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Glossary term: 雙星

Description: 雙星是由兩顆恆星組成的系統,它們在引力的作用下圍繞共同的質心運行。它們的軌道遵循開普勒運動定律,呈橢圓形(形狀像一個壓扁的圓)或圓形。

銀河系中一半以上的恆星要麼屬於雙星系統,要麼是有一顆以上伴星的系統(稱為高階多星系統)的一部分。由於與地球距離遙遠,大多數雙星和高階多星系統在觀測者看來都是單顆恆星。

根據發現雙星所用的觀測方法,雙星可以分為如下幾類,它們可能同時屬於多個類別:

目視雙星是直接觀測即可分辨的兩顆靠近的獨立恆星。並不是所有看起來在天空中離得很近的兩顆恆星都是受引力約束的雙星,有些可能只是出於巧合在天空中看起來很近,但並不受引力約束。不受引力約束的雙星可能相距數百光年。

光譜雙星是由於恆星圍繞它們共同的質心運行時,恆星光譜中的譜線發生了多普勒頻移而被髮現的。

食雙星是其中一顆恆星從它的伴星和觀測者之間穿過時,擋了住來自伴星的部分光線,使系統的組合光線看起來短暫變暗而被探測到的。

天體測量雙星是指只能觀測到一個恆星圖像的系統——可能是由於其中一顆恆星太暗而無法觀測到,也可能是由於兩顆恆星的圖像被混合在一起——但雙星系統中恆星的軌道運動會導致恆星圖像中最亮的點在天空中的位置發生週期性變化。

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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

This is an automated transliteration of the simplified Chinese translation of this term

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Related Diagrams


Carina appears as the hull of a line drawing of a ship which faces left (east). Canopus is on its right (west) edge

Carina Constellation Map

Caption: The constellation Carina along with its bright stars and surrounding constellations. Carina is surrounded by (going clockwise from the top): Vela, Puppis, Pictor, Volans, Chamaeleon, Musca and Centaurus. Carina is notable for Canopus, the second brightest star in the night sky and for the famous variable star Eta Carinae. This latter object is a binary star system of two young very massive stars. Its brightness has varied greatly over the past few centuries. At one point it outshone Canopus before dimming by a factor of four thousand to become invisible to the naked eye. In recent years it has brightened enough to again be visible without the aid of a telescope. Carina is a southern constellation and thus the whole constellation is visible at some point in the year to the entire southern hemisphere. The whole constellation is also visible from equatorial regions of the northern hemisphere with parts of the constellation visible from northern temperate regions. The open clusters NGC 2516, NGC 3532 and IC 2602 lie in Carina. These are marked here by yellow circles. The Carina Nebula, also known as NGC 3372, lies in the constellation. This large nebula contains many massive young stars, including Eta Carinae. This diagram maps an area around the south celestial pole. Here lines of constant right ascension converge. The right ascension values of these lines are marked on the x-axis above and below the diagram. Some of the lines of constant declination are marked on the y-axis. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. Carina was previously part of the larger Argo Navis constellation along with Vela and Puppis. As the letter designations for stars were created before this division took place, Greek letter designations are now divided between the three constellations with Carina having stars designated alpha and beta but no gamma or delta. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. Neither the constellation boundaries, nor the lines joining the stars appear on the sky.
Credit: Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope

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