Monthly Information about Comets in December 1996

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Updated on December 10, 1996
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  • Comets Ranking
  • Explanations
  • Faint Comets
  • Ephemeris Table
  • Finding Charts (PostScript)
  • ---------------------------------------------------------------------

    * Comets Ranking

    Here is the ranking of comets in December, 1996.

    Comet C/1995 O1 (Hale-Bopp), the probable greatest comet in this century, had seemed to go faint a bit in September and surprised us. But it began to brighten again after that and reached 4.5 mag now. It comes to conjunction with Sun through this and next month, then it will appears at dawn in mid January and the highlight comes.

    Comet C/1996 Q1 ( Tabur ) had been brightening rapidly and reached 5 mag in late September. But, to be very surprised, it turned to go faint in October. It stopped brightening just after October came and had been stable with 5-6 mag until mid October, and it has suddenly faded away on 20th and reached to 9 mag in a few days. Now it is 10 mag or fainter, extremely diffused.

    Though 96P/Machholz 1 and 85P/Boethin have not been observed yet at this return, they have already closed to Sun and set under the horizon. We have another chance to observe 85P/Boethin in next autumn, but it is almost impossible to see 96P/Machholz 1 this time.

    * No. 1 C/1995 O1 ( Hale-Bopp ) 4.5 -> 3.5 mag

    - No. 2 C/1996 J1 ( Evans-Drinkwater ) 9.5 mag

    * No. 3 C/1996 Q1 ( Tabur ) 11 -> 13 mag

    * No. 4 81P/Wild 2 13 -> 12 mag

    - No. 5 116P/Wild 4 12.5 -> 13 mag

    * No. 6 126P/IRAS 13 -> 14 mag

    * No. 7 118P/Shoemaker-Levy 4 13.5 -> 13 mag

    * No. 8 22P/Kopff 14 -> 15 mag

    ! No. 9 85P/Boethin 15 -> 14 mag

    * No. 10 29P/Schwassmann-Wachmann 1 14 mag

    - No. 11 65P/Gunn 14.5 mag

    * No. 12 C/1996 P2 ( Russell-Watson ) 15 -> 15.5 mag

    * No. 13 46P/Wirtanen 16 -> 15 mag

    - No. 14 124P/Mrkos 15 -> 15.5 mag

    * No. 15 C/1996 R1 ( Hergenrother-Spahr ) 15 -> 16.5 mag

    * No. 16 121P/Shoemaker-Holt 2 15.5 mag

    Other faint comets are as follows.

    - C/1996 B2 ( Hyakutake ) 15.5 -> 16.5 mag
    * 95P/Chiron 16 -> 15.5 mag
    * 57P/du Toit-Neujmin-Delporte 16 -> 16.5 mag
    + D/1978 C2 ( Tritton ) 16 -> 16.5 mag
    ! 96P/Machholz 1 16 -> 18.5 mag
    * 119P/Parker-Hartley 16.5 mag
    * 32P/Comas Sola 16.5 -> 17 mag
    * 107P/Wilson-Harrington 17 mag
    * C/1996 N1 ( Brewington ) 17 -> 18.5 mag
    * 94P/Russell 4 17.5 -> 17 mag
    * P/1996 R2 ( Lagerkvist ) 17 -> 17.5 mag
    * 2P/Encke 17.5 -> 17 mag
    + 100P/Hartley 1 18 -> 17 mag
    * C/1996 E1 ( NEAT )17.5 -> 19 mag
    * 43P/Wolf-Harrington 18 -> 17.5 mag
    * C/1994 J2 ( Takamizawa )18 mag
    * P/1996 A1 ( Jedicke )18 mag
    * 67P/Churyumov-Gerasimenko 18 -> 18.5 mag
    * 1996 PW 18.5 -> 19 mag
    * (5145) Pholus 19 -> 18.5 mag
    * 74P/Smirnova-Chernykh 18.5 -> 19 mag
    * 129P/Shoemaker-Levy 3 18.5 -> 19 mag
    * P/1996 N2 ( Elst-Pizarro ) 19 -> 19.5 mag
    * 111P/Helin-Roman-Crockett 20 mag
    * 120P/Mueller 1 20.5 mag
    * 127P/Holt-Olmstead 21 mag

    *Observable now -Not observable in the Northern Hemisphere +Periodic comets not yet observed at this return !Periodic comets not yet observed at this return but not observable in the Northern Hemisphere

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    * Explanations

    * C/1995 O1 ( Hale-Bopp )

    Comet Hale-Bopp, the probable greatest comet in this century, has stopped its favorable brightening until July in August, then it seemed to go faint a bit as 6 mag and made us impatient in September. But it began to brighten again after that. It reached about 4.5 mag in late November and early December.

    The magnitude has brightened from the discovery in 1995 summer to last July so well along the equation:

    m1 = -2.0 + 5 log d + 10.0 log r
    The change of magnitude after September has been along the equation:

    m1 = -0.4 + 5 log d + 8.0 log r
    As you see, the coefficient of log r is 8.0 which shows that the current brightening is a bit flatter. Here I depend on this equation. It shows that the comet will be 0 mag in next March and April. This is about 2 mag fainter than expected from the previous equation.

    Now the comet is 4.5 mag in the west at dusk. The altitude is so low and hard to see it. It moves northwards through Serpens (tail) and getting lower and lower. The magnitude is about 4 mag, so probably observable until just after mid December. It becomes lower than 10 deg one hour after sunset after Dec. 20.

    The comet will appear again at dawn in January. It becomes higher than 10 deg one hour before sunrise on Jan. 10. The magnitude will be about 3 mag then. It moves in Aquila in January. It is easy to find it because it locates just upper of Altair from mid to late January.

    After appearing again at dawn, it will go brighter rapidly. Then the highlight of this super comet comes. It reappears as 3 mag in mid January and comes to be bright as 2 mag in late January. In February it moves through Aquila and Cygnus and brightens from 2 to 1 mag. The altitude at one hour before sunrise keeps 25 deg. In March it enters in Pegasus and begins to be lower. But the magnitude keeps brightening and reaches the highlight as 0 mag in late March when it is seen low in the northeast.

    March 9 is the day of a solar eclipse in Mongolia and Siberia and the comet is seen overhead just in the eclipse. It is expected to be bright as 0.5 mag then even from the current flat equation, so bright enough to see it during the eclipse. The "eclipse comet" is after an interval of 115 years. Let's look forward to a fine view.

    The comet begins to be seen also at dusk after mid March. The condition at dusk becomes better again after late March. The comet passes the perihelion on April 1 and then it is seen 25 deg high in the northwest about one hour after sunset in mid April. The magnitude is still around 0 mag. In May the altitude begins to be low in the evening sky. At the same time, it begins to go faint rapidly. It will reach to 2 mag when being too low and too close to the sun in mid May.

    In autumn it appears just over the horizon in the southeast with magnitude 5-6 from September to October. But it leaves to the south in November and then will never seen again in the Northern Hemisphere.

    * C/1996 J1 ( Evans-Drinkwater )

    C/1996 J1 (Evans-Drinkwater) is a new comet discovered on May 16 with magnitude about 16. It had been observed until July with magnitude 13. Then it closes to the sun. It will pass the perihelion on Dec. 30 but is still not observable. The predicted magnitude is 9 mag.

    Because this comet moves forwards on an orbit with perihelion distance 1.3 AU, the condition changes extremely depending on the relation with the Earth. If it locates at a good position, it closes to the Earth around the perihelion date and brightens so much. Then it also keeps observable for a long period around it with a good condition. On the other hand, if it passes opposite side of the sun, we cannot see it for a long period because it keeps close to the sun.

    This comet comes with a worst relation. We cannot see it for a year around the perihelion date. The next chance to see this is June 1997 when it appears at dawn in Triangulum but the magnitude is 13. After this it goes away from the Sun and comes fainter on and on.

    If it has passed the perihelion in mid July, it would close to the Earth from June to August and reach to 5 mag, and be observable for a year around it.

    * C/1996 Q1 ( Tabur )

    Comet C/1996 Q1 ( Tabur ) is a new comet discovered on Aug. 19 by Mr. Tabur in Australia as 10 mag. It had been brightening more rapidly than expected in September and reached to 5 mag and became a naked-eye object in late September. The change of magnitude in this period is along the equation:

    m1 = 6.6 + 5 log d + 15.0 log r
    So it is expected to be bright as 4.5 mag in mid October when the comet closes to the Earth.

