Comet discoverers & Comet
discoveries by amateurs
1978 - 1999
Last update: 18. March 2017
|Discoveries from 2000 to 2009
||Discoveries 2010 to 2019
||Discoveries 2020 to now
In 1990, with a total of 10 discoveries, 3 were discovered by amateurs:
In 1991, with a total of 22 discoveries, 6 were discovered by amateurs:
In 1992, with a total of 13 discoveries, 7 were discovered
In 1993, with a total of 10 discoveries, 1 were discovered by amateurs:
In 1994, with a total of 11 discoveries, 6 were discovered by amateurs:
In 1995, with a total of 6 discoveries, 4 were discovered by amateurs:
In 1996, with a total of 44 discoveries, 4 were discovered by amateurs:
Kazimieras Cernis - Tsuruhiko Kiuchi - Yuji Nakamura - C/1990 E1
IAUC 4980 announced a new comet discovery on
March 14 by Kazimieras Cernis from Vilnius,Lithuania
with his 120 mm f/5 refractor (magnification X35, FOV 2
near Vilnius, Lithuania (more exactly, in Lavariskes, 25 km to east from
Two days later independent discoveries where made visually by two Japanese amateurs, Tsuruhiko Kiuchi with a 25x150 binocular and Yuji Nakamura with a 20x120 binocular. The comet was also confirmed by Alan Hale(USA). At the moment of the discovery the comet appeared like a diffuse object of 9th mag and 2’ diameter. The comet reached a peak of 8 mag. during that apparition.
from Kazimieras Cernis:
I used 631 hours of visual searching (during 358 nights, from discovery of comet C/1983 O1)
Kazimieras Cernis (b.1958) the discovery of C/1990E1 was the 3rd. for him after the discoveries of C/1980 O1 and C/1983 O1.
David H. Levy - C/1990 K1
Another comet discovery for David H. Levy was announced on IAUC 5017 on 1990 May 20 during his comet hunting with his 0,41m f/5 reflector. Alan Hale (Las Cruces, USA) with his 0,4m reflector and Charles Morris (Pine Mountain Club, USA) with his 0,26m reflector confirmed the discovery the day after. At the moment of the discovery the comet was estimate of 9-10 mag, well condensed and a coma of 1-2’. The comet reached a peak of 4th. mag in late summer.
Copyright Wendee Levy
Tsuchiya-Kiuchi - C/1990 N1
IAUC 5052 announced a new comet discovery on July 13, 1990N1, by Kiyoshi Tsuchiya (Asahikawa, Hokkaido) with a f/4 camera + T-Max film and Tsuruhiko Kiuchi (Usuda, Nagano) with a 25x150 binoculars. The comet appeared of 8/9 mag at the moment of the discovery.
Coypright Gerald Rhemann 23-10-1990
(b.1954) is a comet-researcher from Usuda-machi,
Minamisaku-gun, Nagano Prefecture. This discovery is the 2nd. for him here an interview of his
typical day, an intensive day divide by work and comet hunting:
"Look more closely from farther away. That is my way of thinking."
Kiuchi's daily regimen starts at 7 a.m. He has to be in his office at 7:30. He departs for his workshop between 5:30 and 6:30 p.m. This workshop is like a child's secret club house, a sanctuary in which he can relax and enjoy the moment. Upon returning home, he bathes, finishes his evening meal, and then goes out to star-gaze. The normal routine for his observation runs from an hour and a half after sunset until an hour and a half before sunrise. He only takes breaks or is unable to make his observations during inclement weather, on days when he has to give lectures, and during the five-day cycle of the full moon. Aside from these restrictions, he performs his observations every day.
Howard Brewington -
On Jan 7 Howard Brewington (Cloudcroft, USA) discovered is second comet, 1991A1, during his session of comet hunting with his 0,41m reflector (IAUC 5155). The comet was rapidly confirmed by Alan Hale with a 0,20m reflector. As reported on IAUC 5159 the comet was independently discovered also by Tsuruhiko Kiuchi (Usuda, Japan) with his 25x150 binocular and William Bradfield(near Adelaide, Australia). All observer estimated the comet around 9 mag.
