C/2016 VZ18 (PANSTARRS)

메타데이터

항목
Designation C/2016 VZ18 (PANSTARRS)
Type C
Perihelion (tp_cal, UTC) 2017-03-07T09:07:19.603200Z
Orbit solution date (soln_date, UTC) 2021-04-15T23:33:28Z
Obs used 351
NEO -
M1 18.400
K1 9.000
PC 0.030
Osculating 궤도요소
항목
Epoch (epoch_cal, TDB) 2017-02-20.0000000
e 0.99532240
q (au) 0.910266
a (au) 194.601204
i (deg) 24.035635
Ω (om, deg) 98.954808
ω (w, deg) 36.386221
M (ma, deg) 359.994416

밝기

C/2016 VZ18 (PANSTARRS) · Magnitude (Full range)

산란 + 전체 선형

$$ M_a = (14.990 + 6.000\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta $$ $$ \theta = 180^\circ - \alpha $$ $$ \Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b) $$ $$ \Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1 $$

모델 상수

항목
H0 14.990
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)
2026-03-26 00:00 19:49:27.40 -26:50:32.3 HIP 97613 14.35
2026-03-26 12:00 19:49:29.66 -26:50:35.6 HIP 97613 13.96
2026-03-27 00:00 19:49:31.87 -26:50:39.0 HIP 97613 13.58
2026-03-27 12:00 19:49:34.04 -26:50:42.6 HIP 97613 13.22
2026-03-28 00:00 19:49:36.17 -26:50:46.3 HIP 97613 12.88
2026-03-28 12:00 19:49:38.25 -26:50:50.2 HIP 97613 12.55
2026-03-29 00:00 19:49:40.29 -26:50:54.2 HIP 97613 12.24
2026-03-29 12:00 19:49:42.28 -26:50:58.3 HIP 97613 11.95
2026-03-30 00:00 19:49:44.23 -26:51:02.5 HIP 97613 11.68
2026-03-30 12:00 19:49:46.14 -26:51:06.9 HIP 97613 11.43
2026-03-31 00:00 19:49:48.00 -26:51:11.4 HIP 97613 11.20
2026-03-31 12:00 19:49:49.81 -26:51:16.1 HIP 97613 10.99
2026-04-01 00:00 19:49:51.58 -26:51:20.9 HIP 97613 10.80
2026-04-01 12:00 19:49:53.30 -26:51:25.8 HIP 97613 10.63
2026-04-02 00:00 19:49:54.98 -26:51:30.8 HIP 97613 10.47
2026-04-02 12:00 19:49:56.61 -26:51:36.0 HIP 97613 10.34
2026-04-03 00:00 19:49:58.20 -26:51:41.3 HIP 97613 10.23
2026-04-03 12:00 19:49:59.74 -26:51:46.7 HIP 97613 10.13
2026-04-04 00:00 19:50:01.23 -26:51:52.3 HIP 97613 10.05
2026-04-04 12:00 19:50:02.68 -26:51:58.0 HIP 97613 10.00
2026-04-05 00:00 19:50:04.09 -26:52:03.8 HIP 97613 9.95
2026-04-05 12:00 19:50:05.44 -26:52:09.8 HIP 97613 9.93
2026-04-06 00:00 19:50:06.75 -26:52:15.9 HIP 97613 9.92
2026-04-06 12:00 19:50:08.02 -26:52:22.1 HIP 97613 9.92
2026-04-07 00:00 19:50:09.24 -26:52:28.5 HIP 97613 9.94
2026-04-07 12:00 19:50:10.41 -26:52:35.0 HIP 97613 9.98
2026-04-08 00:00 19:50:11.53 -26:52:41.6 HIP 97613 10.02
2026-04-08 12:00 19:50:12.61 -26:52:48.3 HIP 97613 10.08
2026-04-09 00:00 19:50:13.64 -26:52:55.2 HIP 97613 10.15
2026-04-09 12:00 19:50:14.63 -26:53:02.2 HIP 97613 10.22
2026-04-10 00:00 19:50:15.56 -26:53:09.3 HIP 97613 10.31
2026-04-10 12:00 19:50:16.45 -26:53:16.6 HIP 97613 10.40
2026-04-11 00:00 19:50:17.29 -26:53:24.0 HIP 97613 10.51
2026-04-11 12:00 19:50:18.09 -26:53:31.5 HIP 97613 10.62
2026-04-12 00:00 19:50:18.84 -26:53:39.2 HIP 97613 10.73
2026-04-12 12:00 19:50:19.54 -26:53:47.0 HIP 97613 10.85
2026-04-13 00:00 19:50:20.19 -26:53:54.9 HIP 97613 10.98
2026-04-13 12:00 19:50:20.79 -26:54:02.9 HIP 97613 11.11
2026-04-14 00:00 19:50:21.35 -26:54:11.1 HIP 97613 11.24
2026-04-14 12:00 19:50:21.86 -26:54:19.3 HIP 97613 11.38
2026-04-15 00:00 19:50:22.32 -26:54:27.8 HIP 97613 11.52
2026-04-15 12:00 19:50:22.74 -26:54:36.3 HIP 97613 11.66
2026-04-16 00:00 19:50:23.10 -26:54:45.0 HIP 97613 11.81