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关注5月的宝瓶座η流星雨!

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meteorobs 发表于 2005-4-28 22:37 | 显示全部楼层 |阅读模式 来自: 中国–天津–天津 电信

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宝 瓶 座 流 星 雨 (Aquarid meteor shower) 是 哈 雷 彗 星 (Halley's comet) 的 碎 片 (debris) 造 成 的 , 地 球 每 年 会 在 五 月 和 十 月 进 入 哈 雷 彗 星 的 轨 道 两 次 , 目 前 哈 雷 彗 星 离 地 球 很 远 , 大 约 是 在 木 星 (Jupiter) 的 轨 道 之 外 ; 不 过 , 哈 雷 彗 星 会 每 七 十 六 年 接 近 太 阳 , 下 一 次 哈 雷 彗 星 接 近 太 阳 是 在 二 零 六 一 年 ; 上 图 所 见 , 是 显 示 哈 雷 彗 星 的 轨 道 。
000503unac1.gif
 楼主| meteorobs 发表于 2005-4-28 22:38 | 显示全部楼层 来自: 中国–天津–天津 电信
科 学 家 指 出 , 宝 瓶 座 流 星 雨 会 在 每 年 五 月 三 日 後 的 十 天 内 出 现 , 而 在 五 月 四 日 至 六 日 出 现 得 最 频 繁 , 我 们 在 北 半 球 可 以 每 小 时 看 到 十 五 至 二 十 颗 流 星 , 而 在 南 半 球 则 可 以 看 到 多 达 每 小 时 六 十 颗 流 星。

宝 瓶 座 流 星 雨 将 会 在 宝 瓶 座 (Aquarius) 附 近 出 现 , 因 此 科 学 家 称 这 次 流 星 雨 为 宝 瓶 座 流 星 雨 , 宝 瓶 座 流 星 雨 最 频 繁 的 时 间 是 在 五 月 五 日 黎 明 时 分 ; 下 图 所 见 , 是 宝 瓶 座 流 星 雨 在 天 空 出 现 的 位 置1 。
000503unac2.gif
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 楼主| meteorobs 发表于 2005-4-28 23:42 | 显示全部楼层 来自: 中国–天津–天津 电信
下面是IMO(国际流星组织)对宝瓶座流星雨的背景介绍和对今年的的预测:

这是一个与1P/Halley彗星(哈雷彗星)有关的,高密度的流星群,就像十月份的猎户座流星雨,但是只能在赤道和南半球,天亮前几个小时内观测到。尽管最近几年甚至从北纬40°附近都得到了一些有用的结果,但是北方还是很少有该群流星的报告,然而为这个流星雨组织更多的观测者还是值得的。快速和明亮的流星,值得我们为辐射点的升起而等待,而且很多群内流星都留下变化的美丽余迹。当辐射点仍然很低的时候,宝瓶座eta的群内流星常有很长的轨迹,这使得观测者容易低估流星的速度,所以做这样的角速度记录时要多加注意。
同时也会让第一次看到这么长的流星的人留下深刻的印象。

宝瓶座流星雨有一个相对较宽的极大期,经常在五月初出现。从Tim Cooper对IMO在1988至1997年间的观测所进行的分析,和后来的目视、无线电观测的验证上看,ZHR(每小时天顶标准流星数)在5月3-10日间一般都会高于30颗。


今年的具体情况:

今年的极大时刻是世界时5月6日的0点,也就是北京时间的6日早上8点。
其实,由于极大期比较宽,观测者可以在5月3日到6日期间的每天凌晨的2点到4点之间注视着东南方的天空,对这个群开始监测。
而且今年的月相对于观测者来说也是非常有利,5月6日是农历的28,弯弯的残月从东北方的地平线升起时天色已经基本大亮了,所以不会对观测造成什么影响。

最后再说一句,如果在天亮之后(5点以后)开始利用无线电设备监测那就更好了!因为今年的极大时刻是北京时间的6日早上8点,这时正好可以利用无线电设备在家中监测,以便验证科学家们的预测。