    But it suddenly stopped brightening just after October came and became stable with magnitude 5-6. It kept the same magnitude until mid October anyway and the tail, which extended northwards, was also observed. However, to be very surprised, it suddenly has fade away on Oct. 20 and reached to 9-10 mag in late October. The image has been so diffused. Because the altitude bacame so low at the same time, it came to too hard to see this comet in late October. Though the perihelion date was Nov. 3, it came to THE END before that.

    After that it closed to the Sun and only few observations was reported. They say the comet kept 9-10 mag in November but so diffused and hard to see it.

    The comet will moves southwards between Hercules and Serpens (head) in December and January. It is in the morning sky. In early December it is so low yet, but the altitude will be higher and higher. The predicted magnitude is 11-13 mag, but much harder to observe it because it is so diffused. Maybe it fades awar rapidly, as many other diffused comets have done it. Anyway the positional condition will be better after this, it is worth trying to observe it. The triangle at the head of Serpens will be a good base to find it in December and January.

    This comet moves on a quite same orbit as that of C/1988 A1 ( Liller ) which appeared in 1988 and reached 5-6 mag. Therefore these two comets separated from each other at the previous perihelion (about 3,000 years ago) and came back again with 8 year interval. The brightening in September and fading awar in October may be the same phenomena as that a child object of a separated comet sometimes becomes brighter than the parent nucleus temporarily.

    Because the discoverer of this comet lives in Australia despite having an Estonian name, the pronunciation of the name is not clear and many Japanese were confused. As a result, we can read it whichever in Aussie English style or Estonian style by the discoverer's comment.

    * 81P/Wild 2

    81P/Wild 2, which will pass the perihelion on May 6, 1997, has been brightening so rapidly. It was about 16.5 mag in September, 15 mag in October, 14 mag in November and then reached 13 mag in early December. Observations with eyes are also reported. The change of the magnitude is along the equation:

    m1 = 5.2 + 5 log d + 21.5 log r
    It shows that the comet may be observable with eyes as 10 mag for a long period from late January to early June in next year.

    It locates at the east of Cancer in December and January. It is at opposition in January and seen with a good condition, overhead at midnight. The magnitude may reach 11-12 mag in December, 10 mag in January.

    The comet will be observable in the evening sky from January to August in 1997.

    * 116P/Wild 4

    116P/Wild 4, which has been bright as 12 mag in this spring, moves from Libra to Scorpius in December and enters Ophiuchus in January. It is still at conjunction with the sun and not observable.

    The total light curve from the recovery in February 1995 (20.5 mag) to the observations in spring and summer as around 12 mag is alogn the equation:

    m1 = 1.4 + 5 log d + 27.0 log r
    We can see how rapidly it came bright.

    It appears again in the southeast low sky at dawn in late January. It keeps low from February through mid April, about 15-20 deg at the beginning of the day light, and hard to observe it. But after mid April the altitude goes higher slowly. Though it has already passed the perihelion on Aug. 31, it will still be bright as 13.5 mag in next February. Then it is observable until it reaches 17 mag in summer.

    * 126P/IRAS

    126P/IRAS is a periodic comet discovered in 1983 by a satellite and this is the first return. It had not been recovered for a while because it was not observable in the Northern Hemisphere, but finally recovered on Aug. 8. The magnitude is 13, same as expected. It began to be seen in the Northern Hemisphere after late September. Unfortunately the total magnitude has reached only 12 mag in October. It has already passed the perihelion on Oct. 29 and been getting faint. It was 13 mag in early December.

    The comet moves through Pegasus, from the head to the body, in December and January. It is now high in the evening sky. At the end of day light, it locates in the south sky in December and in the west sky in January. There are some bright star as 3 mag along the comet's path, so it is easy to find it. But the magnitude goes faint from 13 to 14 mag.

    It keeps moving northwards after this and observanle until April when it becomes low in the west with magnitude 17.

    * 118P/Shoemaker-Levy 4

    118PShoemaker-Levy 4, which is in its first return now, will pass the perihelion on Jan. 12. This return is best, just at opposition around the perihelion date.

    This comet has been expected to become as 14.5 mag, but actually it is coming much brighter than it. It was as 17 -> 16 mag from July to September, 15 mag in October, 14 -> 13 mag in November. Some reported it as 12 mag in early December with eyes.

    It is now the highlight of this comet, about 12 mag with eyes and 13 mag with CCDs. It moves at the head of Orion and easy to find where it is. If you have a large telescope, please try to see it with your eyes. Now is at the opposition and high in the south sky at midnight.

    This comet will be observable until setting in the west in June as 16-17 mag.

    * 22P/Kopff

    22P/Kopff has already passed the perihelion on July 2. The condition of this return is best, almost opposition around the perihelion day, and reached 8 mag. Though it keeps high altitude after that for a while, only a few observations were reported after mid September somehow. They show the comet has been coming faint as same as pre-perihelion brightening. It was observed as 13.5 mag in early December. The total light curve of this return is along the equation:

    m1 = 5.3 + 5 log d + 21.0 log r

    It moves across Aquarius from December to January. It moves gradually to the southwest sky at dusk. In late January the altitude at the end of day light becomes 25 deg. The magnitude will fade as 14 -> 15. Now it is about the end of the season of 22P/Kopff's this return. It sets in the west in early March.

    The comet passes about 2 deg south of Saturn on Feb. 10. There are such comets as 46P/Wirtanen and P/1996 R2 ( Lagerkvist ) nearby this comet at the same time.

    * 85P/Boethin

    Comet 85P/Boethin, which will pass the perihelion on Apr. 17, 1997, has finally set in the west not been observable already though it has not been observed in this return yet. The condition of this return is quite worst. It should be 9.5 mag around the perihelion but too close to the sun to see it. It will appear again at dawn next October 1997, but then it is as faint as 17 mag.

    The comet moves in Sagittarius in December and Capricornus in January. Though it has not been observable already, the predicted magnitude is 15 -> 14 in this month. But because it was not observed in last summer when it has been 18-19 mag at opposition, it may be much fainter.

    It passes about 3 deg south of Jupiter in early December. The altitude at the time is so low but maybe the last chance to observe it. Then comet 65P/Gunn is also 3 deg south of this comet.

    * 29P/Schwassmann-Wachmann 1

    22P/Schwassmann-Wachmann 1 has bursted out in February during the last season. It reached about 11 mag, then became faint and diffused and set in the west as 14 mag in June.

    It has already appeared again at dawn and the new season has already started. In November it was observed as 14.5 mag. It seems as smoldered as ever. It is now in the south of the head of Virgo and seen high in the morning. But there are few remarkable stars around and so hard to catch it in your camera field.

    It has closed to P/1996 A1 ( Jedicke ) on Nov. 5. The distance was only about 10'. They are now separating from each other but the distance is still about 1 deg in early December.

    * 65P/Gunn

    65P/Gunn has already passed the perihelion on July 24. The condition of this return is good and it had been observed as 12 mag from May to July. It has been going gradually faint after this and observed as 13.5 mag in September. But no observations succeeded after that.

    It is in the west of Sagittarius now and near to Jupiter and 85P/Boethin. It is already too low in the west to observe. This season of this comet has finished. But the eccentricity is like a circle and it becomes observable again in Cetus at dawn in June 1997 with magnitude 15.

    * C/1996 P2 ( Russell-Watson )

    A new comet C/1996 P2 (Russell-Watson) was discovered on August 10 as 13 mag in the southern constellation Sculptor. It has already passed the perihelion on Mar. 1 and the perihelion distance is as far as 2.0 AU, so it is going fainter slowly.

    Probably because it was in the southern sky and observable only for a moment in the Northern Hemisphere, only few observations are reported despite the brightness. Though it was at opposition in October and November, only few are reported, either. The comet was about 12-13 mag in August and September, 13.5 mag in October and reached 15 mag in early December.

    It moves northwards in Sculptor in December and January. It enters in Cetus in late January. It is seen low in the south sky at dusk with magnitude around 15. This comet is observable until it becomes low in the west late in next February. The it is about 16.5 mag.

    It closes less than 2 deg to a globular nebula NGC288 (8.1 mag, 14') on Dec. 20.

