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原文完整版http://user.qzone.qq.com/446469755/blog/1331619267此次流星雨月亮反照率为1.5%,约-4等,距离太阳约11度。流星雨辐射点距离太阳约110度.国际流星组织的信息:北京时间4月22日13时30分天琴座流星雨极大,极大值为ZHR=18.(或可能接近90)爱尔兰阿马山天文台信息:今年没有爆发的可能性,上次爆发1922年ZHR约为320.下次爆发可能在2040年ZHR约为70.********************************************4月22日天琴座流星雨全球各地观看情况表(表格中数字单位为ZHR)
中国部分地区
| 极大时间北京
| 城市
| 郊区
| 农村
| 很黑地区
| 北京
| 04时16分
| 0.8
| 5
| 10.1
| 15
| 新疆乌鲁木齐
| 06时00分
| 0.9
| 5.2
| 10.4
| 15.4
| 新疆喀什
| 07时00分
| 0.9
| 5.3
| 10.7
| 15.9
| 西藏拉萨
| 06时22分
| 0.9
| 5.3
| 10.6
| 15.7
| 四川成都
| 05时30分
| 0.9
| 5.2
| 10.4
| 15.5
| 四川攀枝花
| 05时44分
| 0.9
| 5.2
| 10.4
| 15.4
| 四川南充
| 05时20分
| 0.9
| 5.2
| 10.4
| 15.4
| 云南丽江
| 05时50分
| 0.9
| 5.2
| 10.4
| 15.5
| 四川九寨沟
| 05时22分
| 0.9
| 5.2
| 10.4
| 15.5
| 云南西双版纳
| 05时46分
| 0.9
| 5.1
| 10.3
| 15.3
| 广西桂林
| 05时06分
| 0.9
| 5.1
| 10.2
| 15.2
| 海南三亚
| 05时10分
| 0.8
| 5
| 10
| 14.8
| 澳门
| 04时56分
| 0.8
| 5
| 10.1
| 15
| 香港
| 04时54分
| 0.8
| 5
| 10.1
| 15
| 台北
| 04时24分
| 0.8
| 5
| 10.1
| 15
| 上海
| 04时16分
| 0.8
| 5.1
| 10.2
| 15.1
| 湖南长沙
| 04时56分
| 0.9
| 5.1
| 10.2
| 15.2
| 河北张家口
| 04时20分
| 0.8
| 5
| 10.1
| 15
| 黑龙江漠河
| 03时00分
| 0.8
| 4.6
| 9.2
| 13.7
| 甘肃兰州
| 05时18分
| 0.9
| 5.2
| 10.4
| 15.4
| 台湾高雄
| 04时20分
| 0.8
| 5
| 10
| 15.9
| 台湾花莲
| 04时24分
| 0.8
| 5
| 10
| 14.9
|
国外部分地区
| 极大时间当地
| 城市
| 郊区
| 农村
| 很黑地区
| 澳大利亚港市
| 04时02分
| 0.3
| 1.8
| 3.7
| 5.5
| 荷兰首都
| 03时54分
| 0.9
| 5.4
| 10.9
| 16.2
| 智利北部
| 04时36分
| 0.6
| 3.4
| 6.8
| 10.1
| 西萨摩亚首都
| 03时20分
| 0.6
| 3.7
| 7.4
| 11
| 希腊首都
| 04时32分
| 1
| 5.8
| 11.5
| 17.2
| 新西兰奥克兰
| 04时36分
| 0.3
| 1.6
| 3.2
| 4.7
| 伊拉克巴克达
| 04分20分
| 0.9
| 5.6
| 11.3
| 16.8
| 泰国曼谷
| 04时46分
| 0.8
| 4.9
| 9.9
| 14.7
| 美国波士顿
| 03时22分
| 1
| 6.2
| 12.3
| 18.3
| 巴西巴西利亚
| 03时24分
| 0.7
| 4.2
| 8.4
| 12.4
| 匈牙利
| 03时20分
| 0.9
| 5.6
| 11.1
| 16.6
| 危地马拉
| 03时48分
| 1
| 5.7
| 11.5
| 17.1
| 古巴哈瓦那
| 04时14分
| 1
| 6
| 12.1
| 18
| 以色列
| 04时00分
| 1
| 5.7
| 11.4
| 17
| 英国伦敦
| 03时18分
| 0.9
| 5.5
| 11
| 16.4
| 西班牙马德里
| 04时46分
| 1
| 5.9
| 11.8
| 17.5
| 美国新奥尔良
| 03时42分
| 1
| 6.1
| 12.1
| 18.1
| 挪威奥斯陆
| 02时32分
| 0.8
| 4.8
| 9.6
| 14.2
| 法国巴黎
| 04时22分
| 0.9
| 5.6
| 11.3
| 16.8
| 冰岛雷克雅末克
| 02时38分
| 0.7
| 4.3
| 8.6
| 12.8
| 瑞典斯德哥尔摩
| 02时08分
| 0.8
| 4.8
| 9.6
| 14.3
| 日本东京
| 03时54分
| 0.8
| 4.9
| 9.9
| 14.7
| 美国华盛顿
| 03时48分
| 1
| 6.1
| 12.3
| 18.3
|
从以上表格可以看出北美洲为最佳观赏地区
