Weekly Information about Bright Comets (2009 Aug. 15: South)

Japanese version
Home page
Updated on September 12, 2009
Last week North Next week

Best time and the azimuth, altitude (A,h) are at lat. 35 deg in the Southern Hemisphere.
Azimuth indicates 0 for south, 90 for west, 180 for north, 270 for east.

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

* C/2006 W3 ( Christensen )

Now it is so bright as 8.0 mag (Aug. 11, Juan Jose Gonzalez). It will be observable at 8-10 mag in good condition for a long time until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  20 22.87   22 22.4   2.313   3.150   139    8.0  22:45 (180, 33)  
Aug. 22  20  7.76   18 57.6   2.334   3.158   137    8.1  22:03 (180, 36)  

* C/2008 Q3 ( Garradd )

It brightened up to 6.7 mag in June (June 9, Marco Goiato). Now it is fading, but still bright as 9.5 mag (Aug. 8, Marco Goiato). In the Northern Hemisphere, it is observable until mid August in the evening low sky. In the Southern Hemisphere, it will be getting lower after this, and will be too low to observe in late August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  12 41.23    0 57.9   2.461   1.921    47    9.7  18:53 (111, 26)  
Aug. 22  12 44.28    2 12.1   2.604   1.953    40   10.1  18:58 (107, 20)  

* C/2007 Q3 ( Siding Spring )

It brightened up to 9.8 mag on June 13 (Marco Goiato). Now it is not observable. But it keeps as bright as 10-11 mag for a long time untio 2010 spring. In the Northern Hemisphere, it will appear in the morning sky in early October, then it keeps observable at 10 mag in good condition for a long time. In the Southern Hemisphere, it will locate extremely low only after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   9 19.73    2 40.6   3.312   2.333    12    9.8   5:15 (272, -8)  
Aug. 22   9 32.85    3 24.0   3.296   2.313    11    9.8   5:07 (271, -7)  

* C/2008 T2 ( Cardinal )

It brightened up to 8.5 mag in May and June (May 26, Juan Jose Gonzalez). Now it is fading, but still bright as 9.5 mag (Aug. 8, Marco Goiato). It will never be observable again in the Northern Hemisphere. In the Southern Hemisphere, it keeps observable for a long time after this in the evening sky.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  10 36.16  -37  8.2   1.919   1.539    53    9.9  18:53 ( 59, 22)  
Aug. 22  11  2.39  -40 52.7   1.967   1.605    54   10.1  18:58 ( 55, 23)  

* 22P/Kopff

It brightened up to 8.8 mag in May and June (May 19, Juan Jose Gonzalez). Now it is still bright as 10.2 mag (Aug. 11, Juan Jose Gonzalez). It will be bright at 9-10 mag for a long time until autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  22 56.43  -12 26.4   0.784   1.773   160   10.0   1:24 (180, 67)  
Aug. 22  22 52.83  -13 21.5   0.802   1.804   168   10.2   0:53 (180, 68)  

* 217P/2009 F3 ( LINEAR )

It has already brightened up to 11.3 mag (July 25, Juan Jose Gonzalez). It will be observable at 10-11 mag in a good condition for a long time from summer to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   2 58.35   -2 55.1   0.598   1.265   100   11.5   5:15 (184, 58)  
Aug. 22   3 29.58   -3  3.5   0.585   1.246    99   11.2   5:07 (190, 58)  

* C/2009 F6 ( Yi-SWAN )

It was bright as 8-9 mag in April and May. Now it is not observable. But it will appear in the morning sky again at 12 mag in late August, then it will be fading slowly in the low sky. In the Southern Hemisphere, it keeps observable in good condition for a long time after August.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   7 37.71    6 36.4   2.733   1.930    30   11.5   5:15 (254, 10)  
Aug. 22   7 44.41    3 43.8   2.737   2.002    35   11.7   5:07 (254, 15)  

* 24P/Schaumasse

It reaches up to 11 mag in summer. However, the condition of this apparition is worst. We can not observe it at all.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   9 46.42   19 28.1   2.220   1.216     5   11.6  18:53 (101,-19)  
Aug. 22  10 13.47   17 26.8   2.226   1.225     6   11.7  18:58 ( 98,-19)  