    * 46P/Wirtanen

    Comet 46P/Wirtanen, which will pass the perihelion on Mar. 14, has been observed as 19 mag from July and October, which is much fainter than expected. But it seemed to begin brightening recently. It was 15.5 mag in December. However this comet will be bright as only 12-13 mag in next spring if the the brightening keeps the current pace. Yet this comet tends to brighten so rapidly around perihelion date, please watch out the magnitude.

    It is in the south of Capricornus in December and moves to Aquarius in January. It is seen in the southwest sky at dusk. It will keep same altitude, 25 deg high, at dusk from now through early next July.

    It closes 1 deg to NGC7293 (7.0 mag, 13') on Dec. 24 and 25. It passes about 3 deg south of Saturn in early February, then 22P/Kopff and P/1996 R2 ( Lagerkvist ) are also in the neighborhood.

    * 124P/Mrkos

    124P/Mrkos is returning for the first time. It has been already recovered in October 1995 as 19.5 mag, but no observations are reported since it because it has been too close to the Sun during 1996. It is still too low in the southeast sky at dawn this month and impossible to observe it. The condition of this return is so bad and no one tell anything on it. But the perihelion date is Nov. 9 and it is brightest now as 15 mag.

    The comet moves Virgo -> Hydra -> Lupus in December, Lupus -> Scorpius in January. Because it comes far away from the Sun moving southwards, it is seen just on the horizon at dawn and impossible to observe it in the Northern Hemisphere. On the other hand, in the Southern Hemisphere it becomes high enough to observe in late December and the altitude comes higher after January.

    * C/1996 R1 ( Hergenrother-Spahr )

    A new comet discovered on Sept. 7 as 14 mag. The perihelion date is Aug. 28, so it was discovered under the best condition, around opposition just on perihelion day. It was seen overhead at midnight in September in the Northern Hemisphere and the magnitude was around 11.5-12.5. But it moved southwards rapidly and became to be seen only in the evening sky. So only few observations were reported after mid October. It seemed to fade awar more rapidly, 14 mag in early November and 16 mag in early December.

    It moves southwards in the east of Capricornus in December. It has already been low in the evening sky and hard to observe it. The magnitude is faint as 15-16 mag. After mid December it becomes too low to observe. After conjunction, it appears again at dawn in the Southern Hemisphere in late March. But the comet keeps moving southwards and will be never observable in the Northern Hemisphere again.

    * 121P/Shoemaker-Holt 2

    Comet 121P/Shoemaker-Holt 2 was discovered in 1989 and is now in its first return. If the comet had kept the brightness at the discovery, it would have been observed as 12-13 mag for a while. But actually, it was recovered in November 1995 as 18 mag, which was 5 mag fainter than expected. Then it has been as 19 mag and becomes at conjunction with the sun around the perihelion on Aug. 20. However, after it began to appear again at dawn in October, it was observed as 16 mag, which was 2-3 mag brighter than before-perihelion. In 1989 it was discovered after perihelion, too. So maybe this is a comet which becomes brighter after perihelion.

    It is on the back of Leo in December and January and almost overhead in the morning sky. Though it has passed the perihelion already, it becomes closer to the Earth and keeps 15-16 mag until it becomes at opposition in next spring.

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    * Faint Comets

    C/1996 B2 (Hyakutake), which became one of the greatest comets as 0 mag with 100 deg long tail in March and April, is now not seen in the Northern Hemisphere. It has been observed in the Southern Hemisphere after the perihelion day on May 1, and reached 12 mag in early September. But no observations has been reported after that and recent status is so unclear. The predicted magnitude is about 16. It is is Corona Austrina in December and January. Though it was low both at dusk and at dawn even in the Southern Hemisphere in October and November, the altitude at dawn becomes higher after this. But maybe no more observations are reported.

    95P/Chiron, whose period is about 50 years and which is also registered as an asteroid (2060), begins to appear at dawn again. It passed the perihelion in February and was observed as 15 mag in the last season. But the perihelion distance is so large and the magnitude changes slightly. It will be 15 mas again when it is at opposition in next spring. We can trace it for a few years at least. It is just in the south of Spica now.

    57P/du Toit-Neujmin-Delporte, which was expected to be as 18-19 mag from pre-perihelion observations, has bursted out and been as bright as 12-13 mag in late July. Then it has been stable with magnitude about 15 after September. I wonder Until when this stable situation continues. It moves from the root of Pisces to Aries in December and January and is seen high in the south sky at dusk.

    A lost periodic comet D/1978 C2 (Tritton), which had not recovered in 1984 and 1990, is expected to be brightest now. It is around the forefoot of Leo and high in the south sky at dawn. This comet seems to go both bright and faint rapidly, so the chance to recover it is for a moment. Though it will be at opposition in February, the magnitude will be 18 then. The predicted position is good just on the ecliptic. Will the comet happen to be recovered.

    A famous periodic comet for its quite small q (0.12 AU), 96P/Machholz 1, is too close to the sun and impossible to see it this month. The condition of this return is worst to see the comet in the Northern Hemishpere and can never observe it. It has been slightly observable in August and September in the Southern Hemisphere. But no observations succeeded. It will keep close to the sun after this and the comet goes faint rapidly. In the Northern Hemisphere it comes to be observable late in next March but the magnitude will be fainter than 20 mag then. Probably no one can see this comet in this return after all.

    119P/Parker-Hartley is in its first return now. It had been already observed in last autumn and winter as 16-17 mag. It passed the perihelion on June 24 and was too close to observe it then. Now the comet appears at dawn again. It is in Gemini as 16.5 mag. It is at opposition in January and seen overhead at midnight. Then it faints to 18.5 mag at set in the west in May.

    32P/Comas Sola has been much brighter than expected, about 14.5 mag, in early 1996. Then it becomes at conjunction with the sun around the perihelion on Jun. 10. But it has appeared again at dawn last month. It is in Virgo and seen high in the morning sky. The brightness is still about 16 mag. There are 95P/Chiron and 67P/Churyumov-Gerasimenko in the neiborhood.

    Comet 107P/Wilson-Harrington, which is also registered as an asteroid (4015), passes the perihelion on this Dec. 6. It was observed as 19 mag in May but no following observations was reported. It moves Capricornus -> Aquarius -> Pisces from December to January. It is in the southwest sky at dusk as ever, but the altitude at the end of day light becomes highter, 25 -> 35 deg in December, 35 -> 45 deg in January. It is close to 22P/Kopff, 2P/Encke and P/1996 R2 ( Lagerkvist ) in early January. It passes 5 deg north of Saturn. Because the perihelion distance is 1.00 AU, it can close to the Earth so much and be bright if the comet passes the perihelion in late September. But the condition of this return is bad and reaches 17 mag at most.

    Comet C/1996 N1 (Brewington), which was discovered on July 4, brightened as 8 mag in August and faded slowly 8.5 -> 10 mag in September. But in mid October it fade away rapidly from 11 mag to 14 mag. Then the comet seemed to be diffused and no following observations succeeded despite the good location. It moves from Pegasus to Andromeda in December and January. It is seen at a good position, almost overhead at dusk, but the predicted magnitude is so faint as 17 -> 19. Because the comet is extremely diffused, it is much harder to observe it.

    94P/Russell 4, which will passes the perihelion on Feb. 3, has been observed as 19 mag in November, a bit fainter than expected. It is in Leo in December and Virgo in January as 17-18 mag in the south sky at dawn. It enteres among the galaxies in Virgo. Though this is a small faint comet, the condition is good and reaches 16 mag almost at opposition in next March. Then it is observable until the end of summer when it becomes low in the west as 19 mag.

    A new periodic comet P/1996 R2 ( Lagerkvist ), which was discovered on Sept. 10 as 17 mag, passes the perihelion on Jan. 20. It has been observed as 16.5 mag recently, which is about 1 mag brighter than at discovery. It moves from Aquarius to Pisces in December and January and seen in the south sky at dusk. It gathers with 22P/Kopff and 46P/Wirtanen near Saturn in early February. Then it becomes too low to observe it. After conjunction with the sun, it becomes to be observable again as 18-19 mag in next summer.

