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圣诞节彗星(C/2002 X5)观测用星图:

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rjxie 发表于 2002-12-17 17:03 | 显示全部楼层 |阅读模式 来自: 中国–辽宁–大连 联通

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December 16, 2002 | Early on the morning of December 14th, Japanese amateur Tetuo Kudo was searching the skies with his giant 20 x 120 binoculars. While scanning the constellation Hercules, he spotted something new — a fuzzy 9th-magnitude glow moving slowly east-southeast. Follow-up observations by Ken-ichi Kadota (Saitama, Japan) confirmed the object and revealed a short tail about 1/3° in length, pointing away from the Sun.
The comet was announced on International Astronomical Union Circular 8032.

A preliminary orbit calculated by Brian G. Marsden of the Minor Planet Center in Cambridge, Massachusetts, indicates that this comet is headed for perihelion in late January,  
Binoculars should be all you need to spot the new comet just before dawn in the last two weeks of December. (You can find when dawn begins at your site by entering your location into our almanac.) Start with the bright landmark stars Arcturus (top right) and Vega (lower left). The sky's position with respect to the horizon is shown very approximately. This horizon is drawn for skywatchers at 40° north latitude when dawn begins around the end of December. Before that date the comet will be less high than shown here; after that it will be higher than here. Stars are plotted to magnitude 6.8. Sky & Telescope diagram.


 
 
when it will pass well inside the orbit of Mercury and may brighten considerably. Unfortunately, it will then be almost directly behind the Sun as seen from Earth, hence virtually impossible to observe. Before that time, Northern Hemisphere observers should be able to follow the comet with binoculars in the morning sky through mid-January. Skywatchers in the Southern Hemisphere are in a position to see it emerging from the Sun's glare in late February, in the evening sky.

Currently the comet is about 7th magnitude, making it a viable binocular object for amateurs. It could be 6th magnitude or brighter by the year's end.

The comet's preliminary designation is C/2002 X5. Once it is confirmed that there were no independent discoverers, its name will likely be changed to Comet Kudo.

The following ephemeris gives the comet's right ascension and declination (equinox 2000.0) at 0 hours Universal Time on each date, its elongation angle from the Sun, predicted magnitude, and the constellation through which it's passing.

Comet C/2002 X5
Date
(0h UT) R.A. (2000)
h   m Dec.
°   ' Elong.
° Mag.
 Const.
 
Dec. 16 16 02.6 +44 13 70.6 7.4 Her.
Dec. 17 16 11.0 +43 35 69.8 7.3 Her.
Dec. 18 16 19.5 +42 54 68.9 7.2 Her.
Dec. 19 16 27.9 +42 09 68.0 7.1 Her.
Dec. 20 16 36.4 +41 22 67.0 6.9 Her.
Dec. 21 16 44.9 +40 31 66.0 6.8 Her.
Dec. 22 16 53.4 +39 36 64.9 6.7 Her.
Dec. 23 17 01.8 +38 38 63.8 6.6 Her.
Dec. 24 17 10.2 +37 37 62.6 6.5 Her.
Dec. 25 17 18.5 +36 32 61.3 6.4 Her.
Dec. 26 17 26.7 +35 24 60.0 6.2 Her.
Dec. 27 17 34.9 +34 13 58.6 6.1 Her.
Dec. 28 17 42.9 +32 59 57.2 6.0 Her.
Dec. 29 17 50.8 +31 41 55.7 5.9 Her.
Dec. 30 17 58.6 +30 20 54.2 5.7 Her.
Dec. 31 18 06.2 +28 57 52.7 5.6 Her.

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pooky 发表于 2002-12-17 17:17 | 显示全部楼层 来自: 中国–广东–汕头 电信

新彗星定名為「工藤.藤川」彗星

當天除了日本熊本県菊池郡西合志町的工藤哲生先生用20x120雙筒鏡發現外,香川県三豊郡大野原町的藤川繁久先生也差不多時間獨立發現此彗星、所以定名為「工藤・藤川彗星」(COMET C/2002 X5、KUDO-FUJIKAWA)
藤川先生於12月14日日本時間上午5時35分用口径16厘米反射望遠鏡發現。通過日本國立天文台渡部潤一先生向IAU報告。原來藤川先生也是彗星老獵手,六十年代開始已獨立發現五顆彗星,這次為第六顆。
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以下為藤川繁久先生以前發現的彗星:
藤川彗星(C/1969 P1)
大道.藤川彗星(C/1970 B1)
森.佐藤.藤川彗星(C/1975 T1)
Denning.藤川彗星(72P)
菅野.三枝.藤川彗星(C/1983 J1)
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ASKA 发表于 2002-12-18 17:57 | 显示全部楼层 来自: 中国–云南 联通

好漂亮

好漂亮耶
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