax observations, New Horizons is still speeding out of the solar system. It has cleared the Kuiper Belt and today is 61 AU from Earth.

When asked if the parallax measurements will be made again under better circumstances Gomez replied. “I hope so. Now that we’ve written a paper in The Astronomical Journal that’s getting some interest, hopefully we can reproduce it, but nothing has been planned so far.”

In a way, the parallax measurements have brought Gomez full-circle. “When I was doing [high school] mathematics more years ago than I care to remember, I was a massive Star Trek fan and I did a three-dimensional interstellar navigation system as my mathematics project!”

Now here he is, as part of a team using the stars to guide our own would-be interstellar emissary.

 

The post Spacecraft can navigate using light from just two stars appeared first on Physics World.

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星际导航 视差测量 New Horizons 柯伊伯带 天体物理
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