Well this was a bit of a surprise.... I had not
downloaded the STEREO images data for a good couple of weeks. I have been
restricting my data usage due to changing personal circumstances(got to get a
real job), so not as active with this stuff. Also I have been working with
processing,org software exploring a few concepts.
Any way, the image viewer I have been working on needed
some current data so I downloaded and processed the FITS images for
20140204 into PNG's. Scanning around the edges I saw this fuzzy move up and
left near the top edge. A very not usual place for a fuzzy. It moved fast and
was almost out of the FOV. So reported to Stereo Hunter Forum and to Mr.
Sungrazer, could be a new STEREO comet....
Then I realized that this was moving out of the FOV and
should have been detectable a few days earlier. So, got to downloading 20140202
FITS data. IT was lower down and much brighter, hmm....must have been there for
a good number of days.
Checked out the online SECCHI images for COR2A, after a
detection report on STEREO Hunter forum. Quite evident as it crossed the COR2A
FOV from lower right to upper left quarter, crossing the center of view.
the dotted line across the centre is the comet(20140131) the angled lines are stars. |
over night the other members of the STEREO Hunter forum
got active and confirmed the comet and even measured an estimate of the comets
orbit. From Man-to
"As a
quick attempt I assumed eccentricity e=1 for this object in FIND_ORB, thereby I
got the following result:
Orbital elements: WATK14A
Perihelion 2014 Feb 18.476940 +/- 0.268 TT; Constraint: e=1
Epoch 2014 Feb 4.0 TT = JDT 2456692.5 Earth MOID: 0.2865 Ve: 0.0406
q 0.51008071 +/- 0.000731
H 1.2 G 0.15 Peri. 56.86757 +/- 0.25
Node 283.34633 +/- 0.0018
e 1.0 +/- 0 Incl. 135.39576 +/- 0.032
From 86 observations 2014 Feb. 1-4; mean residual 29".611.
Perihelion 2014 Feb 18.476940 +/- 0.268 TT; Constraint: e=1
Epoch 2014 Feb 4.0 TT = JDT 2456692.5 Earth MOID: 0.2865 Ve: 0.0406
q 0.51008071 +/- 0.000731
H 1.2 G 0.15 Peri. 56.86757 +/- 0.25
Node 283.34633 +/- 0.0018
e 1.0 +/- 0 Incl. 135.39576 +/- 0.032
From 86 observations 2014 Feb. 1-4; mean residual 29".611.
Cheers,
Man-To
--------------------------------------------------
Man-To Hui (Cantonese)
Wentao Xu, Wen-Tao Hsu (Mandarin Chinese)
Astrosite: comethunter.lamost.org
Blog: pachacoti.wordpress.com "
--------------------------------------------------
Man-To Hui (Cantonese)
Wentao Xu, Wen-Tao Hsu (Mandarin Chinese)
Astrosite: comethunter.lamost.org
Blog: pachacoti.wordpress.com "
This put the comet some were in the Northern morning
twilight according to my Starry night settings.
In the next few days I looked for the comet in Stereo
HI2A wide field images across 20140210-15, the orbit put the comet in the upper
right quarter of the FOV. No, luck the comet had faded to below mag 10 and was
likely lost to detection and being small and in the twilight not good prospects
for ground detection. An Mpec was released with a proposed orbit solution a few
days later, http://www.minorplanetcenter.net/mpec/K14/K14C25.html
and softcmt file for starry night updated. The comet now has a name C/2014 C2 STEREO.
and softcmt file for starry night updated. The comet now has a name C/2014 C2 STEREO.
So, this morning of 20140220, the tweets from Sungrazer indicated that Hidetaka Sato had used Itelescope T11 to get a set of
confirmation images, very close to the calculated orbit. A much appreciated effort. Amazing that this small
comet was ground detected, and still showing a small active tail.
image credit Hidetaka Sato |