下面是宝瓶座流星雨极大时的流星群的辐射点示意图
该图的对应时间和区域应该是在辐射点升起,凌晨2点左右的东南方的星空。
eta_aquarids.jpg
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活动星图 发表于 2005-4-29 00:01 | 显示全部楼层 来自: 中国–广西–桂林 电信
啊!得到了急需的资料,多谢马大爷! ^^
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 楼主| meteorobs 发表于 2005-4-29 00:10 | 显示全部楼层 来自: 中国–天津–天津 电信
你如果真的想观测好这次流星雨的话,就马上去勘测地点吧。。
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活动星图 发表于 2005-4-29 00:17 | 显示全部楼层 来自: 中国–广西–桂林 电信
找到了。
家里:楼顶
学校:田径场

^^
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heike 发表于 2005-4-29 01:05 | 显示全部楼层 来自: 中国–重庆–重庆–沙坪坝区 联通/联通信息港
5月6日在深圳能不能观啊?
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活动星图 发表于 2005-4-29 01:19 | 显示全部楼层 来自: 中国–广西–桂林 电信
那要看看老天爷给不给面子。还有光污染要考虑!
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LAMOST 发表于 2005-4-29 09:56 | 显示全部楼层 来自: 中国–天津–天津 电信
MQ:我们在北京也会有观测的.
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mars2 发表于 2005-4-29 10:57 | 显示全部楼层 来自: 中国–江苏–南京–江宁区 电信/奔浪网吧
等待ing....
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 楼主| meteorobs 发表于 2005-4-29 16:46 | 显示全部楼层 来自: 中国–天津–天津–河西区 联通
[quote:ced46c4bfd="heike"]5月6日在深圳能不能观啊?[/quote]

中国越是靠南的地区对于观测这次流星雨来说越是有利!
因为越往南走,宝瓶座流星雨的辐射点的位置越高,每小时所看到的
流星数就会越多! 8)
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 楼主| meteorobs 发表于 2005-4-29 16:47 | 显示全部楼层 来自: 中国–天津–天津–河西区 联通
[quote:e12196c8c3="LAMOST"]MQ:我们在北京也会有观测的.[/quote]

你们的观测地点定下来了吗?在哪里?
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 楼主| meteorobs 发表于 2005-4-29 19:09 | 显示全部楼层 来自: 中国–天津–天津–河西区 联通
宝瓶座η流星雨辐射点附近的星空示意图:
ldmsapp.jpg
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 楼主| meteorobs 发表于 2005-4-29 19:18 | 显示全部楼层 来自: 中国–天津–天津–河西区 联通
最新消息:
今天从meteorobs(IMO的讨论组)上收到了美国流星协会的Robert Lunsford
发表的世界时4月29日至5月5日的流星活动的细节预报和背景介绍:

Meteor Activity Outlook for Apr 29-May 5, 2005

This upcoming period will see the moon reaching its last quarter phase on
Sunday May 1. At this time the moon rises near 0100 local daylight time and
will be interfering with observations the remainder of the morning. As the
week progresses, the moon will rise later in the morning and its illuminated
portion will decrease as it approached its new phase. The estimated total
hourly rates for evening observers this week should be near two for those in
the Northern Hemisphere and three for those observers south of the equator.
For morning observers the estimated total hourly rates should be near six
for those located in the Northern Hemisphere and nine for those in the
Southern Hemisphere. Morning rates are reduced due to moonlight. These rates
assume that you are watching from rural areas away from all sources of light
pollution. The actual rates will also depend on factors such as personal
light and motion perception, local weather conditions, alertness and
experience in watching meteor activity.

The radiant positions listed below are exact for Saturday night/Sunday
morning April 30/May 1. These positions do not change greatly day to day so
the listed coordinates may be used during this entire period. Most star
atlases (available at science stores and planetariums) will provide maps
with grid lines of the celestial coordinates so that you may find out
exactly where these positions are located in the sky. A planisphere or
computer planetarium program is also useful in showing the sky at any time
of night on any date of the year. Activity from each radiant is best seen
when it is positioned highest in the sky, either due north or south along
the meridian, depending on your latitude. Meteor activity is not seen from
radiants that are located below the horizon. The positions below are listed
in a west to east manner in order of right ascension (celestial longitude).
The positions listed first are located further west therefore are accessible
earlier in the night while those listed further down the list rise later in
the night.

