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It brightened rapidly in outburst in mid October. Now it is bright as 7.8 mag (Feb. 22, Maik Meyer). It keeps 8-9 mag for a long time until early summer, and it keeps observable in the morning sky in the Northern Hemisphere. In the Southern Hemisphere, it is getting higher and it will be observable in excellent condition after spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 19 19.13 0 22.9 2.002 1.602 52 8.2 4:18 (256, 19)
Mar. 8 19 37.04 -0 44.5 1.980 1.611 53 8.2 4:26 (254, 23)
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It passed only 0.4 A.U. from the earth, and 0.8 A.U. from the sun in November and December, and brightened up to 4.7 mag (Nov. 28, Juan Jose Gonzalez). Now it is 8.0 mag (Feb. 22, Maik Meyer). In the Northern Hemisphere, it keeps observable in excellent condition for a long time until 2014 autumn when the comet will fade out. It is getting higher in the morning sky also in the Southern Hemisphere, and it keeps observable in good condition after this.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 18 31.20 0 31.7 1.590 1.462 64 9.0 4:18 (247, 28)
Mar. 8 18 33.07 -1 4.9 1.588 1.556 69 9.2 4:26 (242, 35)
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Now it is bright as 11.7 mag (Mar. 1, Marco Goiato). The brightening is somewhat slow, but it is expected to brighten up to 6-7 mag in 2014 autumn. It keeps observable in good condition for a long time in the Northern Hemisphere. It keeps locating low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 16 35.34 20 21.0 2.553 2.822 95 11.4 4:18 (208, 30)
Mar. 8 16 32.11 22 47.9 2.369 2.742 101 11.1 4:26 (197, 30)
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First return of a new periodic comet discovered in 1998. It brightened up to 10 mag at the discovery. Now it is 11.8 mag (Feb. 22, Carlos Labordena). A bit fainter than originally expected. But in the Northern Hemisphere, it keeps observable in excellent condition from autumn to spring. It locates somewhat low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 6 22.99 25 5.9 1.544 2.159 115 12.3 20:05 (175, 30)
Mar. 8 6 29.36 23 44.1 1.611 2.157 109 12.4 19:54 (173, 31)
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It passed the perihelion on Feb. 15. It is appearing in the evening sky in the Northern Hemisphere. It will be observable also in the Southern Hemisphere in early March. Then it keeps observable while the comet will fade out very rapidly.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 0 58.19 -0 16.1 1.196 0.662 33 12.6 20:05 ( 93, 4)
Mar. 8 1 43.99 3 9.9 1.147 0.723 38 13.3 19:54 (100, 8)
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It reaches up to 12 mag in 2014 spring. But the condition in this apparition is bad. It locates low around the brightest days. Now it is not observable. It will appear in the morning sky at 13 mag in late July.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 23 23.85 -1 24.4 2.839 1.877 11 13.5 20:05 ( 78,-15)
Mar. 8 23 40.70 0 2.6 2.822 1.846 8 13.3 19:54 ( 79,-16)
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Already bright as 14.4 mag (Jan. 3, Mt. Lemmon Survey). It will brighten up to 13 mag and to be observable in excellent condition from spring to summer.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 14 7.43 -13 29.0 1.952 2.656 125 13.6 3:34 (180, 69)
Mar. 8 14 9.60 -13 28.2 1.870 2.643 132 13.4 3:08 (180, 69)
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It brightened up to 2 mag by unusual major outburst in 2007. It is coming back now. It will be 14 mag at best by normal prediction. But actually, it is already very bright as 13.5 mag (Nov. 25, Hidetaka Sato). Now it is not observable. It will appear in the morning sky in May.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 22 41.60 -4 58.7 3.056 2.067 3 13.5 4:18 (291,-19)
Mar. 8 22 55.77 -2 53.4 3.050 2.062 4 13.4 4:26 (285,-16)
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Now it is 14.7 mag (Jan. 27, Taras Prystavski).