B. G. Marsden, Center for Astrophysics, notes that preliminary orbital elements from the above observations strongly resemble those of P/Metcalf (1906 VI). Consequently the comet was numbered 97P/Metcalf-Brewington.
Howard Brewington with his personal observatory near
Cloudcroft, New Mexico
He was born in 1952 in South Carolina. For years he visually sweeping the night sky with his home-built reflecting telescopes, his first comet was C/1989W1 discovered from South Carolina. To improve his chances of additional finds, he moved to southern New Mexico in the fall of 1990 and built a comet hunting observatory on a mountain ridge east of Cloudcroft. From 1991 to 1996, the relocation issued four more visual discoveries (97P,C/1991Y1,154P, 1996N1). Brewington prophesied the end of visual comet discoveries and wrote about it in the Summer 1995 issue of CCD Astronomy magazine in an article titled "The Future of Comet Hunting”. Brewington stopped comet hunting in 1999, moved back to South Carolina, and enrolled at the University of South Carolina in Columbia. He graduated with honors in the summer of 2002 and was hired by year's end as a 2.5-meter telescope operator through the Astronomy Department of New Mexico State University. From 2002 to 2015, he worked at the Apache Point Observatory in Sunspot, New Mexico as part of the Sloan Digital Sky Survey. Brewington, now retired, lives in Las Cruces, New Mexico. He is a member of the Astronomical Society of Las Cruces and often attends national star parties.
Masaru Arai - C/1991 A2
IAUC 5157 announced a new comet discovery, C/1991A2, by Masaru Arai (Yorii, Japan) on Jan 5. From an image taken with a 0.16m reflector. The comet appeared diffuse with central condensation with a total magnitude around 12. The comet was confirmed by R. McNaught (Siding Spring, Australia).
(b.1952) is a prolific discoverer of asteroids with a total of 45
discoveries in collaboration with Hiroshi Mori.
IAUC 5291 announced another comet discovery for David H. Levy (Tucson, USA) on June 14th with his 0,41m f/5 reflector. The comet showed a 3’ coma and a 8th. magnitude. This object turned to be a periodic comet and will return around 2042. As suggested by Levy on his book, the comet is parent of the August pavonid meteor shower. According to Levy there is a possibility that it may be the same as the comet of 1499. In that year Chinese and Korean observers observed a comet pas from Hercules through Draco, and the Little an Big Dippers.
William Bradfield (Australia) discovered his 15th comet on January 31.74 as reported on IAUC 5442. The comet was found in the morning sky, on the borders of Scorpius, Lupus and Norma as it was brightening on its way to perihelion. Of 10 magnitude, it was diffuse and without condensation. Paul Camilleri of Cobram, Victoria, Australia found images of it on pre-discovery Kodak T-Max 400 plates taken with an 85 mm lens on Jan 30.7. Albert Jones observed the comet on 1992 February 13.7, making it 10.1 in his 0.32-m reflector. Cometary activity evidently decreased rapidly as the comet approached perihelion as it should have been around 7m at this time. Poor observations were made for this comet.
Don Machholz (Colfax, USA) reported the discovery of a probable 10 mag. comet to the CBAT on March 31st and the estimated daily motion indicated a possible identity with another object reported to the bureau on March 27th. This object had been discovered by Zenichi Tanaka (Yodoe, Japan) on March 24th, but an incorrect daily motion was given (IAUC 5487). The comet was also confirmed by Alan Hale on April 1st. At discovery it was moving north in the morning sky in Pegasus and passed through Andromeda in mid April on its way to perihelion on April 22nd.
Copyright H. Mikuz, 1992 Apr.
William Bradfield discovered his 16th comet, a 10 magnitude diffuse object without central condensation on May 3.81 as reported on IAUC 5514. The comet was in the morning sky, moving east in Cetus, and brightening towards perihelion on May 25th. Its solar elongation decreased and few observations of it were made. Only 10 astrometric positions were obtained, the last taken on June 4th.
Donald Machholz discovered his sixth comet, a diffuse 9 mag. object with condensation, using 27x120 binoculars on July 2.46 as reported on IAUC 5553. The comet was in the morning sky, moving SE on the Perseus/Auriga border and had been brightening on its way towards perihelion. The comet was possibly within discovery range for most of the previous month. No section observations were received as the solar elongation was poor and it faded after discovery.