    A famous periodic comet 2P/Encke will begin to brighten gradually for the perihelion on May 23. It has been already observed as 19-20 mag from July to October. It is in Aquarius to Pisces as 17 mag in December and January. The condition of this return is worst for observers in the Northern Hemisphere. It will be observable until mid February before perihelion , when it is 16 mag, and after perihelion, it reappears in August in Scorpius in the evening southern sky, when the comet is already 12.5 mag. Then it is observable until late November as 19 mag. On the other hand, the condition in the Southern Hemisphere is good. Because the comet closes to the Earth as 0.19 AU on July 5, it becomes much bright in June and July. The comet appears as 7 mag in late June and goes faint 7 -> 10 mag in the high altitude at dusk in July.

    100P/Hartley 1, which will pass the perihelion on May 28, has been observable at dawn since mid September and has to be coming brightening now. But no one could observe it yet at this return. It moves from Coma Berenices to Arcturus in December and January. There are many galaxies along the path. It is seen almost overhead in the morning sky and brightens 18 -> 17 mag this month, so it will be observed at first soon. This time the condition is good, almost opposition around the perihelion date, and the magnitude will reach 14 mag in next spring. Then it is observable until it becomes 16 mag in summer.

    Comet C/1996 E1 ( NEAT ) has been not so clear on its magnitude since the discovery. Anyway on the average, it reached as 11-12 in summer and faded as 13-14 mag in October. After that the comet became so diffused and very hard to observe it. It goes faint as 17 -> 19 mag in Aquarius in the southwest sky at dusk. But it is much harder to observe it than the magnitude shows. In addition the altitude becomes lower rapidly and too low in January. It closes about 1 deg to 43P/Wolf-Harrington on Dec. 6.

    43P/Wolf-Harrington, which will pass the perihelion on Sept. 29, 1997, is coming brighter slowly now. It is in Aquarius in December and January and seen in the southwest sky at dusk as 18 mag. The altitude is coming lower and lower, and it becomes too low to observe it in late January. After conjunction with the sun, it appears again at dawn as 13.5 mag in early next summer. Then it reaches 12 mag in autumn and observable with the same brightness for a while. It closes about 1 deg to C/1996 E1 ( NEAT ) on Dec. 6. It passes about 2 deg north of a globular nebula M2(6.5 mag, 13') on Jan. 10.

    C/1994 J2 ( Takamizawa ), which was discovered in May 1994 and was observed as 9-10 mag in May and June, has been observed for a long time and even now. It was about as bright as 15 mag in autumn in 1995, 16.5 mag in early 1996. Now it is observed as 18 mag. The comet is in the bottom of Orion, almost at opposition and seen in the south sky at midnight. It will be observed as 18-19 mag until next spring. It closes about 10' to Kappa-Ori(2.1 mag) on Dec. 21. In January it moves towards Rigel.

    A new periodic comet P/1996 A1 ( Jedicke ) discovered in January 1996 as 17 mag has been observed as 16-17 mag until last June. Then it was at conjunction with the sun and it appears again at dawn now. For the recovery in next return, more observations can be a big help. In December and January it is in the south of the head of Virgo and very close to 29P/Schwassmann-Wachmann 1. They closed about 10' each other on Nov. 5 and the distance is still about 1 deg in early December.

    67P/Churyumov-Gerasimenko, which passed the perihelion in January 1996 and reached 11 mag then, has been not observable at conjunction with the sun after it faded as 14.5 mag in June. Now it appears again at dawn, just north of Spica. The predicted magnitude is about 18, but not so clear. The altitude will become higher and higher after this. There are 32P/Comas Sola and 95P/Chiron in the neiborhood now.

    A new asteroid 1996 PW was discovered on Aug. 9 as 18 mag. But the true character is a quite rare object. The orbital elements show that it moves on an orbit with 2.5AU perihelion distance and 3000 year period. That is a typical one of a long periodic comet. But the following observations say that it is quite stella as 17 mag and no sign as a comet has been detected. It has already passed the perihelion on Aug. 8 and it faints 18.5 -> 19 mag this month. It is near Fomalhaut in early December and moves to Beta-Cetus (2.0 mag) and closes it in early February. It is seen in the south or southwest sky at dusk. It will be observable until early February and it will reach 21 mag when it appears again after conjucntion. Then this object goes far away from our solor system and will never be observed again. It was remarkable in comparison with the asteroid-like comet P/1996 N2 (Elst-Pizarro) which was also discovered in this summer.

    A new asteroid (5145) Pholus, which was discovered on Jan. 9, 1992 as 17 mag, was quite a rare object. The orbital elements show that it moves on an orbit with 8.7AU perihelion distance and 90 year period. Because that is very similar to that of 95P/Chiron, which had been regarded as an asteroid for a long time and the true character is a comet, maybe this object is also a comet. But no coma was detected by the following observations. Though 5 years have already passed since the perihelion date, it can be observed as 18 mag because of the large perihelion distance. No observations are reported after April 1994, but there are some images on films taken in 1997, 14 years before the perihelion, so the object will be observed for a few years after this. It is in Coma Berenices and high in the morning sky this month. The motion is so slight.

    74P/Smirnova-Chernykh is now just after the ahelion and in its faintest period as 18 mag. It will brighten slowly until next perihelion in 2001. It is in Aquarius and seen low in the south or southwest sky at dusk now. It set in the west in late January.

    129P/Shoemaker-Levy 3 was recovered in October with a predicted magnitude, 19 mag. The perihelion date is Mar. 4, 1998, more than one year ahead, but the orbit is like a circle, the eccentricity is 0.25, and it has already been a CCD target. It is in Pisces in December and January and seen high in the evening sky. It passes about 40' south of a galaxy M74(9.1 mag, 10') on Feb. 2. This comet is a small one and reaches only 17 mag around the perihelion.

    A new periodic comet P/1996 N2 ( Elst-Pizarro ), discovered on July 14 as 18 mag, is a remarkable object. The orbital elements show that it moves on a typical asteroid orbit. It has already faded away so much and the current image shows only the tail with no nucleus. Maybe the comet has bursted a bit temporarily and the tail extended and then discovered. It is in Aquarius now and seen in the southwest sky at dusk. It will set in the west in February. It was remarkable in comparison with the comet-like asteroid 1996 PW which was also discovered in this summer.

    111P/Helin-Roman-Crockett has just passed the perihelion on Oct. 31. But the eccentricity is 0.14, like a circle, so the magnitude will change slightly. It has been observed as 21 mag since 1995, which is so faint. It is in the south of Pollux in Gemini now. It is at opposition in January and locates overhead at midnight.

    120P/Mueller 1 is now at opposition. The condition of this return is worst, at conjunction around the perihelion in last April. So it brightens at most at opposition both half a year before and after the perihelion. So now it is brightest but the magnitude is extremely faint, fainter than 20 mag. It is in Auriga and almost overhead.

    127P/Holt-Olmstead is also just after opposition now. It has been brightest this autumn but the magnitude was so faint as 21 mag. The perihelion date is next February, but it goes fainter after this. It is in Aquarius and so low in the southwest sky at dusk.

    ---------------------------------------------------------------------

    * Ephemeris Table

    * C/1995 O1 ( Hale-Bopp )

    m1 = -0.4 + 5 log d + 8.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  17 56.47   -1 26.8   2.250   2.985    35    4.8
    1996-12- 3  18  6.22   -0 18.6   2.124   2.913    30    4.5
    1996-12-13  18 17.34    1  6.1   1.998   2.816    27    4.3
    1996-12-23  18 29.87    2 51.6   1.871   2.694    26    3.9
    1997- 1- 2  18 43.98    5  3.0   1.743   2.549    28    3.6
    1997- 1-12  18 60.00    7 47.0   1.617   2.383    30    3.2
    1997- 1-22  19 18.50   11 12.4   1.492   2.200    34    2.7
    1997- 2- 1  19 40.49   15 29.6   1.369   2.006    37    2.2
    

    * C/1996 J1 ( Evans-Drinkwater )

    m1 = 6.5 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  16 43.09  -26 27.2   1.413   2.361    12    9.9
    1996-12- 3  17 21.79  -25 25.6   1.361   2.319    10    9.7
    1996-12-13  18  1.24  -23 44.0   1.324   2.287     8    9.5
    1996-12-23  18 40.64  -21 22.5   1.302   2.268     8    9.4
    1997- 1- 2  19 19.27  -18 24.5   1.298   2.264     8    9.4
    1997- 1-12  19 56.59  -14 56.8   1.311   2.276     8    9.5
    1997- 1-22  20 32.21  -11  8.0   1.342   2.303     9    9.6
    1997- 2- 1  21  5.96   -7  7.3   1.387   2.346    10    9.8
    

