梅西耶马拉松
Messier Marathon

原始链接: https://en.wikipedia.org/wiki/Messier_marathon

梅西耶马拉松是一项业余天文活动,参与者尝试在一个晚上观测尽可能多的110个梅西耶天体(由查尔斯·梅西耶编目的深空天体)。最佳时间和地点是在三月中旬到四月初,大约北纬25度,新月期间。此时间段平衡了天空中各个天体的可见性。虽然其他时间也可以进行部分马拉松,但具体观测到的天体取决于季节和观测者位置。这项活动起源于20世纪70年代,它需要从西方日落开始观测,逐渐向东移动,在东方日出时结束。成功需要耐力、良好的天气和周密的计划,尤其是在应对像室女座星系团这样拥挤的区域时。当地天文组织经常主办这些活动,有时会为参与者或取得成就者颁发证书。

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  • 原文

    Astronomy competition

    Plot of the Messier objects relative to the modern constellations, ecliptic, and Milky Way, using equatorial coordinates (right ascension, declination)

    A Messier marathon is an attempt, usually organized by amateur astronomers, to find as many Messier objects as possible during one night. The Messier catalogue was compiled by French astronomer Charles Messier during the late 18th century and consists of 110 relatively bright deep-sky objects (galaxies, nebulae, and star clusters).

    When and where a marathon is possible

    [edit]

    The number of Messier objects visible in any one night varies depending on a few factors, including the location of the observer, the duration of daylight and nighttime, and the season (the positions of the Messier objects relative to the Sun varies with the season, as does the length of the night).

    Because Messier compiled his catalog from a northern latitude, not all of the Messier objects are visible from the southern hemisphere. In particular, M81, M82, M52, and M103 make southern-hemisphere Messier marathons difficult, because they are all located at a declination of 60° north or greater. Although a Messier marathon can be attempted from any northern latitude, low northern latitudes are best. In particular, a latitude of around 25° north lends the best possibility to complete a Messier marathon at the right time of year.

    At low northern latitudes, particularly around latitude 25° north, it is possible to observe all Messier objects in one night during a window of a few weeks from mid-March to early April. In that period the dark nights around the time of the new moon are best for a Messier marathon.

    Other times of year

    [edit]

    Less complete Messier marathons can be undertaken at other times of the year, with the actual quantity of Messier objects seen depending upon season and location. In particular, there is a short period around the autumnal equinox when most of the objects can be seen.[1]

    The Messier Marathon was invented independently by American astronomers Tom Hoffelder, Donald Machholz, and Tom Reiland in the 1970s. Typically an observer attempting a Messier marathon begins observing at sundown and will observe through the night until sunrise in order to see all 110 objects. An observer starts with objects low in the western sky at sunset, hoping to view them before they dip out of view, then works eastward across the sky. By sunrise, the successful observer will be observing the last few objects low on the eastern horizon, hoping to see them before the sky becomes too bright due to the rising sun. The evening can be a test of stamina and willpower depending on weather conditions and the physical fitness of the observer. Particularly crowded regions of the sky (namely, the Virgo Cluster and the Milky Way's Galactic Center) can prove to be challenging to an observer as well, and a Messier marathon will generally budget time for these regions accordingly.

    Organized marathons

    [edit]

    Marathons are typically organized by a local astronomy organization or astronomical society as a special type of star party. These are usually attempted at least once every year. Some clubs issue certificates/awards either for participation or for achieving a set number of objects.

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