Howard J. Brewington - P/1992 Q1
Howard J. Brewington reports the discovery of his fourth comet with his 0,41m reflector on August 28th. The comet appeared very small, diffuse and around 10 magnitude. Brewington had spent 99 hours comet hunting before finding this comet. As reported on IAUC 5596 the comet was confirmed by A. Sugie and T. Kojima from Japan. The first published orbit came on September 1st., when B. G. Marsden calculated a parabolic orbit using 11 positions from August 28 to 31. The perihelion date was given as 1992 June 20.97. Marsden considered the orbit "somewhat uncertain." Following S. Nakano's (Sumoto, Japan) remark "that the comet is evidently of short period", Marsden calculated an elliptical orbit that was published on September 27th. Using 18 positions obtained during the period of August 28th to September 26th., he determined the perihelion date as June 4.05 and the period as 8.65 years. Syuichi Nakano published a new orbit, he took 82 positions obtained during the period spanning 1992 August 28th. to 1993 March 30th and applied perturbations by planets and minor planets, the result was that the comet passed perihelion on 1992 June 7.79. Nakano then integrated the motion forward and predicted the comet would next arrive at perihelion on 2003 February 18.84. This comet was recovered by Fernanda Artigue, Herbert Cucurullo, and Gonzalo Tancredi (Molinos Astronomical Observatory, Montevideo, Uruguay) on 2002 August 26.98; so the comet was numbered as 154P/Brewington.
IAUC 5620 reported a new comet discovery on September 26th. by Tsuruhiko Kiuchi, with the suggestion that it might be P/Swift-Tuttle with perihelion time in mid-December. Kiuchi used a 25x150 binoculars and described the comet diffuse without condensation with a coma of 4'. Confirmation of the discovery by several observers in Canada, the U.S. and Japan leaves no doubt that this identification with the Perseid parent comet is correct. The identification in turn confirms the suggestion that Kegler's 1737 observations were indeed of P/Swift-Tuttle. Finally the comet was linked with 1737 II- 1862 III, so was recalled 109P/Swift-Tuttle.
Copyright Misunori Tsumura
Nobuo Oshita - C/1992 W1
Nobuo Ohshita (Furukawa-machi, Japan) discovered an 11 mag. comet with 25x150B on November 24.85 and confirmed it with images taken with a telephoto lens on T-Max film on November 28.8 - 30.8 IAUC 5668 (Iauc 5668). The comet was moving NE in Virgo as it emerged from conjunction in the morning sky and faded after discovery. No visual observations of this comet were obtained.
Yoshio Kushida - Osamu Muramatsu - P/1993 X1
IAUC 5903 announced a new comet discovery on December 8.7UT, 1993X1, by Yoshio Kushida and Osamu Muramatsu of Yatsugatake South Base Observatory, Japan, during a photographically session of comet hunter using a 0,25m reflector. At discovery the comet was moving east and was diffuse with a central condensation and a coma of about 1'-2' diameter and a magnitude of 16,5. Several Japanese astronomer (T. Kojima, T. Urata , A. Nakamura T. Kobayashi) confirmed the comet during the following days.
The comet was recovered on 2000
October 3.72, when T. Oribe (Saji Observatory) obtained CCD images
with the 103-cm reflector, and sub sequentially was numbered
(b.1957) is a seismologist and amateur astronomer. Is a prolific
asteroid discoverer with a total of 56 and also discovered two
periodic comets (144P,147P).
Osamu Muramatsu (b.1949). He worked at the planetarium of Sibuya, he is also an amateur astronomer. He discovered the periodic comet 147P and 71 asteroid, more of them with Y. Kushida.
Yoshio Kushida - C/1994 A1
discovered his second comet on January 8.8UT with a 0.10-m f/4.0
patrol camera. The comet appeared with a strong central condensation
with coma diameter about 1'-2'. The comet was estimate about 12/13
magnitude and was confirmed by several Japanese astronomer including
T.Kojima, T. Urata and A. Nakamura. (IAUC 5918)
The comet's next perihelion date was 2001 June 27 and it was recovered by C. E. Delahodde and O. R. Hainaut (European Southern Observatory, La Silla) on 2000 July 25. After this the comet was numbered as 144P/Kushida.