    * C/1996 Q1 ( Tabur )

    m1 = 10.5 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  15 45.78   25 50.7   0.915   1.255    46   10.6
    1996-12- 3  15 55.78   21 34.7   1.001   1.417    44   11.3
    1996-12-13  16  3.43   18  6.9   1.107   1.545    45   11.9
    1996-12-23  16  9.38   15 18.2   1.226   1.638    48   12.5
    1997- 1- 2  16 13.74   13  1.7   1.352   1.700    52   13.0
    1997- 1-12  16 16.32   11 12.4   1.482   1.732    58   13.4
    1997- 1-22  16 16.77    9 45.9   1.614   1.739    66   13.8
    1997- 2- 1  16 14.63    8 38.1   1.747   1.725    74   14.1
    

    * 81P/Wild 2

    m1 = 5.2 + 5 log d + 21.5 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   8 13.05   17  3.2   2.213   1.556   119   13.6
    1996-12- 3   8 18.99   16 44.1   2.155   1.404   127   13.1
    1996-12-13   8 22.32   16 35.6   2.098   1.265   137   12.6
    1996-12-23   8 22.68   16 40.9   2.042   1.143   147   12.2
    1997- 1- 2   8 19.93   17  1.7   1.987   1.040   158   11.7
    1997- 1-12   8 14.26   17 38.0   1.934   0.958   169   11.3
    1997- 1-22   8  6.52   18 26.7   1.883   0.899   177   10.9
    1997- 2- 1   7 58.17   19 21.6   1.834   0.864   165   10.5
    

    * 116P/Wild 4

    m1 = 1.4 + 5 log d + 27.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  15 13.77  -19  4.1   2.091   3.057     9   12.5
    1996-12- 3  15 37.04  -20 38.3   2.116   3.056    14   12.6
    1996-12-13  16  0.29  -22  0.0   2.142   3.049    18   12.8
    1996-12-23  16 23.38  -23  8.7   2.171   3.035    23   12.9
    1997- 1- 2  16 46.18  -24  4.4   2.201   3.014    28   13.0
    1997- 1-12  17  8.54  -24 47.3   2.233   2.985    33   13.2
    1997- 1-22  17 30.30  -25 18.3   2.267   2.948    38   13.3
    1997- 2- 1  17 51.29  -25 38.2   2.301   2.903    44   13.5
    

    * 126P/IRAS

    m1 = 8.5 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  21 54.84   -2 54.5   1.723   1.432    88   12.8
    1996-12- 3  22  5.50    2  8.2   1.743   1.559    83   13.1
    1996-12-13  22 17.71    6 44.0   1.770   1.689    78   13.4
    1996-12-23  22 31.23   10 59.2   1.802   1.819    73   13.6
    1997- 1- 2  22 45.87   14 58.7   1.840   1.950    68   13.9
    1997- 1-12  23  1.53   18 46.2   1.883   2.078    64   14.2
    1997- 1-22  23 18.17   22 24.4   1.930   2.204    61   14.5
    1997- 2- 1  23 35.72   25 54.8   1.982   2.328    57   14.8
    

    * 118P/Shoemaker-Levy 4

    m1 = 6.7 + 5 log d + 21.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   5 42.81    8 13.7   2.059   1.137   151   13.6
    1996-12- 3   5 38.06    7 55.2   2.045   1.092   159   13.4
    1996-12-13   5 31.59    7 56.9   2.035   1.069   164   13.3
    1996-12-23   5 24.77    8 21.0   2.027   1.069   161   13.3
    1997- 1- 2   5 19.04    9  6.4   2.023   1.092   154   13.3
    1997- 1-12   5 15.58   10  9.5   2.021   1.136   144   13.4
    1997- 1-22   5 15.22   11 24.5   2.023   1.199   135   13.5
    1997- 2- 1   5 18.21   12 45.7   2.027   1.278   126   13.7
    

    * 22P/Kopff

    m1 = 5.3 + 5 log d + 21.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  22  6.59  -16 11.9   2.095   1.901    86   13.4
    1996-12- 3  22 24.15  -14 29.7   2.153   2.067    81   13.9
    1996-12-13  22 41.52  -12 43.6   2.211   2.235    75   14.3
    1996-12-23  22 58.69  -10 54.6   2.270   2.405    70   14.7
    1997- 1- 2  23 15.62   -9  4.0   2.330   2.575    64   15.1
    1997- 1-12  23 32.33   -7 12.8   2.390   2.742    59   15.4
    1997- 1-22  23 48.81   -5 21.8   2.449   2.906    53   15.8
    1997- 2- 1   0  5.07   -3 32.0   2.509   3.065    47   16.1
    

    * 85P/Boethin

    m1 = 6.5 + 5 log d + 20.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  19  3.94  -26 16.4   2.183   2.792    43   15.5
    1996-12- 3  19 23.42  -25 30.6   2.090   2.781    37   15.1
    1996-12-13  19 44.40  -24 32.3   1.997   2.757    32   14.7
    1996-12-23  20  6.78  -23 19.4   1.905   2.722    27   14.3
    1997- 1- 2  20 30.48  -21 49.8   1.813   2.676    23   13.8
    1997- 1-12  20 55.47  -20  1.4   1.722   2.622    18   13.3
    1997- 1-22  21 21.69  -17 52.4   1.633   2.561    15   12.8
    1997- 2- 1  21 49.12  -15 21.5   1.547   2.496    12   12.3
    

    * 29P/Schwassmann-Wachmann 1

    m1 = 4.0 + 5 log d + 7.5 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  11 59.12   -6 16.8   6.309   6.762    58   14.1
    1996-12- 3  12  3.32   -6 57.1   6.309   6.616    67   14.1
    1996-12-13  12  6.79   -7 33.9   6.309   6.461    76   14.1
    1996-12-23  12  9.43   -8  6.4   6.310   6.300    86   14.0
    1997- 1- 2  12 11.18   -8 33.8   6.310   6.137    95   13.9
    1997- 1-12  12 11.95   -8 55.6   6.310   5.977   105   13.9
    1997- 1-22  12 11.70   -9 11.0   6.311   5.824   115   13.8
    1997- 2- 1  12 10.45   -9 19.8   6.311   5.685   125   13.8
    

    * 65P/Gunn

    m1 = 7.7 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  19  4.30  -29  9.5   2.571   3.196    43   14.3
    1996-12- 3  19 24.62  -28 40.0   2.589   3.294    37   14.4
    1996-12-13  19 44.98  -28  1.0   2.608   3.384    32   14.5
    1996-12-23  20  5.22  -27 13.2   2.627   3.465    27   14.6
    1997- 1- 2  20 25.23  -26 17.2   2.648   3.537    21   14.7
    1997- 1-12  20 44.94  -25 13.9   2.670   3.598    16   14.7
    1997- 1-22  21  4.25  -24  4.3   2.693   3.649    11   14.8
    1997- 2- 1  21 23.12  -22 49.4   2.716   3.689     8   14.9
    

    * C/1996 P2 ( Russell-Watson )

    m1 = 6.5 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   0 55.34  -31 37.0   3.628   3.134   112   14.6
    1996-12- 3   0 55.52  -29 57.1   3.713   3.329   105   14.8
    1996-12-13   0 57.34  -28 11.4   3.799   3.533    98   15.0
    1996-12-23   1  0.64  -26 22.8   3.885   3.743    90   15.3
    1997- 1- 2   1  5.20  -24 33.7   3.971   3.956    83   15.5
    1997- 1-12   1 10.82  -22 45.7   4.057   4.170    76   15.7
    1997- 1-22   1 17.32  -21  0.2   4.142   4.381    69   15.9
    1997- 2- 1   1 24.54  -19 18.2   4.228   4.587    62   16.1
    

    * 46P/Wirtanen

    m1 = 11.5 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  21 28.30  -27 28.6   1.739   1.710    74   16.3
    1996-12- 3  21 44.30  -25 29.7   1.654   1.727    69   16.0
    1996-12-13  22  2.66  -23 13.0   1.570   1.734    63   15.6
    1996-12-23  22 23.13  -20 37.0   1.487   1.731    59   15.3
    1997- 1- 2  22 45.54  -17 39.6   1.407   1.719    54   14.9
    1997- 1-12  23  9.82  -14 19.1   1.331   1.698    51   14.5
    1997- 1-22  23 35.94  -10 34.4   1.260   1.671    48   14.1
    1997- 2- 1   0  3.94   -6 25.6   1.196   1.638    46   13.7
    