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 15 57.30 -30 8.3 5.967 6.160 96 13.8 4:18 (255, 75)
Mar. 8 15 58.37 -30 21.3 5.855 6.159 103 13.8 4:26 (237, 82)
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Now it is 14.1 mag and visible visually (Feb. 24, Chris Wyatt). It is expected to brighten up to 7.5 mag and to be observable in excellent condition from summer to autumn in 2014 in the Southern Hemisphere. The condition is bad in the Northern Hemisphere. It will pass extremely close to Mars in 2014 October.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 2 37.86 -30 47.3 3.793 3.382 58 13.9 20:05 ( 77, 39)
Mar. 8 2 36.99 -29 43.4 3.795 3.311 54 13.8 19:54 ( 76, 36)
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It brightened up to 11-12 mag in 2012. Now it is 14.1 mag (Jan. 26, Taras Prystavski). It will be observable in good condition at 14 mag until 2014 early summer.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 13 1.40 -13 35.4 6.395 7.185 140 13.8 2:28 (180, 69)
Mar. 8 12 55.90 -13 13.4 6.354 7.219 148 13.8 1:55 (180, 68)
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Now it is 13.9 mag and visible visually (Feb. 1, Chris Wyatt). It keeps 14 mag for a long time until 2014 summer. It keeps observable in good condition in the Northern Hemisphere. It is observable only until February in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 2 43.77 30 30.6 1.904 1.795 68 13.9 20:05 (132, 4)
Mar. 8 2 48.27 33 30.4 1.957 1.762 63 13.9 19:54 (133, 0)
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Now it is 12.9 mag (Nov. 27, Sandor Szabo). It keeps bright at 13-14 mag for a long time until 2014. In the Northern Hemisphere, it will be getting higher gradually, and it keeps observable for a long time after this. In the Southern Hemisphere, it keeps unobservable until March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 19 54.19 4 26.8 6.897 6.232 44 14.1 4:18 (258, 9)
Mar. 8 19 55.74 4 24.7 6.839 6.248 50 14.1 4:26 (253, 16)
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Now it is bright as 13.2 mag (Jan. 28, Taras Prystavski). It keeps 13-14 mag and observable in good condition in the Northern Hemisphere for a long time from 2013 to 2014. In the Southern Hemisphere, it is not observable until 2014 autumn.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 0 4.46 57 46.7 3.755 3.497 67 14.2 20:05 (141,-34)
Mar. 8 0 13.11 56 27.0 3.850 3.508 62 14.2 19:54 (139,-34)
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Although it had been unobservable for a while, it is appearing in the morning sky. Now it is 15.2 mag (Feb. 6, Taras Prystavski). It keeps bright as 13-14 mag for a long time from 2013 to 2014.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 19 30.60 -26 19.4 3.600 3.059 50 14.5 4:18 (282, 31)
Mar. 8 19 41.42 -26 10.4 3.524 3.058 54 14.5 4:26 (279, 36)
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It brightened very rapidly, and brightened up to 10.5 mag from autumn to winter. Now it is fading, but it is bright as 14.3 mag still now (Feb. 11, Yasukazu Ikari). It is visible visually at 12.2 mag still now (Feb. 22, Carlos Labordena). In the Northern Hemisphere, it keeps observable in excellent condition until May when it becomes fainter than 18 mag. It will not be observable after this in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 2 33.03 32 24.7 1.961 1.822 67 14.5 20:05 (132, 1)
Mar. 8 2 54.43 33 23.2 2.046 1.858 64 15.0 19:54 (133, 1)
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New bright comet discovered in the STEREO spacecraft images. It brightened up to 3.8 mag on Jan. 31 thanks to the forward scattering. It was observed at 15.2 mag on the ground (Feb. 20, Hidetaka Sato). It approached to the Sun down to 0.5 a.u. on Feb. 18. Because the absolute magnitude is faint as 18 mag, it may be disintegrated. It is appearing in the morning sky in the Northern Hemispehre. In the Southern Hemispehre, it will not observable after this. Colin Drescher reported the comet was visible on SWAN images for several days in late December at about 11 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 21 1.52 15 57.2 0.768 0.573 35 15.0 4:18 (258,-10)