These are the showers that may be observed this week:

The Anthelion radiant is now centered at 15:40 (235) -19. This area of the
sky is located in eastern Libra, seven degrees west of the third magnitude
star Acrab (Beta Scorpii). These meteors were once called the Alpha
Scorpiids, as the radiant is located close to the bright orange star this
time of year. Since this radiant is large and diffuse, any slow to medium
speed meteor from eastern Libra or northwestern Scorpius could be a
candidate for this shower. The center of this area is best placed near 0200
local daylight time when it lies on the meridian and is highest in the sky.
At this time expect to see two shower members per hour no matter your
location.

Unlike most of the annual showers the antihelion source is produced by
debris from unknown objects orbiting in a direct motion like the earth.
These objects are most likely asteroids, which produce stony and metallic
debris whose density is much greater than material produced by comets. There
is also the possibility that some of this activity may be caused by the
"Jupiter family of comets", comets which have been altered by Jupiter's
gravity into much shorter orbits. This material collides with the earth on
the inbound portion of its orbit, before its closest approach to the sun.
Therefore we best see them just after midnight when we are facing the
direction from which this activity appears. The antihelion source is active
all year from an area of the sky nearly opposite that of the sun. The center
of this source will move approximately one degree eastward per day and
travels through many different constellations over the course of a year. It
may make sense to list these meteors as anthelions or "ANT" but a majority
of meteor organizations prefer that you list them from the constellation in
which the radiant is currently located or the constellation where the shower
reaches maximum activity. Observers who send their reports to the
International Meteor Organization (I.M.O.) should label these meteors as
Sagittarids (SAG).

The Beta Corona Australids (CAU) are listed among the radiants of the Dutch
Meteor Society. The current radiant position is located at 17:32 (263) -42.
This area of the sky is located in southeastern Scorpius, two degrees
northwest of the second magnitude star Sargas (Theta Scorpii). The best time
to view this activity is near 0400 local daylight time, when the radiant
lies highest in a dark sky. Rates at maximum activity (May 16) are only
three shower members per hour. Current rates would be still less than one
per hour. Observers in the Southern Hemisphere have an advantage with the
radiant rising much higher in their sky. With an entry velocity of 45
kilometers per second, a majority of these meteors will appear to move at
moderate speeds.

宝瓶座η流星雨:
The Eta Aquarids (ETA) are particles from Halley's Comet, which last passed
through the inner solar system in 1986. Even though this is now nineteen
years ago, material is still encountered every year in late April and
throughout most of May. We pass closest to Halley's orbit on May 5. Current
rates would be 1-2 per hour from a radiant located at 22:12 (333) -04. This
area of the sky is located in northern Aquarius, four degrees south of the
third magnitude star Sadalmelik (Alpha Aquarii). The best time to view this
activity is just before the start of morning twilight, when the radiant lies
highest in a dark sky. Observers located closer to the tropics have a better
chance of seeing these meteors as the radiant will rise higher into a dark
sky. Morning twilight is especially troublesome in the high Northern
latitudes, where the radiant is situated low in the sky at the start of
twilight. With an entry velocity of 66 kilometers per second, a majority of
these meteors will appear to move swiftly and produce a high percentage of
persistent trains.

The Sporadic rates for the Northern Hemisphere are now reaching their low
plateau for the year. From now through June morning sporadic rates will
remain near five per hour. During the dark evening hours perhaps two random
meteors can be seen per hour. Sporadic rates seen from the Southern
Hemisphere are slowly increasing toward a July maximum. From south of the
equator one would expect to see approximately five random meteors per hour
during the late morning hours and three per hour during the evening. Rates
are reduced during the morning hours for both hemispheres due to moonlight.