Kesao Takamizawa - David H. Levy - C/1994 G1
and David H. Levy report their discoveries of what appears to be the same
comet observed between April 14-15. K. Takamizawa (Saku-cho, Japan).
Estimated of 12.5 magniutde on his two 4-min photographic films,
taken with a 0.10-m f/4.0 camera. The comet appeared diffu with
central condensation and coma diameter about 1'. David H. Levy
(Tucson, USA) observed the object visually with his 0,41m reflector.
Copyright Norbert Mrozek 1994 May 13
Kesao Takamizawa - C/1994 J2
Kesao Takamizawa discovered his 4th and last comet on 1994 May 6.7 UT with a 0.10-m f/4.0 patrol camera. The comet appeared of 11 magnitude with a strong central condensation and coma diameter about 1'. (IAUC 5986)
Coyright H. Mikuz, 1994 May.
Masamitsu Nakamura - Hideo Nishimura - Donald E. Machholz - C/1994 N1
IAUC 6013 announced a new comet discovered by
three amateur astronomers:
Masamitsu Nakamura (Hamamatsu, Shizuoka-Ken, Japan) and Hideo Nishimura (Kakegawa, Shizuoka-Ken, Japan) discovered the comet with a 25x150 binoculars independently on July 5.7UT. They estimated the object of 9 mag. and a coma of 2,5’(Nishimura) and 5’(Nakamura). Donald Machholz (Colfax, USA) discovered the comet on July 6.4UT with his 27x120, he estimated about 10.5 magnitude.
Donald E. Machholz - P/1994 P1
Donald E. Machholz discovered another comet visually with a 0.25m reflector on August 13th. He estimated about 10 mag. with little condensation and a coma diameter of 3’-4’(IAUC 6053). The comet was confirmed by T. Kojima. Michael Jäger (Vienna, Austria) reported his discovery of a second comet just 48 arc minutes from comet Machholz 2 on August 28.04. He said it appeared to have the same motion as Machholz and estimated the magnitude as 11. This comet continued being observed during the days that followed. Fourth and fifth objects were found by Pravec on September 4.1 and confirmed elsewhere. Letter designations were assigned to the 5 comets on September 21. The primary comet was the most westward and was designated "A". Working eastward, "B" was the fourth comet found, "C" was the third comet, "D" was the second comet, and "E" was the fifth comet. Interestingly, Pravec reported that CCD images obtained on October 5.14 indicated "D" exhibited two condensations within its coma. The comet return again on 1999 with only fragment “A” and later was recovered the fragment “D”, so it was numbered as 141P.
Donald E. Machholz - C/1994 T1
Donald E. Machholz reported his 3rd. visual discovery of a comet in 1994! (IAUC 6091) The comet was discovered on October 8.5 UT with his 0,25m f/3.8 reflector. He estimated as a diffuse object of 11.5 mag with weak condensation.
Copyright Marcus Richert, Uwe Wohlrab
Alan Hale - Thomas Bopp - C/1995 O1
Independent reports of the visual discoveries of a new comet have been received from Alan Hale and Thomas Bopp (IAUC 6187). All observers note the comet (estimated around 10/11 mag) to be diffuse with some condensation and no tail, motion toward the west- northwest. Alan Hale (Cloudcroft, USA) found the comet with his 0.41-m reflector while Thomas Bopp (near Stanfield, USA) discovered the comet with a 0.44-m f/4.5 Dobsonian during a star party while observing M70. The comet turned to be one of the brightest of the century and was visible for a very long time between 1995-1998. The comet reached perihelion on 1997 April 1st. and studies revealed a nuclear of 60km!
Copyright Kevin Gill
William A. Bradfield - C/1995 Q1
William A. Bradfield of Dernancourt (Australia) discovered his seventeenth comet, a 6 mag. object with a tail over 1° long, on August 17.4 IAUC 6206. The comet was in Crater, two weeks from perihelion, and was well placed for some time prior to discovery.
