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Comet 46P/Wirtanen in November 2018

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#1 cbellh47

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Posted 03 November 2018 - 05:51 AM

Comet 46P/Wirtanen is passing through the southern sky constellation of Fornax in November 2018 and reaches southernmost declination on 2018-Nov-03. Sky motion has slowed and is near its minimum of 0.13 arcsec/minute. The position angle of a dust tail as it develops should shift during November. When the dust tail lengthens beyond the coma it is expected to develop some curvature, since the r and - v position angle vectors are near perpendicular. If an ion tail develops it should appear as a thin tail pointing away from the sun.

The coma of 46P was recently measured at 15 arc minutes in diameter and should increase noticeably during the month as the distance between Earth and comet decreases from 0.269 AU on 2018-Nov-02 to 0.120 AU on 2018-Dec-01. The coma is diffuse with stars visible inside as has been reported by Chris Wyatt. Color images should show an enlarging blue-green gas coma from CN, C3, and C2 emission. Visually a Swan filter can be used to enhance contrast as has been reported by Chris Wyatt.

Total visual magnitude has been steadily brightening from near magnitude 8.2 reported by Paul Camilleri on 2018-Nov-02 to about 5th magnitude by 2018-Dec-01 using either the 46P light curve by S. Yoshida or COBS.

Nuclear magnitudes have been steadily brightening from near magnitude 13.8 reported by J. G. Bosch on 2018-Oct-29 to about 11th magnitude by 2018-Dec-01.

R band Afrho measurements reported by the Spanish Comets-Obs group also show steadily increasing values which have ranged between 40 to 60 cm for aperture radius of 10,000 km during October 2018.

Water production was detected by Dave Schleicher at Lowell Observatory on 2018-Oct-06. Dave Schleicher detected OH using narrowband filter photometry on 6 October (r=1.38 AU). Haser models gave an OH production of Q(OH)=2.0×10^27 molecules/s. This converts to a water production rate of Q(H2O)=2.3×10^27 molecules/s or . Production rates for other species on the same date: Q(CN)=4.5×10^24 molecules/s, Q(C2)= 6.3×10^24 molecules/s, and Afrho(5260A) = 20 cm. See the UMd comet Wirtanen web pages for more info.DrAW58MUUAA1PZC.jpg


Edited by cbellh47, 03 November 2018 - 05:52 AM.


#2 aa6ww

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Posted 07 November 2018 - 02:41 PM

its still too low for me to observe it here in California.

 

Ralph



#3 Cirus

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Posted 07 November 2018 - 09:46 PM

Could a Svbony 1.25" UHC or 82A filter possibly help with visual contrast of the comet and tail?

#4 aa6ww

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Posted 08 November 2018 - 03:36 AM

I have a comet swan filter from Lumicon if this comet has an Ion tail but I havent heard that it does. The filter helps when there is an Ion tail. I have a 2" filter and also two 1.25" filters for my APM 100mm ED binoculars.  I always try the filter once a comet is in view. The last comet I followed closely was Comet 21/P a few months back.

 

...Ralph



#5 Waddensky

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Posted 08 November 2018 - 04:12 AM

Very interesting, thanks for sharing. 46P is moving north rapidly and will become visible from mid-northern latitudes in a few weeks. It's 'predicted' to reach naked-eye brightness, but the huge coma (one degree) makes it a better target for binoculars, I suppose. One to look forward to.




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