* 88P/Howell

It is so bright as 11.2 mag visually (Aug. 8, Marco Goiato), much brighter than this ephemeris. It will be 10 mag in autumn. It keeps observable for a long time until 2010 February. But in the Northern Hemisphere, it keeps very low after this. It locates a bit higher in the Southern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  13 55.46  -12 54.4   1.529   1.505    69   12.0  18:53 (113, 49)  
Aug. 22  14 12.13  -14 41.1   1.542   1.475    66   11.8  18:58 (107, 47)  

* C/2009 G1 ( STEREO )

It has been observed bright as 8-9 mag from April to June. Now it is fading, but still bright as 11.0 mag (July 12, Marco Goiato). In the Southern Hemisphere, it keeps observable in a good condition for a long time. In the Northern Hemisphere, it will never be observable again.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   9 43.81  -51  5.5   2.346   2.130    65   12.6  18:53 ( 41, 20)  
Aug. 22   9 55.69  -50 41.6   2.485   2.210    62   12.9   5:07 (319, 20)  

* 116P/Wild 4

Now it is very bright as 11.9 mag (July 12, Marco Goiato). However, it will be too low to observe soon. It will appear in the morning sky at 15 mag in early 2010. But it locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  12 20.69   -2 24.9   2.803   2.183    43   13.2  18:53 (105, 24)  
Aug. 22  12 34.01   -3 58.3   2.857   2.188    40   13.2  18:58 (100, 21)  

* C/2007 N3 ( Lulin )

It passed near by the earth in late February, and it reached up to 4.9 mag (Feb. 23, Juan Jose Gonzalez). It had been unobservable for a while, but it is appearing in the morning sky again. Now it is 14.9 mag (Aug. 14, Ken-ichi Kadota). In the Northern Hemisphere, it is observable at 15 mag in good condition from autumn to winter. It may be visible visually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   7 17.64   21  5.5   3.977   3.190    34   14.0   5:15 (240,  5)  
Aug. 22   7 18.99   21  0.5   3.966   3.264    40   14.1   5:07 (237,  8)  

* 64P/Swift-Gehrels

Appearing in the morning sky. Now it is 12.8 mag and visible visually (July 25, Juan Jose Gonzalez). It will be getting higher gradually while fading slowly after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   7  8.15   26 26.3   2.246   1.562    37   14.2   5:15 (234,  3)  
Aug. 22   7 28.49   25 31.9   2.254   1.602    39   14.3   5:07 (235,  4)  

* 29P/Schwassmann-Wachmann 1

Now it is not observable. It will appear in the morning sky in September.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   8 59.71   17 20.3   7.149   6.153     9   14.2   5:15 (257,-12)  
Aug. 22   9  4.89   16 54.5   7.125   6.155    15   14.2   5:07 (256, -9)  

* C/2007 G1 ( LINEAR )

It brightened up to 11.5 mag in last summer (Aug. 4, Marco Goiato). Now it is 15.9 mag (Aug. 12, H. Sato). It keeps observable in good condition for a long time in the Southern Hemisphere. It will be observable again also in the Northern Hemisphere after September. It will keep 15-16 mag until next spring.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   6 30.36  -37 17.3   4.097   3.830    67   14.4   5:15 (290, 46)  
Aug. 22   6 33.88  -37 32.6   4.111   3.878    69   14.5   5:07 (289, 49)  

* C/2006 OF2 ( Broughton )

It brightened up to 9.8 mag in winter (Dec. 28, Juan Jose Gonzalez). It faded down to 12.5 mag in May (May 26, Juan Jose Gonzalez), and became unobservable. Now it is not observable, however, it will be observable in good condition again in winter at 15 mag. Then it may be still visible visually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   9 19.61   16 55.3   5.232   4.225     5   14.4   5:15 (260,-16)  
Aug. 22   9 26.54   16  1.8   5.271   4.279    10   14.5   5:07 (259,-13)  