Yuji Hyakutake - C/1995 Y1
IAUC 6279 announced the discovery of a new comet by Yuji Hyakutake (Hayato, Aira-gun, Kagoshima-ken) on December 25, with a 25x150 binoculars. The comet appeared diffuse with coma diameter of 3'.5 and total mag of 10th. The comet was observed in twilight while further confirmations arrived by T. Kojima and Y. Kushida.
Information about discovery story were written by D.H Levy on Sky and Telescope, May 1998:
“…E. Szczepanski is a Lawyer, specializing in maritime law. He also a complished astrophotographer and telescope maker. One day in January 1996 he was perusing old astronomy magazines during his lunch break when an article I wrote on comet hunting caught his attention. As he red he wondered what it would be like to discoverer a comet. That evening Szczepanski drove out to the Houston Astronomical Societys observory site near Columbus for a solitary astrophotography session. He set up is 4-inch Takahashi refractor and, with Kodak Technical Pan 2415 film, began imaging deep-sky object. M101, the huge spiral galaxy north of Bug Dipper’s handle, was the last one on his list. When he developed his film the following day, he was surprised to see the trailed image of a 10th magnitude fuzzy object ½° south of M101. He immediately reported it to the IAU's Central Bureau for Astronomical Telegrams…”
Yuji Hyakutake - C/1996 B2
Only one month later Y.Hyakutake discovered another and most popular C/1996 B2. The comet was announced on IAUC 6299. The comet was discovered on 30.8 January 1996 with his 25x150 Binoculars. The comet appeared diffuse and of 2.5’ diameter and 11th mag. In the next months the comet became a “great comet” approaching Earth on March 25th with a total magnitude of 0th and a tail of 80°!!
Copyright: Michael Jager, Erich Kolmhofer, Herbert Raab. 25-03-1996
Howard J. Brewington - C/1996 N1
IAUC 6428 announced a new comet discovered, by amateur Howard J. Brewington from Cloudcroft(USA). The comet was discovered on July 4th visually with a 20cm reflector and was later confirmed by G.Garradd.
Copyright David Hanon
Vello Tabur - C/1996 Q1
IAUC 6455 announced the discovery of a new comet,C/1996Q1, on August 19 by Vello Tabur (Wanniassa,AUS). The comet was discovered with 20cm reflector and appeared of 11th magnitude and 3’ diameter.
Copyright Stefan Beck
Justin Tilbrook from Clare, South
Australia, reported a visual discovery of a comet on July 22.43UT with a
20cm reflector. Justin is a variable star observer and he discovered the
comet while was observing TV Corvi when he saw a 10th mag “blob” of 70” in diameter. Several
minutes later he saw that the object had moved. One day later Gordon
Garradd (from Loomberah) confirmed the comet using a 25cm reflector+
CCD, the images showed a little fuzzy of 2’ without tail. IAU Circular
6705 announced the discovery on July 23 while a preliminary orbit
announced in IAUC 6707 showed the comet was close to perihelion at about
1.4AU from the Sun and a similar distance from the Earth. If the comet
had been 3 months earlier, it would have been visible in 7x50 binoculars
from the Earth. Copyright
Picture of C/1997O1 taken by Justin, using a 35mm camera with a 200mm zoom lens and 400ASA Fujicolor print film; on the evening of 1997 July 26 (10:45 UT). The camera was hand-guided for an exposure lasting 10 minutes, to capture this faint image of Comet Tilbrook.
Comet Tilbrook image taken by Akimasa Nakamura on 1997 July 24.47UT with a 60cm Reflector f6.
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 McNaught 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!
IAUC 7222 announced the visual discovery of a new comet C/1999 N2 on July 13th. by Daniel W. Lynn, Kinglake West, Victoria, Australia with 10x50 binoculars and 0.20-m f/6 reflector (40x, 150x). Comet low in sky, moving northeastward at about 10'/hr. Coma diameter 4'.2, fairly strong central brightening, but no discernible nuclear condensation and no tail.
Korado Korlevic - P/1999 WJ7
IAUC 7368 announced the discovery of a new comet P/1999 WJ7. An apparently asteroidal object discovered on Nov. 28th by Korado Korlevic at Visnjan with a 0.41-m f/4.3 reflector + CCD turned out to be a comet. It was discovered while doing routine asteroid search.