Mar. 8 22 15.57 33 48.6 0.651 0.660 41 15.3 4:26 (246,-27)
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Big asteroid discovered in 1906. It suddenly showed the cometary activity on Dec. 11, 2010, probably due to an impact of a small object. It has already turned to be stellar.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 1 17.84 -0 34.4 3.986 3.268 38 15.2 20:05 ( 95, 8)
Mar. 8 1 25.85 0 32.8 4.054 3.275 33 15.1 19:54 ( 95, 5)
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It became much brighter than expected, and reached up to 8.5 mag (Aug. 15, Alexandre Amorim). Now it is fading rapidly, but it is bright as 13.8 mag still now (Jan. 28, Taras Prystavski). In the Southern Hemisphere, it will keep observable in good condition for a long time until 2014 summer when the comet fades out. It will never be observable again in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 17 13.15 -69 42.3 2.947 2.949 80 15.3 4:18 (342, 50)
Mar. 8 17 16.16 -70 11.2 2.941 3.019 84 15.5 4:26 (345, 52)
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It brightened up to 14.0 mag from spring to summer in 2013 (June 11, Sandor Szabo). Now it is 14.9 mag, much brighter than origianlly predicted (Jan. 27, Taras Prystavski). In the Northern Hemisphere, it will be observable at 15-16 mag in excellent condition until spring. It locates somewhat low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 13 19.54 22 43.7 3.435 4.245 140 15.5 2:46 (180, 32)
Mar. 8 13 10.63 24 59.3 3.429 4.283 145 15.6 2:10 (180, 30)
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It is expected to brighten up to 13 mag and to be observable in good condition in 2015. Now it is 15.9 mag (Jan. 26, Taras Prystavski). In 2014, it will be observable at 15 mag in good condition from winter to summer.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 14 1.94 -3 59.6 4.285 4.979 129 15.6 3:28 (180, 59)
Mar. 8 14 1.62 -3 38.7 4.165 4.937 136 15.5 3:00 (180, 59)
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Now it is 14.7 mag (Jan. 19, Taras Prystavski). It keeps 15 mag until March, and will be observable in excellent condition in the Northern Hemisphere. It locates low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 5 12.40 32 33.4 1.316 1.774 99 15.6 20:05 (161, 19)
Mar. 8 5 27.71 31 45.6 1.372 1.773 95 15.7 19:54 (160, 20)
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Now it is 15.7 mag (Jan. 27, Taras Prystavski), brighter than origianlly predicted. It will be observable at 14-16 mag for a long time from 2013 to 2014.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 16 14.45 -23 24.6 3.823 4.019 94 15.9 4:18 (243, 69)
Mar. 8 16 17.57 -23 44.2 3.730 4.031 100 15.9 4:26 (227, 74)
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Now it is 15.0 mag (Feb. 24, Taras Prystavski). Somewhat brighter than this ephemeris, so it can be brightening rapidly. It will be observable in excellent condition from spring to summer in the Southern Hemisphere. It locates somewhat low in the Northern Hemispehre.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 7 52.01 -25 13.9 1.574 2.302 126 16.1 21:15 (180, 80)
Mar. 8 7 50.46 -24 45.2 1.563 2.258 122 16.0 20:46 (180, 80)
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Now it is 16.5 mag (Feb. 19, Hidetaka Sato). It is observable at 16 mag in excellent condition at opposition in March. But it will fade out very rapidly after that. It will be fainter than 18 mag in May.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 14 53.58 -10 0.3 1.245 1.901 116 16.3 4:18 (181, 65)
Mar. 8 14 27.46 -4 16.4 1.132 1.930 130 16.1 3:27 (180, 60)
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Now it is 16.5 mag (Feb. 20, A. Klotz, F. Kugel, C. Rinner). It will approach to the earth down to 0.68 a.u., brighten up to 16 mag, and will be observable in excellent condition in spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 12 3.67 24 14.0 0.736 1.688 155 16.3 1:31 (180, 31)