    * 124P/Mrkos

    m1 = 12.0 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  13 50.82  -15 14.7   1.421   2.186    30   15.2
    1996-12- 3  14 17.45  -20 12.6   1.436   2.161    32   15.2
    1996-12-13  14 45.13  -24 58.3   1.459   2.139    35   15.3
    1996-12-23  15 14.01  -29 27.2   1.489   2.121    38   15.4
    1997- 1- 2  15 44.17  -33 35.4   1.525   2.105    42   15.4
    1997- 1-12  16 15.61  -37 19.2   1.567   2.091    45   15.6
    1997- 1-22  16 48.16  -40 36.1   1.613   2.079    48   15.7
    1997- 2- 1  17 21.53  -43 24.4   1.664   2.068    52   15.8
    

    * C/1996 R1 ( Hergenrother-Spahr )

    m1 = 6.2 + 5 log d + 20.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  20 28.77  -19 43.7   2.177   2.427    63   14.9
    1996-12- 3  20 30.46  -21 29.3   2.238   2.679    53   15.3
    1996-12-13  20 33.77  -22 51.7   2.303   2.909    43   15.8
    1996-12-23  20 38.21  -23 58.4   2.372   3.114    34   16.2
    1997- 1- 2  20 43.42  -24 54.8   2.444   3.292    25   16.5
    1997- 1-12  20 49.13  -25 44.8   2.519   3.439    17   16.9
    1997- 1-22  20 55.10  -26 31.7   2.596   3.555    11   17.2
    1997- 2- 1  21  1.13  -27 18.1   2.675   3.639    10   17.6
    

    * 121P/Shoemaker-Holt 2

    m1 = 7.0 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  10 25.23   20 11.1   2.726   2.535    90   15.6
    1996-12- 3  10 35.37   20 35.0   2.739   2.418    98   15.5
    1996-12-13  10 43.72   21 14.3   2.754   2.306   106   15.4
    1996-12-23  10 50.03   22 10.3   2.770   2.202   115   15.4
    1997- 1- 2  10 54.06   23 22.9   2.786   2.109   124   15.3
    1997- 1-12  10 55.59   24 50.3   2.804   2.031   133   15.3
    1997- 1-22  10 54.55   26 28.1   2.823   1.972   143   15.2
    1997- 2- 1  10 51.11   28  9.3   2.843   1.935   151   15.2
    

    * C/1996 B2 ( Hyakutake )

    m1 = 2.0 + 5 log d + 18.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  16  3.54  -65  0.5   3.617   4.252    44   15.2
    1996-12- 3  16 21.75  -65 25.6   3.739   4.394    43   15.5
    1996-12-13  16 39.30  -65 57.1   3.860   4.517    43   15.8
    1996-12-23  16 56.10  -66 35.0   3.980   4.620    44   16.1
    1997- 1- 2  17 12.10  -67 19.1   4.097   4.704    46   16.4
    1997- 1-12  17 27.16  -68  9.9   4.213   4.770    50   16.6
    1997- 1-22  17 41.09  -69  7.5   4.328   4.819    54   16.9
    1997- 2- 1  17 53.65  -70 12.4   4.441   4.852    59   17.1
    

    * 95P/Chiron

    m1 = 4.0 + 5 log d + 7.5 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  13 35.43  -10 47.9   8.517   9.307    34   15.8
    1996-12- 3  13 40.23  -11 12.6   8.521   9.204    43   15.8
    1996-12-13  13 44.66  -11 34.9   8.526   9.084    52   15.8
    1996-12-23  13 48.62  -11 54.4   8.531   8.948    62   15.7
    1997- 1- 2  13 52.05  -12 10.6   8.536   8.799    71   15.7
    1997- 1-12  13 54.88  -12 23.3   8.541   8.642    80   15.7
    1997- 1-22  13 57.03  -12 32.2   8.546   8.481    90   15.6
    1997- 2- 1  13 58.47  -12 37.0   8.551   8.321   100   15.6
    

    * 57P/du Toit-Neujmin-Delporte

    m1 = 10.0 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   2  1.66    9 56.3   2.765   1.862   150   15.8
    1996-12- 3   1 57.77    9 34.7   2.818   1.995   139   16.0
    1996-12-13   1 56.27    9 27.7   2.871   2.148   129   16.2
    1996-12-23   1 57.11    9 34.4   2.923   2.316   119   16.5
    1997- 1- 2   2  0.04    9 53.1   2.975   2.496   109   16.7
    1997- 1-12   2  4.82   10 21.8   3.027   2.685   100   17.0
    1997- 1-22   2 11.19   10 58.3   3.078   2.877    92   17.2
    1997- 2- 1   2 18.89   11 40.7   3.128   3.071    84   17.4
    

    * D/1978 C2 ( Tritton )

    m1 = 13.0 + 5 log d + 20.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   9 52.02   16 36.6   1.451   0.957    96   16.1
    1996-12- 3  10 11.69   13 39.6   1.471   0.917   101   16.2
    1996-12-13  10 27.37   10 50.4   1.497   0.880   106   16.2
    1996-12-23  10 38.72    8 15.3   1.531   0.846   113   16.3
    1997- 1- 2  10 45.42    5 59.8   1.571   0.818   121   16.5
    1997- 1-12  10 47.26    4  9.1   1.616   0.796   130   16.7
    1997- 1-22  10 44.38    2 47.3   1.665   0.785   140   16.9
    1997- 2- 1  10 37.54    1 56.0   1.719   0.788   151   17.2
    

    * 96P/Machholz 1

    m1 = 13.0 + 5 log d + 12.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  16 48.19  -11  5.7   1.152   2.071    15   15.3
    1996-12- 3  17 13.10  -12 33.6   1.358   2.303    12   16.4
    1996-12-13  17 34.08  -13 35.3   1.551   2.511     9   17.3
    1996-12-23  17 52.23  -14 18.0   1.734   2.695     9   18.0
    1997- 1- 2  18  8.17  -14 46.5   1.908   2.853    12   18.6
    1997- 1-12  18 22.25  -15  4.4   2.075   2.985    18   19.2
    1997- 1-22  18 34.68  -15 14.3   2.235   3.090    24   19.6
    1997- 2- 1  18 45.54  -15 18.4   2.391   3.169    31   20.0
    

    * 119P/Parker-Hartley

    m1 = 2.0 + 5 log d + 25.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   7 24.76   18 21.8   3.147   2.412   130   16.4
    1996-12- 3   7 22.08   18  6.3   3.161   2.330   141   16.3
    1996-12-13   7 17.34   17 55.8   3.175   2.269   152   16.3
    1996-12-23   7 10.99   17 50.0   3.190   2.233   163   16.3
    1997- 1- 2   7  3.71   17 48.1   3.205   2.226   174   16.4
    1997- 1-12   6 56.31   17 49.3   3.222   2.248   170   16.5
    1997- 1-22   6 49.62   17 52.7   3.238   2.299   159   16.6
    1997- 2- 1   6 44.35   17 57.5   3.256   2.378   148   16.7
    

    * 32P/Comas Sola

    m1 = 5.5 + 5 log d + 22.5 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  13  3.83    3 37.4   2.385   2.922    48   16.3
    1996-12- 3  13 19.06    2 11.5   2.438   2.877    54   16.5
    1996-12-13  13 33.16    0 55.7   2.493   2.824    60   16.7
    1996-12-23  13 45.99   -0  9.0   2.548   2.762    67   16.8
    1997- 1- 2  13 57.41   -1  2.4   2.604   2.693    74   17.0
    1997- 1-12  14  7.24   -1 44.0   2.661   2.617    81   17.2
    1997- 1-22  14 15.26   -2 13.7   2.718   2.538    89   17.3
    1997- 2- 1  14 21.26   -2 31.5   2.775   2.458    98   17.4
    