**************************************************
详情:
1.IMO信息
活动时段: 4月16—25日; 极大时间: 4月22日, 13时30分BJ (λ⊙ = 32.32°), but may vary — see text;
ZHR = 18 (can be variable, up to 90);
辐射点: α 赤经= 271°, δ 赤纬= +34°; Radiant drift: see Table 6;
V∞ 速度= 49 km/s; r 亮度指标= 2.1;
TFC: α = 262°, δ = +16° and α = 282°, δ = +19° (β > 10° S). |
天琴座流星雨辐射点位置移动星图
The λ⊙ = 32.32° timing given above is the 'ideal' maximum found in IMO results from 1988—2000. However, the maximum time was variable from year to year between λ⊙ = 32.0°—32.45° (equivalent to 2012 April 21, 21h30m to April 22, 08h30m UT). Activity was variable too. A peak at the ideal time produced the highest ZHRs, ?6?5 23, while the further the peak happened from this, the lower the ZHRs were, down to ?6?5 14. (The last very high maximum was in 1982, when a shortlived ZHR of 90 was recorded.) The mean peak ZHR was 18 over the thirteen years examined.
While generally thought of as having a short, quite sharp, maximum, this investigation showed the shower's peak length was inconstant. Using the Full-Width-Half-Maximum time (the period ZHRs were above half the peak level), a variation between 14.8 to 61.7 hours was detected (mean 32.1 hours). The best rates are normally achieved for just a few hours even so. The analysis also confirmed that occasionally, as their highest rates occurred, the Lyrids produced a brief increase in fainter meteors. Lyrids are best viewed from the northern hemisphere, but are visible from many sites north and south of the equator. As the radiant rises during the night, watches can be carried out usefully after about 22h30m local time from mid-northern sites, but only well after midnight from the mid-southern hemisphere. New Moon on April 21 makes this year perfect for Lyrid maximum observing, and if the ideal peak time recurs, it should be best-seen from sites across much of North America, particularly the eastern half. Remember, other maximum times are perfectly possible!
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2.来自香港天文学会
相關流星群 :四月天琴座流星雨 (LYR)
出現日期 :4月16日至4月25日
極大日期(香港時間):4月22日(星期日)7時55分
月閃高峰期 :遲0.7小時
天頂每時出射率 ZHR:15 顆 (可能高至 90 顆)
速度 :每秒 49千米(中速)
亮度指標 :2.9(暗淡)
輻射點 (曆元 2000):赤經 18.1時/271.4°赤緯 +33.6°
注意:流星雨的高峰期時間,因觀測條件關係,很多時並非與香港出現流星雨的高峰時間一致。地球、月球及流星體的相對位置亦令月閃(流星撞擊月面產生的閃光)的預報高峰時刻與地球的流星雨預測高峰期有時間差異!