* 65P/Gunn

Now it is 12.5 mag and visible visually (July 24, Juan Jose Gonzalez). It will be too low to observe soon. It will brighten up to 12-13 mag in 2010 summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  12 58.29   -0 23.1   3.231   2.720    51   14.6  18:53 (113, 30)  
Aug. 22  13  7.53   -1 41.4   3.281   2.702    47   14.6  18:58 (108, 27)  

* 222P/2009 MB9 ( LINEAR )

First return of a new bright periodic comet. It was observed as an asteroid in June. Now it is 17.3 mag by CCD observations (Aug. 3, Siding Spring Survey). However, because it looks very diffuse, the total magnitude can be around 14-15 mag. The condition in this apparition is very good. The comet will pass near by the earth and is expected to reach up to 13-14 mag. Now it locates very low in the Northern Hemisphere, but it keeps observable high until early August in the Southern Hemisphere. It is not observable in latter half of August. In the Northern Hemisphere, it appears in the morning sky at 15 mag in late August, then it keeps observable in a good condition. Maybe it becomes visible visually.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   9 23.30   -1 30.7   0.192   0.830    16   14.6   5:15 (277, -6)  
Aug. 22   8 43.34    8  3.6   0.232   0.798    20   14.8   5:07 (260,  0)  

* C/2008 P1 ( Garradd )

Now it is 14.5 mag (July 30, H. Sato). It keeps observable in good condition at 15 mag until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   0 36.20   22 49.2   3.258   3.901   122   15.0   3:03 (180, 32)  
Aug. 22   0 30.52   24 14.4   3.186   3.905   129   14.9   2:30 (180, 31)  

* 81P/Wild 2

Although it had been unobservable for a long time, it is appearing in the morning sky now. It must be already bright as 15 mag. It will be observable bright as 9-10 mag in a good condition for a long time from winter to spring. It keeps observable until 2010 autumn when it fades down to 16 mag.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   7  8.94   20 45.0   3.118   2.376    36   15.1   5:15 (239,  7)  
Aug. 22   7 23.28   20 21.0   3.026   2.335    39   14.9   5:07 (238,  8)  

* (3552) Don Quixote

Now it is 15.2 mag (Aug. 3, H. Sato). It passes the perihelion in September, and now it is brightest. It keeps observable in good condition in the Southern Hemisphere. It is not observable now in the Northern Hemisphere. But it will appear in the evening sky at the end of September, and then it will be getting higher while fading.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  13 16.27  -55  9.1   0.868   1.252    83   15.1  18:53 ( 43, 52)  
Aug. 22  13 54.65  -56  3.0   0.836   1.231    82   15.1  18:58 ( 41, 53)  

* C/2008 N1 ( Holmes )

Now it is 15.9 mag (July 19, Ken-ichi Kadota). It will brighten up to 15 mag in 2009 and 2010, and will be observable for a long time in good condition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  16 14.44   50 20.4   2.722   2.817    84   15.2  18:53 (177,  5)  
Aug. 22  16  0.56   47 24.5   2.787   2.807    80   15.2  18:58 (170,  7)  

* 67P/Churyumov-Gerasimenko

It brightened very rapidly, faster than expected, and reached up to 9.3 mag in spring (Mar. 26, Juan Jose Gonzalez). However, it will never be observable again in this apparition.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  10 32.97   14  4.6   3.199   2.226    13   15.3  18:53 (102, -7)  
Aug. 22  10 46.25   12 43.2   3.267   2.279    10   15.6  18:58 ( 98,-10)  

* 199P/2008 G2 ( Shoemaker 4 )

It has brightened up to 14 mag in outburst in 2008 August. Now it is bright as 14.3 mag (July 13, H. Sato), brighter than originally expected.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  21  6.08  -41 15.1   2.140   3.071   151   15.3  23:29 (  0, 84)  
Aug. 22  21  2.09  -41 49.2   2.187   3.086   147   15.4  22:58 (  0, 83)  

* P/2009 L2 ( Yang-Gao )