    * 107P/Wilson-Harrington

    m1 = 16.5 + 5 log d + 5.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  19 42.69  -19  5.8   1.016   1.230    53   17.0
    1996-12- 3  20 26.92  -16 45.1   1.001   1.189    53   16.9
    1996-12-13  21 12.94  -13 36.6   1.004   1.157    55   16.8
    1996-12-23  21 59.92   -9 45.3   1.025   1.139    57   16.8
    1997- 1- 2  22 46.98   -5 23.2   1.063   1.141    59   16.9
    1997- 1-12  23 33.29   -0 47.5   1.114   1.166    61   17.1
    1997- 1-22   0 18.13    3 43.0   1.176   1.216    63   17.3
    1997- 2- 1   1  0.94    7 52.6   1.246   1.288    64   17.5
    

    * C/1996 N1 ( Brewington )

    m1 = 10.8 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  22 20.78   38 20.6   2.027   1.502   107   16.3
    1996-12- 3  22 48.41   34 30.1   2.153   1.686   104   16.9
    1996-12-13  23 12.15   31 23.7   2.278   1.893    99   17.5
    1996-12-23  23 33.15   28 58.7   2.401   2.117    94   18.1
    1997- 1- 2  23 52.17   27  9.2   2.524   2.354    88   18.7
    1997- 1-12   0  9.73   25 49.2   2.645   2.599    81   19.2
    1997- 1-22   0 26.20   24 53.2   2.765   2.848    75   19.7
    1997- 2- 1   0 41.80   24 16.1   2.884   3.098    68   20.2
    

    * 94P/Russell 4

    m1 = 10.5 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  11 11.69   11 23.6   2.285   2.301    76   17.7
    1996-12- 3  11 27.22   10 13.4   2.271   2.174    82   17.5
    1996-12-13  11 41.69    9 10.8   2.259   2.047    89   17.4
    1996-12-23  11 54.86    8 17.9   2.249   1.923    95   17.2
    1997- 1- 2  12  6.48    7 36.8   2.241   1.803   103   17.0
    1997- 1-12  12 16.22    7  9.7   2.235   1.688   110   16.9
    1997- 1-22  12 23.73    6 57.9   2.231   1.581   119   16.7
    1997- 2- 1  12 28.70    7  2.2   2.229   1.485   127   16.6
    

    * P/1996 R2 ( Lagerkvist )

    m1 = 9.0 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  22 38.53  -10 39.7   2.627   2.330    96   17.1
    1996-12- 3  22 47.63   -9 32.3   2.620   2.452    88   17.2
    1996-12-13  22 58.20   -8 15.8   2.614   2.575    81   17.3
    1996-12-23  23 10.01   -6 51.3   2.609   2.696    74   17.4
    1997- 1- 2  23 22.85   -5 19.9   2.606   2.815    67   17.5
    1997- 1-12  23 36.54   -3 42.7   2.604   2.930    61   17.6
    1997- 1-22  23 50.94   -2  0.8   2.603   3.039    55   17.6
    1997- 2- 1   0  5.93   -0 15.3   2.604   3.141    49   17.7
    

    * 2P/Encke

    m1 = 11.0 + 5 log d + 12.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  22 51.61    0 52.2   2.604   2.191   103   17.7
    1996-12- 3  22 51.25    0 33.5   2.520   2.265    93   17.6
    1996-12-13  22 53.50    0 31.7   2.433   2.337    83   17.5
    1996-12-23  22 58.10    0 46.1   2.343   2.402    74   17.3
    1997- 1- 2  23  4.79    1 15.6   2.248   2.456    66   17.2
    1997- 1-12  23 13.35    1 59.2   2.149   2.495    58   17.0
    1997- 1-22  23 23.63    2 56.3   2.046   2.516    51   16.7
    1997- 2- 1  23 35.51    4  6.0   1.938   2.519    44   16.5
    

    * 100P/Hartley 1

    m1 = 9.0 + 5 log d + 20.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  12  4.82   25 33.8   2.360   2.462    72   18.4
    1996-12- 3  12 22.34   24 26.2   2.314   2.315    77   18.1
    1996-12-13  12 39.21   23 24.3   2.269   2.168    82   17.8
    1996-12-23  12 55.24   22 29.4   2.225   2.023    88   17.5
    1997- 1- 2  13 10.24   21 42.5   2.182   1.879    94   17.1
    1997- 1-12  13 23.92   21  4.5   2.141   1.739    99   16.8
    1997- 1-22  13 35.91   20 35.3   2.101   1.603   106   16.5
    1997- 2- 1  13 45.80   20 14.2   2.062   1.474   112   16.1
    

    * C/1996 E1 ( NEAT )

    m1 = 7.4 + 5 log d + 23.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  20 36.26    3 14.9   2.150   2.226    72   16.8
    1996-12- 3  20 47.98   -0 11.5   2.251   2.492    64   17.5
    1996-12-13  20 59.35   -2 45.3   2.354   2.753    56   18.2
    1996-12-23  21 10.45   -4 40.7   2.458   3.003    48   18.8
    1997- 1- 2  21 21.26   -6  7.9   2.562   3.237    39   19.3
    1997- 1-12  21 31.80   -7 14.1   2.666   3.451    31   19.9
    1997- 1-22  21 42.04   -8  4.9   2.770   3.644    23   20.4
    1997- 2- 1  21 51.95   -8 44.5   2.874   3.812    15   20.9
    

    * 43P/Wolf-Harrington

    m1 = 8.0 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  20 34.12   -1 21.8   3.070   3.255    70   17.9
    1996-12- 3  20 44.09   -1 15.5   3.014   3.327    63   17.8
    1996-12-13  20 55.28   -0 58.4   2.957   3.390    56   17.7
    1996-12-23  21  7.54   -0 30.4   2.900   3.441    49   17.6
    1997- 1- 2  21 20.74    0  8.3   2.843   3.480    43   17.5
    1997- 1-12  21 34.77    0 57.4   2.785   3.506    37   17.4
    1997- 1-22  21 49.54    1 56.7   2.726   3.518    31   17.3
    1997- 2- 1  22  4.98    3  5.7   2.667   3.518    26   17.1
    

    * C/1994 J2 ( Takamizawa )

    m1 = 4.2 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   6  4.67   -9 31.8   8.563   7.821   136   18.0
    1996-12- 3   5 58.85   -9 37.3   8.636   7.832   142   18.0
    1996-12-13   5 52.77   -9 35.5   8.709   7.871   146   18.1
    1996-12-23   5 46.68   -9 26.2   8.781   7.942   146   18.1
    1997- 1- 2   5 40.79   -9  9.7   8.853   8.042   143   18.2
    1997- 1-12   5 35.32   -8 46.6   8.925   8.172   137   18.3
    1997- 1-22   5 30.44   -8 17.9   8.997   8.329   130   18.3
    1997- 2- 1   5 26.29   -7 44.8   9.069   8.509   121   18.4
    

    * P/1996 A1 ( Jedicke )

    m1 = 3.0 + 5 log d + 17.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  12  3.49   -6 46.1   4.780   5.234    57   18.1
    1996-12- 3  12  9.87   -7 36.2   4.807   5.123    65   18.1
    1996-12-13  12 15.38   -8 21.6   4.834   5.003    74   18.1
    1996-12-23  12 19.90   -9  1.4   4.862   4.876    83   18.1
    1997- 1- 2  12 23.33   -9 34.8   4.890   4.747    92   18.1
    1997- 1-12  12 25.56  -10  0.9   4.918   4.619   101   18.1
    1997- 1-22  12 26.53  -10 18.8   4.946   4.497   111   18.1
    1997- 2- 1  12 26.22  -10 28.0   4.975   4.385   121   18.1
    

    * 67P/Churyumov-Gerasimenko

    m1 = 9.3 + 5 log d + 11.5 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  13 11.32   -2 58.1   3.214   3.856    43   18.1
    1996-12- 3  13 21.26   -3 56.2   3.276   3.805    51   18.1
    1996-12-13  13 30.26   -4 46.7   3.337   3.740    58   18.2
    1996-12-23  13 38.17   -5 29.0   3.398   3.662    66   18.2
    1997- 1- 2  13 44.85   -6  2.5   3.457   3.574    75   18.3
    1997- 1-12  13 50.12   -6 26.8   3.515   3.479    84   18.3
    1997- 1-22  13 53.81   -6 41.4   3.572   3.379    93   18.3
    1997- 2- 1  13 55.77   -6 46.1   3.629   3.280   102   18.3
    

