P/2014 W4 (PANSTARRS)

메타데이터

항목 값
Designation P/2014 W4 (PANSTARRS)
Type P
Perihelion (tp_cal, UTC) 2015-12-29T12:04:50.476800Z
Orbit solution date (soln_date, UTC) 2021-04-15T23:33:02Z
Obs used 91
NEO -
M1 7.200
K1 15.500
PC -
Osculating 궤도요소
항목 값
Epoch (epoch_cal, TDB) 2015-09-14.0000000
e 0.35307752
q (au) 4.261090
a (au) 6.586710
i (deg) 15.274347
Ω (om, deg) 33.352591
ω (w, deg) 67.411788
M (ma, deg) 353.790386

밝기

P/2014 W4 (PANSTARRS) · Magnitude (Full range)

산란 + 전체 선형

$$ M_a = (6.548 + 6.000\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta $$ $$ \theta = 180^\circ - \alpha $$ $$ \Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b) $$ $$ \Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1 $$

모델 상수

항목 값
H0 6.548
n 6.000
gf 1.000
gb -0.500
k 1.000
δ90 10.000
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

천체력

Date/Time (UTC) RA (J2000) Dec (J2000) Nearest HIP Dist from HIP (arcmin)
2026-09-20 00:00 20:28:58.15 -35:57:52.8 HIP 100990 14.73
2026-09-20 12:00 20:28:52.34 -35:57:17.4 HIP 100990 14.93
2026-09-21 00:00 20:28:46.66 -35:56:41.3 HIP 100990 15.25
2026-09-21 12:00 20:28:41.12 -35:56:04.5 HIP 100990 15.69
2026-09-22 00:00 20:28:35.70 -35:55:27.1 HIP 100990 16.22
2026-09-22 12:00 20:28:30.42 -35:54:49.1 HIP 100990 16.85
2026-09-23 00:00 20:28:25.28 -35:54:10.5 HIP 100990 17.54
2026-09-23 12:00 20:28:20.27 -35:53:31.2 HIP 100990 18.30
2026-09-24 00:00 20:28:15.39 -35:52:51.3 HIP 101017 18.25
2026-09-24 12:00 20:28:10.65 -35:52:10.8 HIP 101017 17.99
2026-09-25 00:00 20:28:06.04 -35:51:29.7 HIP 101017 17.78
2026-09-25 12:00 20:28:01.57 -35:50:48.0 HIP 101017 17.62
2026-09-26 00:00 20:27:57.23 -35:50:05.7 HIP 101017 17.51
2026-09-26 12:00 20:27:53.03 -35:49:22.8 HIP 101017 17.45
2026-09-27 00:00 20:27:48.97 -35:48:39.2 HIP 101017 17.44
2026-09-27 12:00 20:27:45.05 -35:47:55.1 HIP 101017 17.46
2026-09-28 00:00 20:27:41.26 -35:47:10.5 HIP 101017 17.53
2026-09-28 12:00 20:27:37.61 -35:46:25.2 HIP 101017 17.63
2026-09-29 00:00 20:27:34.10 -35:45:39.4 HIP 101017 17.77
2026-09-29 12:00 20:27:30.72 -35:44:53.0 HIP 101017 17.94
2026-09-30 00:00 20:27:27.49 -35:44:06.0 HIP 101017 18.13
2026-09-30 12:00 20:27:24.39 -35:43:18.5 HIP 101017 18.36
2026-10-01 00:00 20:27:21.43 -35:42:30.5 HIP 101017 18.60
2026-10-01 12:00 20:27:18.62 -35:41:41.8 HIP 101017 18.86
2026-10-02 00:00 20:27:15.94 -35:40:52.7 HIP 101017 19.15
2026-10-02 12:00 20:27:13.40 -35:40:02.9 HIP 101017 19.45
2026-10-03 00:00 20:27:11.00 -35:39:12.7 HIP 101017 19.76
2026-10-03 12:00 20:27:08.75 -35:38:21.9 HIP 101017 20.09
2026-10-04 00:00 20:27:06.63 -35:37:30.6 HIP 101017 20.42
2026-10-04 12:00 20:27:04.66 -35:36:38.7 HIP 101017 20.77
2026-10-05 00:00 20:27:02.82 -35:35:46.4 HIP 101017 21.12
2026-10-05 12:00 20:27:01.13 -35:34:53.5 HIP 101017 21.49
2026-10-06 00:00 20:26:59.58 -35:34:00.1 HIP 101017 21.86
2026-10-06 12:00 20:26:58.18 -35:33:06.2 HIP 101017 22.23
2026-10-07 00:00 20:26:56.91 -35:32:11.8 HIP 101017 22.61
2026-10-07 12:00 20:26:55.79 -35:31:16.9 HIP 101017 23.00
2026-10-08 00:00 20:26:54.81 -35:30:21.5 HIP 101017 23.40
2026-10-08 12:00 20:26:53.97 -35:29:25.6 HIP 101017 23.79
2026-10-09 00:00 20:26:53.28 -35:28:29.2 HIP 101017 24.20
2026-10-09 12:00 20:26:52.73 -35:27:32.4 HIP 101021 24.53
2026-10-10 00:00 20:26:52.32 -35:26:35.1 HIP 101021 24.41
2026-10-10 12:00 20:26:52.05 -35:25:37.3 HIP 101021 24.29
2026-10-11 00:00 20:26:51.93 -35:24:39.0 HIP 101021 24.19