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[vsnet-chat 1564] (fwd) The discovery of C/1998 P1 (Williams)
- Date: Thu, 21 Jan 1999 14:58:04 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 1564] (fwd) The discovery of C/1998 P1 (Williams)
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
From peter_williams@nykline.co.jp Thu Jan 21 13:03 JST 1999
Date: Thu, 21 Jan 99 13:44:26 +0900
From: "Peter Williams"<peter_williams@nykline.co.jp>
To: <tkato@kusastro.kyoto-u.ac.jp>
Subject: Comet C/1998 P1 (Williams)
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Dear Taichi,
Regarding your vsnet-chat 1559 of January 18, you asked about the
discovery of Comet C/1998 P1. Below is the 'official story' which I
prepared for local Australian comet newsletters and periodical
magazine 'Sky & Space'. This gives a personal account of events
leading to this discovery while on my way to observing the dwarf nova
EK TrA. I trust you find this of interest and enjoyable. It was a
very unexpected and pleasant surprise for me! The text is stored on
my works computer so I send it from that location. Please feel free
to distribute all or part through the vsnet-chat or other lists.
Regards
Peter Williams, Heathcote NSW
pfwilliams@onaustralia.com.au
THE DISCOVERY OF COMET C/1998 P1 (WILLIAMS).
Peter Williams
Most people like to complain about the weather and, well, I guess I'm
just like the rest. August is usually associated with strong winds
but this year they were accompanied by driving rains which produced
flooding in many areas of eastern New South Wales.
My backyard observatory at Heathcote, on the southern extremity of
suburban Sydney, was partially flooded with 3cm of water when a nearby
drain became blocked by garden debris. Nearly 170mm of rain was
recorded at Heathcote during the first 9 days of August and I was
beginning to suffer the 'DTs' from a lack of starlight.
Perhaps better known for the observation of variable stars, I have
been fortunate enough to also observe a number of comets over the
years beginning with Comet Bennett, the Great Comet of 1970, and
sending the occasional total magnitude estimate to David Seargent of
the Australian Comet Section during this time.
Monday, August 10 was the first clear night of the month so, although
feeling tired after arriving home from work a little later than usual,
I ventured outdoors after dinner with binoculars in hand to catch up
on some of the brighter variable stars on my regular working list.
A normal night's observing at Heathcote involves preparation under
subdued lighting, a naked eye nova search along the Milky Way followed
by a search to near magnitude 8 in two selected areas with the 10x50mm
binoculars. This is followed by the binocular variables before moving
onto the telescopic stars. Each observing session can last between 30
minutes and several hours.
With the moon just two days after full there was a very narrow 'dark
window' before moon rise. I had used this time for the binocular
variables. After this I returned indoors to help with some domestic
duties and getting the children off to bed. Domestic duties complete,
I sat down with my wife, Linda, and feeling rather tired thought I may
retire early for the night.
However, having been clouded out for near two weeks I felt obliged to
show the 'right stuff' and check on the telescopic variables. In
hindsight, this proved a wise decision.
By 9.30pm local time and with the near full moon well above the
horizon, the roll-off roof of my observatory parted as I prepared for
observation with the 30cm F6 Newtonian reflector.
Working through my usual sequence of variable star fields, I commenced
low in the south west with SY Mus and DI Cru, followed by 8 other
irregular and unusual stars in the Cru-Mus-Cen region.
Then sweeping eastward at a low 72x magnification from Alpha Cir
towards the faint dwarf nova EK TrA, I almost fell of the three step
ladder used to reach the eyepiece as a bright comet-like object came
into view.
'Oh gosh, what have we here?' or words to that effect I muttered,
knowing only too well there should be no fuzzy blobs in that area of
sky.
A full millisecond or two later I forgot completely about EK TrA as
complete panic set in. Was it clear in New Zealand? Was it clear in
Victoria? As I shuffled through my charts to find that for EK TrA, I
pondered who else may be observing this field that evening. Having
located the chart I proceeded to plot the object's position then wait
and look for movement.
At the time of discovery the comet appeared large, round and diffuse
with no tail and a 13th magnitude stellar central brightening.
Through the 20x80mm binoculars it was estimated at magnitude 9.5 but
of somewhat smaller diameter than through the telescope at only 4
arcmin across.
Within half an hour clear movement towards the north west was evident
so I moved indoors at near relativistic speed to seek independent
confirmation. After several frustratingly unanswered phone calls, I
eventually raised David Seargent of the Australian Comet Section who
was able to provide verification.
At this stage even Linda, who is generally content to view the moon
once every second year, left the warmth and comfort of bed to become
only the third person on Earth to view the comet.
David kindly emailed the co-ordinates and magnitude estimates to the
International Astronomical Union's Central Bureau for Astronomical
Telegrams at the Smithsonian Astrophysical Observatory in Cambridge,
USA. The CBAT replied the next day with a request for more
information and additional positions to allow for establishing a
preliminary ephemeris.
I had never realised how long the daylight hours are as I waited for
nightfall!
Tuesday night was essentially cloudy at Heathcote except for several
fortunate clear patches which allowed me to relocate the comet and
establish an additional position. This was duly emailed to the CBAT.
Unknown to me, Gordon Garradd of Loomberah, near Tamworth, had learnt
of the comet through David Seargent and was busy measuring the comet's
position on CCD images obtained that night, providing the accurate
details needed by the CBAT.
IAUC 6986 was issued on Wednesday 12th August 1998 announcing the
discovery of Comet 1998 P1, much to the relief of all concerned.
Many emails and telephone calls from well wishers have since been
received, topping off several days of intense excitement. My two
minutes of fame have certainly been an experience I will long
remember. The help, encouragement and co-operation of local
identities such as David Seargent, Gordon Garradd and Rob MacNaught
played an important part in verifying this comet.
Looking back, however, this discovery was contributed to by a number
of fortunate circumstances.
Firstly, the sky was clear and calm that evening after more than a
week of strong winds and driving rain. Secondly, despite a near full
moon the decision was made to observe through the telescope. Thirdly,
had I delayed going outdoors a little longer I may not have observed
the field of EK TrA. Finally, had I not been monitoring a non-program
suspected variable a little to north of EK TrA, I may not have swept
northward to low magnification and onto the comet.
Luck may have played its part. However, I like to believe - tongue in
cheek - that I have been conducting a systematic search for comets, in
variable star fields, while looking in the wrong direction and under
full moon. Clearly, my methods have been vindicated!
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp