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Messages 16109 - 16139 of 16183   Newest  |  < Newer  |  Older >  |  Oldest
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16139
I have imaged this comet on Nov. 17.52 UT remotely from D25 Tzec Maun Observatory. I also had some doubt about its magnitude - certainly brighter than 17.6m,...
Roman Kostenko
roman.white
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Nov 20, 2009
10:27 am
16138
Rob, Sincere thanks for your image and kind words. 169P is now approaching perihelion ( T 2009 Nov. 30, q=0.608 AU ), developing a wide faint coma. A very dark...
Juan José Gonzá...
jjgsgp
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Nov 19, 2009
2:35 pm
16137
I imaged it on Nov. 10.00 in remote from San Pedro de Atacama : 0169P C2009 11 10.00035 18 06 24.84 -21 36 40.3 17.0 N I10 Francois...
francois kugel
fkspect
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Nov 19, 2009
1:17 pm
16136
Interesting. I imaged the comet's position on Nov 11.4 and nothing was visible brighter than mag 13. So this looks like a very recent development. Terry...
terryjlovejoy
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Nov 19, 2009
1:08 pm
16135
Hi Juan! I managed to get a rough widefield image of the field tonight in fairly poor sky conditions (dust). 169P shows (just), but it appears to be...
kaufman_rob
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Nov 19, 2009
12:21 pm
16134
169P/NEAT: 2009 Nov. 18.77 UT: m1=9.2, Dia.=4', DC=2/, 20 cm SCT (100x). [ Significantly brighter than expected. Elongated wide coma with faint outer region....
Juan José Gonzá...
jjgsgp
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Nov 18, 2009
10:42 pm
16133
Dear all: Concerning comet 107P we need high precision photometry to detect even minute changes in its brightness. In that regard there is a nice calibration...
iferrinv
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Nov 16, 2009
5:33 pm
16132
Hi all, I first tried to spot C/2009 Q4 Boattini on October 21 in my 37cm reflector but was unable to see it. This Sunday morning Nov. 15 I was surprised to ...
Bob King
cometlynx
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Nov 16, 2009
5:20 pm
16131
Giovanni is correct, of course. Ignacio...
iferrinv
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Nov 16, 2009
5:14 pm
16130
Hi all, I have updated my analysis of the currently observable comets. You can find them at http://kometen.fg-vds.de/aktause.htm Regards, Andreas PS: third(!)...
kammerer_a
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Nov 16, 2009
4:12 pm
16129
Hi all, I have updated my analysis of the currently observable comets. You can find them at http://kometen. fg-vds.de/aktause.htm Regards, Andreas PS: second...
kammerer_a
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Nov 16, 2009
4:09 pm
16128
Hi all, I have updated my analysis of the currently observable comets. You can find them at http://kometen.fg-vds.de/aktause.htm. Regards, Andreas...
kammerer_a
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Nov 16, 2009
4:03 pm
16127
Comet 81P has developed a nice tail on images this morning Twitter: http://twitter.com/cbellh47 Flickr: http://www.flickr.com/photos/cbellh47/ Facebook:...
Charles Bell
charbell...
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Nov 16, 2009
10:55 am
16126
Thank you Dimitry and Charles very much! Those will both work. Gratefully yours, Bob ... [Non-text portions of this message have been removed]...
Bob King
cometlynx
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Nov 15, 2009
9:53 pm
16125
... Bob, You can find comet-style orbital elements for 107P with dates of perihelion and info about close approaches at Kazuo Kinoshita home page: ...
Dimitry Chestnov
astroched
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Nov 15, 2009
7:59 pm
16124
Hi everyone, Does anyone have orbital elements for 107P? I found an incomplete set online but none that list the perihelion date and distance for this...
Bob King
cometlynx
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Nov 15, 2009
7:54 pm
16123
Dear Rob McNaught, ... Thank you for your information. I read IAUC 9087 again, and I see that you discovered P/2009 U4 on Oct. 23, and then you found the...
Seiichi Yoshida
seiichi_yosh...
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Nov 14, 2009
7:25 am
16122
Dear Rob Matson, Thank you for your comments. I guess the next return of P/2009 Q1 (Hill) can prove the linkage of your data in 1996 and 1998. Best regards, ...
Seiichi Yoshida
seiichi_yosh...
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Nov 14, 2009
7:25 am
16121
Hello Francois and all. this morning 29P measures bring the same result as your observations. nuclear mag. 13.71 nuclear magn. 10" coma diameter = 9.6" ...
gustavo
gustavo_muler
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Nov 12, 2009
6:54 am
16119
Hello, 29P in outburst again : Nov. 09.22 mag.16.3 (dia=20") Nov. 12.22 mag.13.3 (dia=20") Francois Kugel #A77...
francois kugel
fkspect
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Nov 12, 2009
6:26 am
16118
(4015) Wilson-Harrington was an object of study by the Midcourse Space Experiment (MSX) mission Mission images are available in the Planetary Data System MSX...
Charles Bell
charbell...
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Nov 11, 2009
7:09 pm
16117
Dear Ignacio and all. ... Science works on data and experimental facts, and here we have only *one* observational evidence about a certain occurence. Then,...
gvnn64@...
gvnn64
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Nov 11, 2009
5:20 pm
16116
Hi everyone, I am happy to see this worthwhile discussion on this most interesting object, and like the other posters I would encourage physical observation ...
Alan Hale
ahale15
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Nov 11, 2009
4:47 pm
16115
I agree with Richard Miles that this is how science works. So it is fascinating to see so many hypothesis poping up. In this regard I would like to point out...
iferrinv
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Nov 11, 2009
4:26 pm
16114
Giovanni, I guess this is how science works, people come forward with options for working hypotheses and these are then compared with experimental observation....
RICHARD MILES
gallileo99uk
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Nov 11, 2009
10:47 am
16113
Dear Richard yours is a fashinating working hypothesis (as there are many others). Obviously, without a robust experimental support, I'm afraid it will remain...
gvnn64@...
gvnn64
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Nov 11, 2009
9:58 am
16112
Dear Giovanni, Some meteorites and presumably asteroids contain a significant proportion of hydrated minerals. Energetic particles from a solar flare would...
RICHARD MILES
gallileo99uk
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Nov 11, 2009
9:47 am
16111
Dear all, In the case of non-main belt, NEO comets like 107P (apollo) and 162P (amor) the tails have been found to be of Ionic nature (107P Yanga Fernandez et ...
Juan Lacruz
juan_lacruz
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Nov 11, 2009
8:55 am
16110
Dear Richard and all. ... In the few instances where asteroidal object have shown discontinuous signs of cometary activity (e.g. the so called "main belt...
gvnn64@...
gvnn64
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Nov 11, 2009
8:43 am
16109
I was tempted to try 107P from SSO (0.61-m, no filter) during this lunation and stack a bunch of 90-second images. On clear nights, I routinely get down to...
Matson, Robert D.
rdotdaneelol...
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Nov 10, 2009
10:28 pm
Messages 16109 - 16139 of 16183   Newest  |  < Newer  |  Older >  |  Oldest
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