173P/Mueller
The comet or a star? Seiichi Yoshida remarked on the Comet ML, that the supposed comet is probably a star.
� 2009-03-18 by Bernhard Haeusler, Maidbronn, Germany. Stacked image centered on the stars: movement of the comet: 5"/15min. in PA293�. 3 x 5 min. exposure,
2009-03-18, UT 01:19 to 01:34, 12" SCT
f-7 +
CCD ST10XME, IR/UV-blocking filter
Star field
from POSS2/UKSTU Red
plate (created by the
STScI Digitized Sky Survey) The queried region: (my first measured position of 173P/Mueller for the MPC)
Star A close to the center of the image was determined from the NED Search as:
SDSS J113344.94+240403.5 11h33m44.9s +24d04m04s * ... ... 21.8g (= Star A)
This means,. the stars has a magnitude of 21.8 with g-filter. Here you find the Query result of the NED.
The reference star is Star B extracted from the NED:
SDSS J113342.66+240458.5 11h33m42.7s +24d04m59s * ... ... 21.1g (= Star B)
Star A and the reference Star B are measured with Astrometrica (MPC result):
Star A C2009 03 18.06385 11 33 44.89 +24 04 04.2 19.3
C B82 Star B is definitely visible on my image. It has a magnitude of 19.4 measured with Astrometrica.
Stas A is obviously a little bit fainter on my image, but it is comparable with the magnitude of Star B.
This means: The comet 173P/Mueller is unverifiable on my image.
MPC observation: computed with Astrometrica COD B82 NET CMC-14
0173P C2009 03 18.05670 11 33
45.17 +24 04 04.3 19.5 N B82
Gauss curve produced by Astrometrica. The total PSF is using the
aperture circle of 3 x 3 pixel around the brightest pixel. Photometry computed with FOCAS II, using the Multibox method: COD B82
10x10 20x20 30x30 40x40 50x50 60x60 SNR SB COD
173P
18/03/2009 01:26:47 19.53 18.51 17.96 17.53 17.14 16.83 3.3 19.6
B82 FoCAs II - 07/01/2009-b FOCAS II is a tool for photometry on the base of data coming from Astrometrica. Focas is basically using the .LOG file of Astrometrica. Explanation of the FOCAS II table headings:
Object, date and time are self-explaining.
second line:
Focas II is using the .log file of Astrometrica and is computing
the photometry under different apertures (10x10 ... 60x60).
Orbit of 173P/Mueller at March, 18 2009, Sun distance: 4.41 AU links: http://astrosurf.com/cometas-obs/index_i.htm Visual and CCD Observations and images from the "Cometas Obs" mailing list, using the Focas II format es.groups.yahoo.com/group/Cometas_Obs The Spanish comet observation group in Yahoo
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Copyright: The author of NEO Planner and all sites of this web is Bernhard Haeusler, Dettelbach, Germany, all rights reserved |