New bright periodic comet. It is still bright as 13.3 mag and visible visually (July 13, Carlos Labordena). Moving northwards in the Milky Way. In the Northern Hemisphere, the condition becomes good after this. But the comet will fade out rapidly. It will be fainter than 15 mag in August, and fainter than 18 mag in October.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  18 47.76    4  7.8   0.749   1.625   133   15.5  21:12 (180, 51)  
Aug. 22  18 54.72    3 45.1   0.827   1.671   130   15.8  20:52 (180, 51)  

* P/2009 K1 ( Gibbs )

New periodic comet. It has already passed the perihelion in late June. But unexpectedly, it keeps unusual brightening very rapidly after that. Now it became bright as 15.0 mag (July 30, D. Chestnov). It keeps observable in the evening low sky for a while after this. But it may fade out very rapidly.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  13 26.69   -4 11.6   1.671   1.449    59   15.5  18:53 (116, 38)  
Aug. 22  13 49.53   -6 17.8   1.728   1.484    58   15.8  18:58 (112, 38)  

* C/2006 Q1 ( McNaught )

It reached to 10.9 mag in 2008 spring (May 11, Marco Goiato). It is fading slowly. Now it is 13.4 mag (June 1, Juan Jose Gonzalez), still visible visually. It keeps bright as 13-14 mag for a long time after this until summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  16  6.32   33 13.6   4.751   4.823    88   15.6  18:53 (175, 22)  
Aug. 22  16  8.80   32 27.1   4.864   4.874    84   15.7  18:58 (168, 22)  

* C/2005 L3 ( McNaught )

Now it is 13.4 mag and visible visually (July 18, Jose Carvajal). It had been bright and visible visually around 13 mag from spring to autumn in 2008. It will be visible visually at 14 mag again until summer.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  13  4.04   32 51.7   7.545   6.940    50   15.7  18:53 (139,  7)  
Aug. 22  13  4.63   32 22.7   7.632   6.969    46   15.7  18:58 (133,  3)  

* C/2009 O4 ( Hill )

Now it is 15.7 mag (Aug. 11, Ken-ichi Kadota). It keeps 15 mag until winter. It keeps observable in a good condition in the Southern Hemisphere. But in the Northern Hemisphere, it will be getting lower gradually, and it is only observable until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   0 26.64    1 36.1   2.151   2.959   135   15.9   2:54 (180, 53)  
Aug. 22   0 21.48   -1 48.8   2.040   2.923   144   15.7   2:21 (180, 57)  

* C/2006 S3 ( LONEOS )

Now it is 16.2 mag (Aug. 13, Ken-ichi Kadota), brightening as expected. It will reach up to 12 mag in 2012, and will be observable visually at 12-13 mag for a long time from 2011 to 2013. In 2009, it is observable in good condition at 16 mag from summer to autumn. In the Northern Hemisphere, the comet will be low around its brightest seasons.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  22 27.50    5  2.5   7.729   8.672   157   15.8   0:55 (180, 50)  
Aug. 22  22 22.95    4 41.4   7.664   8.636   162   15.8   0:23 (180, 50)  

* 118P/Shoemaker-Levy 4

Now it is 17.1 mag (July 26, Ken-ichi Kadota). It will brighten rapidly after this. It will reach to 12 mag and become visible visually in winter. In the Northern Hemisphere, it keeps observable in good condition for a long time after this until 2010 spring when it fades out.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   4 21.25   13 31.9   2.274   2.263    76   16.4   5:15 (208, 37)  
Aug. 22   4 33.48   13 36.7   2.176   2.239    80   16.2   5:07 (206, 37)  

* P/2003 A1 ( LINEAR )

Appearing in the morning sky. It has not been recovered yet. But it must have already brightened up to 16.5 mag. It will be getting higher rapidly after this, and will be observable in good condition at 16 mag in autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   5 35.75   27 25.1   2.334   1.986    57   16.5   5:15 (218, 16)  
Aug. 22   5 49.19   29 26.4   2.279   2.003    61   16.4   5:07 (216, 15)  

* C/2008 FK75 ( Lemmon-Siding Spring )

Now it is 16.4 mag (June 12, Ken-ichi Kadota). It will reach to 15 mag in 2010. It keeps observable for a long time after this in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  15  6.95    8  7.8   5.643   5.567    80   16.7  18:53 (152, 43)  
Aug. 22  15  9.12    8  3.5   5.711   5.535    74   16.7  18:58 (143, 40)  

