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首页> 外文期刊>Acta Astronautica >ACADEMY TRANSACTIONS NOTE TETHERED SYSTEM TO GET MAGNIFIED RADIO PICTURES OF THE GALACTIC CENTER FROM A DISTANCE OF 550 AU
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ACADEMY TRANSACTIONS NOTE TETHERED SYSTEM TO GET MAGNIFIED RADIO PICTURES OF THE GALACTIC CENTER FROM A DISTANCE OF 550 AU

机译:学术交易记录系统,用于从550 AU的距离获取银河中心的放大的放射线图像

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The mass of the Sun is by far the largest mass in the solar system. The light-bending effect predicted by general relativity is thus by far larger around the Sun than around any other body in the solar system. The Schwarzschild solution to the Einstein equations yields its value: 4GM/(r c~2), r denoting the "impact parameter", i.e. the minimal distance between the center of the Sun and the bent light path. Now suppose that the light rays come from very far away, specifically from the Galactic Center 32,000 light years (ly) away. This light source may practically be regarded as infinitely distant and it is easy to see that light rays and radio waves from the Galactic Center graze the surface of the Sun and are then focussed by its mass into a point on the other side whose distance is about 550 Astronomical Units (AU), or 3.l7 light days, over l4 times beyond Pluto. This point is the "nearest focus" of the gravitational lens of the Sun, but it is important to realize that every point beyond 550 AU is a focus also because hit by radii having higher impact parameter and so less deflected. A space mission sent along the focal axis (the straight line from the Galactic Center thru the center of the Sun) to 550 AU and beyond would take advantage of the huge radio magnifications of any object lying on the other side of the Sun with respect to the spacecraft position. Such a mission, dubbed "FOCAL" by this author, is described in a formal Proposal submitted to ESA in l993 and in a book published by the author in l997. These studies, however, were restricted by one limitation: the area (of the Galactic Center) hugely magnified by the FOCAL spacecraft is very small: namely, it is a circle equal to the Sun disk or a little more. This restriction is removed in the present paper by the adoption of two antennas, rather than one, tied together by a Tether. We prove that this Tether may have only the modest length of about 2 km if FOCAL is going to magnify the Black Ho1e supposedly located at the Galactic Center (with assumed mass of about a million Sun masses).
机译:迄今为止,太阳的质量是太阳系中最大的质量。因此,由广义相对论预测的光弯曲效应在太阳周围远比太阳系中任何其他物体周围大。爱因斯坦方程的Schwarzschild解得出其值:4GM /(r c〜2),r表示“影响参数”,即太阳中心与弯曲光路之间的最小距离。现在假设光线来自很远的地方,特别是离32,000光年(银河)以外的银河中心。该光源实际上可以被认为是无限远的,很容易看到来自银河中心的光线和无线电波掠过了太阳表面,然后被其质量聚焦到另一侧的点上,该点的距离约为550天文单位(AU),或3.17光日,是冥王星的14倍以上。这一点是太阳引力透镜的“最近焦点”,但重要的是要认识到550 AU以上的每个点都是焦点,因为半径撞击参数具有较高的冲击力,因此偏转较小。沿着焦轴(从银河系中心到太阳中心的直线)发送到550 AU或更高的太空任务将利用位于太阳另一侧的任何物体的巨大无线电放大倍率,相对于航天器的位置。这种任务被该作者称为“ FOCAL”,在1993年提交给ESA的正式提案中以及该作者在1997年出版的书中都有描述。但是,这些研究受到一个局限:由FOCAL航天器极大放大的(银河系中心)面积很小:即,它等于太阳圆盘或更多。在本文中,通过使用由系绳绑在一起的两个而不是一个天线来消除此限制。我们证明,如果FOCAL要放大据推测位于银河中心的黑洞(假定质量约为一百万个太阳质量),则该绳索可能只有大约2 km的适度长度。

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