Mar. 8 11 49.02 21 24.1 0.703 1.674 161 16.2 0:49 (180, 34)
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Now it is 15.1 mag (Jan. 20, Taras Prystavski). It will be fading after this, but it keeps brighter than 18 mag until 2015 spring.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 3 6.32 -14 23.8 8.209 7.824 63 16.2 20:05 ( 99, 38)
Mar. 8 3 7.71 -13 33.9 8.330 7.857 58 16.3 19:54 ( 98, 34)
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Now it is 17.0 mag (Jan. 24, A. Klotz, F. Kugel). It keeps close to the earth around 0.7 a.u. until spring. It will brighten up to 16.5 mag in February and March, and will be observable in excellent condition in the Northern Hemisphere. It locates very low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 4 1.68 35 7.0 0.622 1.127 85 16.5 20:05 (148, 11)
Mar. 8 4 43.31 35 24.0 0.622 1.143 86 16.5 19:54 (153, 13)
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Now it is 15.8 mag (Jan. 18, Taras Prystavski). It keeps 16 mag for a long time until 2015 summer. It keeps observable in good condition in the Northern Hemisphere. It becomes observable only after 2015 in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 4 42.80 52 43.9 3.853 4.071 95 16.5 20:05 (163, -1)
Mar. 8 4 47.56 52 35.5 3.912 4.040 90 16.5 19:54 (161, -2)
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Now it is 16.6 mag (Feb. 20, Katsumi Yoshimoto). It is expected to brighten up to 6 mag in 2014 autumn. At this time, it keeps observable while brightening gradually until April when it becomes 16 mag.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 5 3.50 20 18.3 3.121 3.381 96 16.8 20:05 (153, 30)
Mar. 8 4 58.41 19 58.8 3.172 3.297 88 16.7 19:54 (148, 28)
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It brightened very rapidly in mid November, from 15 mag to 9 mag only within a week. Now it is fading very rapidly. It has already faded down to 18.8 mag (Feb. 20, Katsumi Yoshimoto). It is observable in excellent condition in the Northern Hemisphere. It keeps locating extremely low in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 11 0.53 55 0.8 1.316 2.117 132 17.0 0:28 (180, 0)
Mar. 8 10 54.20 55 3.6 1.408 2.181 129 17.6 23:49 (180, 0)
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Now it is 17.6 mag (Jan. 19, Taras Prystavski). It will approach to the earth down to 0.06 a.u. from May to June, and it is expected to brighten up to 11 mag. In the Northern Hemisphere, it keeps observable in excellent condition until the highlight in late May while the comet will be brightening rapidly. In the Southern Hemisphere, it is not observable now. But it will be observable in mid May. Then it keeps observable in excellent condition at the highlight and after that while the comet will be fading.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 7 27.97 72 42.5 0.621 1.327 108 17.2 20:51 (180,-18)
Mar. 8 7 8.36 73 11.0 0.597 1.268 102 17.1 20:04 (180,-18)
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It brightened up to 12-13 mag from autumn to winter in 2012. Now it is fading. But actually, it is 15.7 mag, brighter than this ephemeris (Jan. 26, Taras Prystavski). It will be observable until April in the Northern Hemisphere, or May in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 5 33.87 -1 26.1 4.900 5.189 101 17.1 20:05 (151, 53)
Mar. 8 5 35.51 -1 10.5 5.046 5.236 95 17.2 19:54 (146, 51)
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It approached to the sun down to 0.73 A.U. on 2013 Mar. 24, and brightened up to 4.7 mag (Mar. 11, Michael Mattiazzo). Now it is fading. It has already faded down to 16.5 mag (Feb. 2, A. Diepvens). In the Northern Hemisphere, it keeps observable in good condition while fading gradually. In the Southern Hemisphere, it will never be observable again.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 20 58.77 55 16.8 5.045 4.745 66 17.2 4:18 (221,-29)
Mar. 8 21 5.47 56 28.4 5.121 4.817 66 17.3 4:26 (218,-26)