這個流星雨是地球經過 C/1861 G1 (Thatcher) 彗星在軌道上的殘留物所形成的。
以下預測均以香港標準時間表示
流星雨理論高峰時刻: 4月22日(星期日)7時55分
建議觀測期間: 4月22日由凌晨0時至5時30分
預料香港高峰時間:4月22日(星期日)凌晨4時52分
流星雨觀賞提示:
注意個人安全,不要單獨前往僻靜無人地區。出發前請知會家人或親友。
凌晨時份天氣寒涼,必須穿足夠禦寒衣服,保持身體溫暖!
找一個遠離城市或街燈,光害較少的黑暗地方。
注意避開有蛇、蟲、蟻出沒位置。
躺在躺椅子或草坪上,最好有地蓆、毯子或睡袋保護。
直望天空,盡可能選擇望見最大的天空範圍。
觀賞前先讓你的眼睛適應黑暗的環境30分鐘,這樣可以見較多的流星。
用肉眼欣賞,無需使用望遠鏡。
有意觀測這個流星雨的同好,可以利用智能手提電話輔助流星觀測,詳情請參閱以下介紹。
http://forum.hkas.org.hk/viewthr ... &extra=page%3D1
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3.爱尔兰阿马山天文台信息:
Introduction
Fig. 1. Space-temporal projection of p2000g1р-ids trails parts onto their minimal distance passages dirung the period 22.01.2009-21.07.2012 (correspondence between colours of the particles and their ejection velocities can be seen here).
Fig. 2. Detailed space-temporal projection of p2000g1р-ids trails parts onto their minimal distance passages dirung the period 22.01.2012-22.07.2012 (correspondence between colours of the particles and their ejection velocities can be seen here).
No encounters with 1 and 2 rev. Lyrid trails are found. Activity is not expected.
4.西格雷夫天文台信息:(月球照明1.5%)
LyridsApril 21-22
Frequency:
| | The swift and bright Lyrid meteors disintegrate after hitting our atmosphere at a moderate speed of 29.8 miles per second. They often produce luminous trains of dust that can be observed for several seconds.
| Parent Comet: C/Thatcher</DIV< td>
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5.Dark Sky Diary信息:
The Lyrids peak on 21/22 April 2012 is the first major shower peak in 15 months where the Moon is absent, meaning that you should get good views of this shower which has a ZHR of only around 20.
6.南非比勒陀利亚气象站信息:
Lyrids meteor streams are groups of meteoroids originating from dust grains ejected from Comet C / 1861 G1 Thatcher. These small dust grains (meteoroids) are distributed along the parent comet's orbit concentrated close to the comet nucleus with fewer grains farther away from the nucleus. Every time the Earth passes through this stream of dust particles (i.e. meteor stream), we experience what is known as a Lyrids meteor shower. These brief streaks of light from meteors, sometimes called "shooting stars", peak on Saturday night the 21st April 2012 when earth moves through the center of the dust trail left behind by the comet.
7.美国流星学会信息:
流星雨名称
| 活动时间段
| 最大
| 辐射点
| 速度
| 极大
| 时间
| 月龄
|
|
| 日期
| λΘ
| 赤经
| 赤纬
| km/s
| ZHR
|
|
| 天琴座流星雨(LYR)
| 4月16- 25日
| 4月22日
| 032.4°
| 18:08
| +32.9°
| 48.4
| 18
| 0400
| 01
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相关新闻链接:
国外
http://earthsky.org/astronomy-essentials/earthskys-meteor-shower-guide
http://www.jeffberkesphotography.com/2/Lyrids2012.html
夏威夷观测http://www.lovebigisland.com/hawaii-blog/lyrids-2012/
http://www.astronomerswithoutborders.org/gam2012-programs/program-schedule/955.html
南非比勒陀利亚气象站http://www.bashewa.com/wxyowindow.php
http://www.astronomylive.com/event/lyrids-meteor-shower-16-april-2012
更多http://astro-observer.com/searchResults.html?cx=partner-pub-3219508095459080%3Afv2y7o-5tec&cof=FORID%3A10&ie=ISO-8859-1&q=Lyrids2012&sa=Search
http://www.facebook.com/events/284810374902298/
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国内:(等待……) |
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