Anthelion (Sagittarids) 15:40 (235) -19
Hourly Rate = 2 N. Hemisphere, 2 S. Hemisphere

Beta Corona Australids (CAU) 17:32 (263) -42
Hourly Rate = 0 N. Hemisphere, <1 S. Hemisphere

Eta Aquarids (ETA) 22:12 (333) -04
Hourly Rate = 1 N. Hemisphere, 2 S. Hemisphere

Clear Skies!
Robert Lunsford
American Meteor Society
生活精彩在于想象力丰富和善于调整心态。幸福来自于深切感触、简单享受、自由思考以及被需要    ——地球历公元2006年2月10日上午11:55分。by  meteorobs
——————————
生命不熄, 观星不止!
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LAMOST 发表于 2005-4-30 14:49 | 显示全部楼层 来自: 中国–天津–天津–南开区 电信
[quote:b4c6962f12="meteorobs"][quote:b4c6962f12="LAMOST"]MQ:我们在北京也会有观测的.[/quote]

你们的观测地点定下来了吗?在哪里?[/quote]
房山区
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 楼主| meteorobs 发表于 2005-5-6 19:38 | 显示全部楼层 来自: 中国–天津–天津–河西区 联通
最新消息:
今天从meteorobs(IMO的讨论组)上收到了美国流星协会的Robert Lunsford
发表的世界时5月6日至5月12日的流星活动的细节预报和背景介绍:

Meteor Activity Outlook for May 6-12, 2005

This upcoming period will see the moon reaching its new phase on Sunday May
8. At this time the moon rises and sets with the sun and will out of the sky
all night long. As the week progresses the moon will enter the evening sky
as a thin waxing crescent but will still set before the active morning hours
arrive. The estimated total hourly rates for evening observers this week
should be near two for those in the Northern Hemisphere and three for those
observers south of the equator. For morning observers the estimated total
hourly rates should be near seventeen for those located in the Northern
Hemisphere and nineteen for those in the Southern Hemisphere. These rates
assume that you are watching from rural areas away from all sources of light
pollution. The actual rates will also depend on factors such as personal
light and motion perception, local weather conditions, alertness and
experience in watching meteor activity.

The radiant positions listed below are exact for Saturday night/Sunday
morning May 7/8. These positions do not change greatly day to day so the
listed coordinates may be used during this entire period. Most star atlases
(available at science stores and planetariums) will provide maps with grid
lines of the celestial coordinates so that you may find out exactly where
these positions are located in the sky. A planisphere or computer
planetarium program is also useful in showing the sky at any time of night
on any date of the year. Activity from each radiant is best seen when it is
positioned highest in the sky, either due north or south along the meridian,
depending on your latitude. Meteor activity is not seen from radiants that
are located below the horizon. The positions below are listed in a west to
east manner in order of right ascension (celestial longitude). The positions
listed first are located further west therefore are accessible earlier in
the night while those listed further down the list rise later in the night.

These are the showers that may be observed this week:

The Anthelion radiant is now centered at 16:08 (242) -20. This area of the
sky is located in northwestern Scorpius, just one degree south of the third
magnitude star Acrab (Beta Scorpii). These meteors were once called the
Alpha Scorpiids, as the radiant is located close to the bright orange star
this time of year. Since this radiant is large and diffuse, any slow to
medium speed meteor from eastern Libra, southwestern Ophiuchus or
northwestern Scorpius could be a candidate for this shower. The center of
this area is best placed near 0200 local daylight time when it lies on the
meridian and is highest in the sky. At this time expect to see two shower
members per hour no matter your location.

Unlike most of the annual showers the antihelion source is produced by
debris from unknown objects orbiting in a direct motion like the earth.
These objects are most likely asteroids, which produce stony and metallic
debris whose density is much greater than material produced by comets. There
is also the possibility that some of this activity may be caused by the
"Jupiter family of comets", comets which have been altered by Jupiter's
gravity into much shorter orbits. This material collides with the earth on
the inbound portion of its orbit, before its closest approach to the sun.
Therefore we best see them just after midnight when we are facing the
direction from which this activity appears. The antihelion source is active
all year from an area of the sky nearly opposite that of the sun. The center
of this source will move approximately one degree eastward per day and
travels through many different constellations over the course of a year. It
may make sense to list these meteors as anthelions or "ANT" but a majority
of meteor organizations prefer that you list them from the constellation in
which the radiant is currently located or the constellation where the shower
reaches maximum activity. Observers who send their reports to the
International Meteor Organization (I.M.O.) should label these meteors as
Sagittarids (SAG).