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Now it is 17.8 mag (Oct. 13, Mt. Lemmon Survey). Distant object, but it keeps observable at 14 mag for a long time from 2015 to 2016.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 19 2.53 -5 30.6 7.980 7.466 55 17.2 4:18 (258, 26)
Mar. 8 19 5.91 -5 14.8 7.856 7.432 61 17.2 4:26 (252, 32)
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It keeps 17-18 mag for a long time from 2013 to 2014. It is observable in excellent condition in the Southern Hemisphere. It is not observable in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 14 15.62 -53 52.0 4.334 4.680 104 17.4 3:42 ( 0, 71)
Mar. 8 14 4.92 -55 19.1 4.246 4.678 109 17.3 3:04 ( 0, 70)
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Now it is 17.6 mag (Jan. 27, K. Sarneczky). It keeps observable at 18 mag for a long time from 2013 to 2016. It keeps locating high in the Northern Hemisphere. It keeps locating very low in the Southern Hemipshere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 19 14.29 31 16.0 6.940 6.566 63 17.4 4:18 (231, 0)
Mar. 8 19 15.57 32 25.9 6.873 6.558 67 17.4 4:26 (225, 4)
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It passed the perihelion on 2013 Mar. 10, and brightened up to 0-1 mag. Now it is fading. It has already faded down to 17.1 mag (Feb. 12, A. Diepvens). It will keep 16-17 mag until spring. It is not observable in the Southern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 17 22.57 31 12.2 5.208 5.240 86 17.4 4:18 (213, 15)
Mar. 8 17 22.63 32 6.4 5.208 5.312 90 17.5 4:26 (205, 18)
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Now it is 16.9 mag (Jan. 29, Taras Prystavski). It tends to be brightest 4 months after the perihelion passage. However, it has already started fading. It will be fainter than 18 mag in March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 6 3.51 23 20.3 2.069 2.591 110 17.8 20:05 (170, 31)
Mar. 8 6 8.79 23 35.1 2.190 2.626 104 18.0 19:54 (167, 30)
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Now it is 17.4 mag (Jan. 15, A. Hidas). It is expected to brighten up to 14 mag from autumn to winter in 2015. The condition is excellent in the Southern Hemisphere, and it keeps observable for a long time after this while the comet will be brightening. In the Northern Hemisphere, it will be unobservable in late March.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 5 10.40 -32 50.4 6.033 6.127 90 17.8 20:05 ( 90, 71)
Mar. 8 5 7.46 -31 37.8 6.072 6.088 86 17.8 19:54 ( 91, 67)
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Now it is 17.4 mag (Jan. 31, iTelescope Observatory, Siding Spring). It keeps 17-18 mag for a long time from 2014 to 2016.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 15 26.43 -13 13.0 5.463 5.837 107 17.8 4:18 (202, 67)
Mar. 8 15 22.10 -13 13.7 5.321 5.817 115 17.8 4:21 (180, 68)
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It keeps 18 mag for a very long time from 2013 to 2018. It locates high in the Southern Hemisphere. But it locates somewhat low in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 11 8.55 -19 18.7 8.465 9.354 152 17.8 0:35 (180, 74)
Mar. 8 11 6.61 -19 8.5 8.434 9.348 155 17.8 0:06 (180, 74)
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Now it is 18.3 mag (Jan. 25, iTelescope Observatory, Siding Spring). It keeps 18 mag from spring to summer. It is observable in good condition in the Southern Hemisphere. It is not observable in the Northern Hemisphere.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 14 41.90 -48 18.0 0.637 1.300 103 17.9 4:08 ( 0, 77)
Mar. 8 15 6.13 -52 40.4 0.632 1.301 104 17.9 4:04 ( 0, 72)
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Now it is 19.9 mag (Feb. 27, D. T. Durig, et al.). First return of a new periodic comet which brightened up to 13 mag in outburst in 2008. It will be observable in good condition from spring to summer. However, it will be only 19-20 mag at best in this apparition.
Date(TT) R.A. (2000) Decl. Delta r Elong. m1 Best Time(A, h)
Mar. 1 12 47.49 11 56.0 1.694 2.600 149 19.9 2:14 (180, 43)
Mar. 8 12 44.61 12 46.1 1.644 2.583 156 19.8 1:44 (180, 42)
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