* 47P/Ashbrook-Jackson

It brightened up to 15-16 mag in 2008 summer. Now appearing in the morning sky again. It keeps observable at 17 mag in good condition for a long time from summer to winter.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   3 36.22   28 34.0   2.949   3.011    83   17.0   5:15 (192, 25)  
Aug. 22   3 42.07   29 26.1   2.870   3.025    88   17.0   5:07 (188, 25)  

* (3200) Phaethon

It passed the perihelion in June, but it was not observable, too close to the sun. Although it was predicted to be 13.5 mag, the STEREO spacecraft revealed that it brightened up to 10-11 mag, much brighter than expected. Now it is 15.8 mag (July 17, Michael Jager). It keeps observable at 16-17 mag until late autumn.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   4 38.26   43 48.1   1.179   1.257    69   17.0   5:15 (200,  7)  
Aug. 22   4 35.84   45 12.2   1.169   1.350    76   17.1   5:07 (195,  7)  

* C/2007 U1 ( LINEAR )

It reached up to 14 mag in 2008 autumn. It is still bright as 16.0 mag (July 30, H. Sato). It keeps observable around 17 mag in a good condition for a while.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  22 44.70   19 17.4   3.907   4.753   142   17.3   1:12 (180, 36)  
Aug. 22  22 33.97   18 36.1   3.903   4.796   148   17.3   0:34 (180, 36)  

* P/2008 O2 ( McNaught )

It was observed at 17.5 mag in 2008 summer. It is also observable at 17.5 mag in 2009 autumn. In the Northern Hemisphere, it located somewhat low in 2008, but it becomes observable in good condition in 2009. However, it is 19.0 mag recently (July 26, Ken-ichi Kadota), much fainter than this ephemeris.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   1 12.18   16  5.0   3.228   3.824   119   17.6   3:39 (180, 39)  
Aug. 22   1 11.47   16 23.6   3.147   3.827   125   17.5   3:11 (180, 39)  

* 107P/(4015) Wilson-Harrington

Now it is 17.0 mag (June 26, Charles Bell). The condition is good in this apparition. It will approach to the earth down to 0.38 A.U., and will be observable in good condition at 16.5 mag in November. It keeps observable until that time after this. But it locates somewhat low in the Northern Hemisphere.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  16  5.87  -18 53.4   0.690   1.329   100   17.6  18:53 (161, 73)  
Aug. 22  16 12.02  -18 47.3   0.682   1.274    95   17.6  18:58 (143, 71)  

* P/2008 J3 ( McNaught )

It was observed around 17 mag from autumn to winter in 2008. It has not been observed since January, but now it is observable in good condition again. It will fade out gradually after this.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   5 21.46   41  4.5   2.872   2.547    61   17.7   5:15 (208,  6)  
Aug. 22   5 34.74   42 10.1   2.820   2.569    65   17.7   5:07 (206,  6)  

* C/2008 S3 ( Boattini )

It keeps observable at 17 mag for a long time from 2010 to 2012.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   3 47.39   20 38.0   9.017   8.949    82   17.8   5:15 (196, 33)  
Aug. 22   3 46.13   20 41.0   8.874   8.931    89   17.7   5:07 (191, 34)  

* C/2007 VO53 ( Spacewatch )

It keeps observable at 17-18 mag for a long time until 2011.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15   4 27.85   63 30.2   5.459   5.233    71   17.9   5:15 (191,-10)  
Aug. 22   4 31.03   65  7.3   5.356   5.213    76   17.8   5:07 (189,-11)  

* C/2009 K2 ( Catalina )

It will be getting lower in the evening sky after this. But it will be observable at 17 mag from spring to summer in 2010.

Date(TT)  R.A. (2000) Decl.   Delta     r    Elong.  m1   Best Time(A, h)  
Aug. 15  16  3.60   43 19.7   3.597   3.649    84   17.9  18:53 (175, 12)  
Aug. 22  16  7.53   40 59.7   3.603   3.620    82   17.9  18:58 (170, 13)  

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

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