    * 1996 PW

    m1 = 14.0 + 5 log d + 5.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  22 59.67  -27  2.9   2.781   2.529    94   18.2
    1996-12- 3  23 11.52  -26 12.7   2.826   2.695    87   18.4
    1996-12-13  23 24.18  -25 10.8   2.874   2.862    80   18.6
    1996-12-23  23 37.48  -23 59.7   2.924   3.030    74   18.7
    1997- 1- 2  23 51.23  -22 42.0   2.978   3.196    68   18.9
    1997- 1-12   0  5.30  -21 19.5   3.033   3.360    62   19.0
    1997- 1-22   0 19.61  -19 54.1   3.091   3.520    56   19.2
    1997- 2- 1   0 34.03  -18 27.5   3.150   3.675    51   19.3
    

    * (5145) Pholus

    m1 = 8.0 + 5 log d + 5.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  13 10.50   16  8.0  11.732  12.278    54   18.8
    1996-12- 3  13 13.62   16  7.0  11.758  12.172    63   18.8
    1996-12-13  13 16.37   16 10.4  11.783  12.054    71   18.8
    1996-12-23  13 18.69   16 18.2  11.809  11.928    80   18.7
    1997- 1- 2  13 20.52   16 30.2  11.835  11.797    89   18.7
    1997- 1-12  13 21.82   16 46.0  11.860  11.667    98   18.7
    1997- 1-22  13 22.57   17  5.2  11.886  11.542   108   18.7
    1997- 2- 1  13 22.76   17 27.2  11.912  11.427   117   18.7
    

    * 74P/Smirnova-Chernykh

    m1 = 8.5 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  22 37.97  -16  4.5   4.780   4.608    93   18.6
    1996-12- 3  22 41.11  -15 31.2   4.779   4.766    84   18.7
    1996-12-13  22 45.38  -14 52.1   4.778   4.920    75   18.8
    1996-12-23  22 50.65  -14  7.9   4.777   5.069    67   18.8
    1997- 1- 2  22 56.78  -13 19.5   4.775   5.209    58   18.9
    1997- 1-12  23  3.63  -12 27.4   4.774   5.337    50   18.9
    1997- 1-22  23 11.10  -11 32.4   4.772   5.450    42   19.0
    1997- 2- 1  23 19.05  -10 35.2   4.770   5.548    34   19.0
    

    * 129P/Shoemaker-Levy 3

    m1 = 11.0 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   1 17.22   15 13.6   3.542   2.711   142   18.7
    1996-12- 3   1 14.32   14 41.5   3.520   2.791   131   18.7
    1996-12-13   1 13.35   14 18.9   3.497   2.889   120   18.7
    1996-12-23   1 14.37   14  7.3   3.474   3.000   110   18.8
    1997- 1- 2   1 17.29   14  7.0   3.452   3.119   101   18.9
    1997- 1-12   1 21.98   14 17.5   3.429   3.244    92   18.9
    1997- 1-22   1 28.28   14 38.2   3.406   3.369    83   19.0
    1997- 2- 1   1 36.01   15  7.5   3.384   3.491    75   19.0
    

    * P/1996 N2 ( Elst-Pizarro )

    m1 = 13.5 + 5 log d + 7.5 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  21 50.98  -13 10.9   2.784   2.701    84   19.0
    1996-12- 3  22  1.82  -12 16.2   2.797   2.848    77   19.1
    1996-12-13  22 13.63  -11 13.9   2.811   2.991    69   19.2
    1996-12-23  22 26.19  -10  4.7   2.825   3.130    63   19.4
    1997- 1- 2  22 39.35   -8 49.6   2.839   3.263    56   19.5
    1997- 1-12  22 52.97   -7 29.2   2.854   3.387    49   19.6
    1997- 1-22  23  6.94   -6  4.6   2.869   3.503    43   19.7
    1997- 2- 1  23 21.17   -4 36.6   2.884   3.608    37   19.7
    

    * 111P/Helin-Roman-Crockett

    m1 = 7.0 + 5 log d + 20.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   8  8.36   21 24.9   3.490   2.873   121   20.1
    1996-12- 3   8  7.71   21 39.0   3.491   2.757   131   20.1
    1996-12-13   8  4.97   21 59.5   3.493   2.660   142   20.0
    1996-12-23   8  0.32   22 25.2   3.494   2.585   153   19.9
    1997- 1- 2   7 54.14   22 53.9   3.496   2.536   165   19.9
    1997- 1-12   7 46.99   23 22.8   3.498   2.516   176   19.9
    1997- 1-22   7 39.62   23 49.4   3.501   2.527   170   19.9
    1997- 2- 1   7 32.80   24 11.6   3.504   2.567   158   19.9
    

    * 120P/Mueller 1

    m1 = 14.0 + 5 log d + 10.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23   6 24.44   35 28.5   3.011   2.155   144   20.5
    1996-12- 3   6 17.90   35 55.5   3.035   2.116   154   20.4
    1996-12-13   6  9.58   36 12.4   3.059   2.102   163   20.5
    1996-12-23   6  0.48   36 16.6   3.084   2.117   167   20.5
    1997- 1- 2   5 51.74   36  7.9   3.109   2.161   161   20.6
    1997- 1-12   5 44.36   35 48.0   3.135   2.232   152   20.7
    1997- 1-22   5 39.13   35 20.4   3.162   2.328   141   20.8
    1997- 2- 1   5 36.43   34 48.7   3.189   2.446   131   21.0
    

    * 127P/Holt-Olmstead

    m1 = 14.0 + 5 log d + 15.0 log r
       Date       R.A.      Decl.      r       d    Elong   m1  
    1996-11-23  22  6.18  -17 31.9   2.219   2.051    86   20.8
    1996-12- 3  22 18.64  -15 11.0   2.203   2.151    79   20.8
    1996-12-13  22 32.42  -12 45.4   2.190   2.251    73   20.9
    1996-12-23  22 47.26  -10 15.4   2.178   2.349    67   20.9
    1997- 1- 2  23  2.97   -7 41.7   2.168   2.444    62   21.0
    1997- 1-12  23 19.40   -5  4.8   2.161   2.537    56   21.0
    1997- 1-22  23 36.45   -2 25.5   2.156   2.625    51   21.1
    1997- 2- 1  23 54.02    0 15.2   2.154   2.710    46   21.2
    

    ---------------------------------------------------------------------

    * Finding Charts (PostScript)

    These finding charts are made with StellaNavigator Ver.2.0 for Windows (AstroArts / ASCII) .

    * C/1995 O1 ( Hale-Bopp )
    C/1996 Q1 ( Tabur )
    83KB
    * C/1996 J1 ( Evans-Drinkwater ) 95KB
    * 81P/Wild 2
    118P/Shoemaker-Levy 4
    119P/Parker-Hartley
    C/1994 J2 ( Takamizawa )
    111P/Helin-Roman-Crockett
    120P/Mueller 1
    98KB
    * 116P/Wild 4
    124P/Mrkos
    96P/Machholz 1
    91KB
    * 126P/IRAS
    57P/du Toit-Neujmin-Delporte
    C/1996 N1 ( Brewington )
    129P/Shoemaker-Levy 3
    83KB
    * 22P/Kopff
    P/1996 R2 ( Lagerkvist )
    2P/Encke
    74P/Smirnova-Chernykh
    P/1996 N2 ( Elst-Pizarro )
    127P/Holt-Olmstead
    65KB
    * 85P/Boethin
    65P/Gunn
    C/1996 R1 ( Hergenrother-Spahr )
    85KB
    * 29P/Schwassmann-Wachmann 1
    95P/Chiron
    32P/Comas Sola
    94P/Russell 4
    100P/Hartley 1
    P/1996 A1 ( Jedicke )
    67P/Churyumov-Gerasimenko
    (5145) Pholus
    68KB
    * C/1996 P2 ( Russell-Watson )
    1996 PW
    64KB
    * 46P/Wirtanen
    107P/Wilson-Harrington
    85KB
    * 121P/Shoemaker-Holt 2
    D/1978 C2 ( Tritton )
    64KB
    * C/1996 B2 ( Hyakutake ) 93KB
    * C/1996 E1 ( NEAT )
    43P/Wolf-Harrington
    66KB

    ---------------------------------------------------------------------

    Copyright(C) Seiichi Yoshida (comet@aerith.net). All rights reserved.