C/2012 X2 (PANSTARRS)

메타데이터

항목
Designation C/2012 X2 (PANSTARRS)
Type C
Perihelion (tp_cal, UTC) 2013-03-31T07:31:18.105600Z
Orbit solution date (soln_date, UTC) 2021-04-15T23:32:29Z
Obs used 186
NEO -
M1 12.600
K1 4.500
PC -
Osculating 궤도요소
항목
Epoch (epoch_cal, TDB) 2013-05-10.0000000
e 0.77049741
q (au) 4.748158
a (au) 20.688908
i (deg) 34.123911
Ω (om, deg) 271.023294
ω (w, deg) 215.631135
M (ma, deg) 0.415663

밝기

C/2012 X2 (PANSTARRS) · Magnitude (Full range)

산란 + 전체 선형

$$ M_a = (10.861 + 2.000\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta $$ $$ \theta = 180^\circ - \alpha $$ $$ \Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b) $$ $$ \Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1 $$

모델 상수

항목
H0 10.861
n 2.000
gf 0.970
gb -1.000
k 1.000
δ90 9.954
파라미터 기호 범위 설명
태양·지구거리 1 AU에서의 절대등급 H0 -5 to 20 혜성의 고유 밝기
광도 기울기 파라미터 n 2 to 6 태양거리 변화에 따른 밝기 변화율
전방 산란 비대칭 계수 gf 0.8 to 1 전방 산란의 강도
후방 산란 비대칭 계수 gb -1 to -0.5 후방 산란의 강도
분할 계수 k 0.8 to 1 전·후방 산란 기여도 비율
먼지/가스 밝기 비 δ90 1 to 10 코마에서 먼지 산란 대비 가스 방출의 상대 기여

참고: EPSC-DPS2025-160

잔차 (구간 선형)

$$\epsilon = a \log_{10} r_{\mathrm{au}} + b$$

시작일 (UTC) 끝 (UTC) a b
2012-01-11 2013-03-14 +4.8190 -2.842
2013-03-31 2014-04-24 -8.5263 +5.540

log10 r = log10(태양거리/AU), Δ = 지구거리(AU)

천체력

Date/Time (UTC) RA (J2000) Dec (J2000) Nearest HIP Dist from HIP (arcmin)
2026-03-26 00:00 18:10:51.35 -24:13:24.4 HIP 89043 13.99
2026-03-26 12:00 18:10:51.77 -24:13:19.3 HIP 89043 14.10
2026-03-27 00:00 18:10:52.13 -24:13:14.2 HIP 89043 14.21
2026-03-27 12:00 18:10:52.45 -24:13:09.1 HIP 89043 14.32
2026-03-28 00:00 18:10:52.71 -24:13:04.0 HIP 89043 14.42
2026-03-28 12:00 18:10:52.93 -24:12:58.9 HIP 89043 14.52
2026-03-29 00:00 18:10:53.09 -24:12:53.8 HIP 89043 14.61
2026-03-29 12:00 18:10:53.20 -24:12:48.7 HIP 89043 14.70
2026-03-30 00:00 18:10:53.26 -24:12:43.6 HIP 89043 14.78
2026-03-30 12:00 18:10:53.26 -24:12:38.6 HIP 89043 14.86
2026-03-31 00:00 18:10:53.22 -24:12:33.5 HIP 89043 14.93
2026-03-31 12:00 18:10:53.12 -24:12:28.5 HIP 89043 15.00
2026-04-01 00:00 18:10:52.98 -24:12:23.5 HIP 89043 15.07
2026-04-01 12:00 18:10:52.78 -24:12:18.4 HIP 89043 15.12
2026-04-02 00:00 18:10:52.53 -24:12:13.4 HIP 89043 15.18
2026-04-02 12:00 18:10:52.23 -24:12:08.4 HIP 89043 15.23
2026-04-03 00:00 18:10:51.88 -24:12:03.4 HIP 89043 15.28
2026-04-03 12:00 18:10:51.47 -24:11:58.4 HIP 89043 15.32
2026-04-04 00:00 18:10:51.02 -24:11:53.4 HIP 89043 15.36
2026-04-04 12:00 18:10:50.52 -24:11:48.4 HIP 89043 15.39
2026-04-05 00:00 18:10:49.96 -24:11:43.5 HIP 89043 15.43
2026-04-05 12:00 18:10:49.35 -24:11:38.5 HIP 89043 15.46
2026-04-06 00:00 18:10:48.69 -24:11:33.5 HIP 89043 15.49
2026-04-06 12:00 18:10:47.98 -24:11:28.6 HIP 89043 15.51
2026-04-07 00:00 18:10:47.22 -24:11:23.7 HIP 89043 15.54
2026-04-07 12:00 18:10:46.41 -24:11:18.7 HIP 89043 15.56
2026-04-08 00:00 18:10:45.55 -24:11:13.8 HIP 89043 15.58
2026-04-08 12:00 18:10:44.64 -24:11:08.9 HIP 89043 15.61
2026-04-09 00:00 18:10:43.68 -24:11:03.9 HIP 89043 15.63
2026-04-09 12:00 18:10:42.66 -24:10:59.0 HIP 89043 15.65
2026-04-10 00:00 18:10:41.60 -24:10:54.1 HIP 89043 15.68
2026-04-10 12:00 18:10:40.49 -24:10:49.2 HIP 89043 15.70
2026-04-11 00:00 18:10:39.32 -24:10:44.3 HIP 89043 15.73
2026-04-11 12:00 18:10:38.11 -24:10:39.5 HIP 89043 15.76
2026-04-12 00:00 18:10:36.84 -24:10:34.6 HIP 89043 15.80
2026-04-12 12:00 18:10:35.53 -24:10:29.7 HIP 89043 15.84
2026-04-13 00:00 18:10:34.16 -24:10:24.8 HIP 89043 15.88
2026-04-13 12:00 18:10:32.75 -24:10:20.0 HIP 89043 15.93
2026-04-14 00:00 18:10:31.28 -24:10:15.1 HIP 89043 15.99
2026-04-14 12:00 18:10:29.77 -24:10:10.2 HIP 89043 16.05
2026-04-15 00:00 18:10:28.20 -24:10:05.4 HIP 89043 16.11
2026-04-15 12:00 18:10:26.59 -24:10:00.5 HIP 89043 16.19
2026-04-16 00:00 18:10:24.93 -24:09:55.7 HIP 89043 16.28