The Beta Corona Australids (CAU) are listed among the radiants of the Dutch
Meteor Society. The current radiant position is located at 18:16 (274) -41.
This area of the sky is located in western Corona Australis, seven degrees
northeast of the second magnitude star Sargas (Theta Scorpii). The best time
to view this activity is near 0400 local daylight time, when the radiant
lies highest in a dark sky. Rates at maximum activity (May 16) are only
three shower members per hour. Current rates would be less than one per
hour. Observers in the Southern Hemisphere have an advantage with the
radiant rising much higher in their sky. With an entry velocity of 45
kilometers per second, a majority of these meteors will appear to move at
moderate speeds.

The Eta Lyrids (IAA) are produced by comet IRAS-Araki-Alcock, which passed
very close to the Earth twenty two years ago this May. Weak activity from
this radiant has been seen in most years from May 5 through May 17, with
maximum activity occurring on May 9. The current radiant position is located
at 19:08 (287) +44. This area of the sky is located in northeastern Lyra,
five degrees northeast of the zero magnitude star Vega (Alpha Lyrae). The
best time to view this activity is just before the start of morning
twilight, when the radiant lies highest in a dark sky. With an entry
velocity of 44 kilometers per second, a majority of these meteors will
appear to move at moderate speeds.

宝瓶座η流星雨:

The Eta Aquarids (ETA) are particles from Halley's Comet, which last passed
through the inner solar system in 1986. Even though this is now nineteen
years ago, material is still encountered every year in late April and
throughout most of May. We passed closest to Halley's orbit on May 5.
Current rates should still be 10-15 per hour from a radiant located at 22:40
(340) -01. This area of the sky is located in northern Aquarius, one degree
southeast of the fourth magnitude star Eta Aquarii. The best time to view
this activity is just before the start of morning twilight, when the radiant
lies highest in a dark sky. Observers located closer to the tropics have a
better chance of seeing these meteors as the radiant will rise higher into a
dark sky. Morning twilight is especially troublesome in the high Northern
latitudes, where the radiant is situated low in the sky at the start of
twilight. With an entry velocity of 66 kilometers per second, a majority of
these meteors will appear to move swiftly and produce a high percentage of
persistent trains.

The Sporadic rates for the Northern Hemisphere are now reaching their low
plateau for the year. From now through June morning sporadic rates will
remain near five per hour. During the dark evening hours perhaps two random
meteors can be seen per hour. Sporadic rates seen from the Southern
Hemisphere are slowly increasing toward a July maximum. From south of the
equator one would expect to see approximately seven random meteors per hour
during the late morning hours and three per hour during the evening.

Anthelion (Sagittarids) 16:08 (242) -20
Hourly Rate = 1 N. Hemisphere, 2 S. Hemisphere

Eta Lyrids (IAA) 19:08 (287) +44
Hourly Rate = 1 N. Hemisphere, 0 S. Hemisphere

Beta Corona Australids (CAU) 18:16 (274) -41
Hourly Rate = 0 N. Hemisphere, <1 S. Hemisphere

Eta Aquarids (ETA) 22:40 (340) -01
Hourly Rate = 10 N. Hemisphere, 10 S. Hemisphere

Clear Skies!
Robert Lunsford
American Meteor Society
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永恒菜鸟 发表于 2014-5-9 14:27 | 显示全部楼层 来自: 中国–浙江–丽水 电信
最近天气不好,估计要悲剧了。。。
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suhuasky 发表于 2014-5-9 15:58 | 显示全部楼层 来自: 中国–湖南–常德 电信
楼上挖坑
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