| Parameter |
Value |
| Designation |
C/2002 V1 (NEAT) |
| Type |
C |
| Perihelion (tp_cal, UTC) |
2003-02-18T07:05:52.609920Z |
| Orbit solution date (soln_date, UTC) |
2021-04-15T23:30:22Z |
| Obs used |
1510 |
| NEO |
- |
| M1 |
10.400 |
| K1 |
14.250 |
| PC |
0.030 |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2002-12-26.0000000 |
| e |
0.99990177 |
| q (au) |
0.099258 |
| a (au) |
1010.516972 |
| i (deg) |
81.706057 |
| Ω (om, deg) |
64.088430 |
| ω (w, deg) |
152.169686 |
| M (ma, deg) |
359.998334 |
Magnitude
Scatter + Global Linear
$$
M_a = (8.600 + 5.819\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
8.600 |
| n |
5.819 |
| gf |
0.800 |
| gb |
-0.500 |
| k |
1.000 |
| δ90 |
10.000 |
| Parameter |
Symbol |
Range |
Description |
| Absolute magnitude at 1 AU from Sun and Earth |
H0 |
-5 to 20 |
Intrinsic brightness of the comet |
| Photometric slope parameter |
n |
2 to 6 |
Rate of brightness change with heliocentric distance |
| Forward scattering asymmetry factor |
gf |
0.8 to 1 |
Degree of forward scattering |
| Backward scattering asymmetry factor |
gb |
-1 to -0.5 |
Degree of backward scattering |
| Partitioning coefficient |
k |
0.8 to 1 |
Ratio between forward/backward scattering contributions |
| Dust-to-gas brightness ratio |
δ90 |
1 to 10 |
Relative contribution of dust scattering to gas emission |
Reference: EPSC-DPS2025-160
Residuals (Piecewise)
$$\epsilon = a \log_{10} r_{\mathrm{au}} + b$$
| Start (UTC) |
End (UTC) |
a |
b |
| 2002-11-06 |
2003-01-09 |
+8.2413 |
-1.967 |
| 2003-01-09 |
2003-02-16 |
-4.0417 |
-0.415 |
| 2003-02-18 |
2003-03-14 |
-5.0184 |
-2.415 |
| 2003-03-14 |
2003-10-22 |
+0.7169 |
-2.971 |
log10 r = log10(heliocentric distance / AU), Δ = geocentric distance (AU)
Ephemeris
| Date/Time (UTC) |
RA (J2000) |
Dec (J2000) |
Nearest HIP |
Dist from HIP (arcmin) |
| 2026-09-20 00:00 |
04:18:33.44 |
-12:08:38.4 |
HIP 20115 |
24.66 |
| 2026-09-20 12:00 |
04:18:32.48 |
-12:09:00.0 |
HIP 20212 |
24.83 |
| 2026-09-21 00:00 |
04:18:31.49 |
-12:09:21.5 |
HIP 20212 |
24.81 |
| 2026-09-21 12:00 |
04:18:30.49 |
-12:09:43.1 |
HIP 20212 |
24.80 |
| 2026-09-22 00:00 |
04:18:29.47 |
-12:10:04.6 |
HIP 20212 |
24.80 |
| 2026-09-22 12:00 |
04:18:28.42 |
-12:10:26.0 |
HIP 20212 |
24.81 |
| 2026-09-23 00:00 |
04:18:27.36 |
-12:10:47.5 |
HIP 20212 |
24.84 |
| 2026-09-23 12:00 |
04:18:26.27 |
-12:11:08.9 |
HIP 20212 |
24.88 |
| 2026-09-24 00:00 |
04:18:25.16 |
-12:11:30.3 |
HIP 20212 |
24.93 |
| 2026-09-24 12:00 |
04:18:24.04 |
-12:11:51.7 |
HIP 20212 |
25.00 |
| 2026-09-25 00:00 |
04:18:22.89 |
-12:12:13.0 |
HIP 20212 |
25.07 |
| 2026-09-25 12:00 |
04:18:21.72 |
-12:12:34.3 |
HIP 20212 |
25.16 |
| 2026-09-26 00:00 |
04:18:20.53 |
-12:12:55.6 |
HIP 20212 |
25.27 |
| 2026-09-26 12:00 |
04:18:19.32 |
-12:13:16.8 |
HIP 20212 |
25.38 |
| 2026-09-27 00:00 |
04:18:18.09 |
-12:13:38.0 |
HIP 20212 |
25.51 |
| 2026-09-27 12:00 |
04:18:16.85 |
-12:13:59.2 |
HIP 20212 |
25.65 |
| 2026-09-28 00:00 |
04:18:15.58 |
-12:14:20.3 |
HIP 20212 |
25.80 |
| 2026-09-28 12:00 |
04:18:14.29 |
-12:14:41.4 |
HIP 20212 |
25.97 |
| 2026-09-29 00:00 |
04:18:12.98 |
-12:15:02.5 |
HIP 20212 |
26.14 |
| 2026-09-29 12:00 |
04:18:11.65 |
-12:15:23.5 |
HIP 20212 |
26.33 |
| 2026-09-30 00:00 |
04:18:10.30 |
-12:15:44.4 |
HIP 20212 |
26.53 |
| 2026-09-30 12:00 |
04:18:08.93 |
-12:16:05.3 |
HIP 20212 |
26.75 |
| 2026-10-01 00:00 |
04:18:07.54 |
-12:16:26.2 |
HIP 19948 |
26.97 |
| 2026-10-01 12:00 |
04:18:06.14 |
-12:16:47.0 |
HIP 19948 |
26.48 |
| 2026-10-02 00:00 |
04:18:04.71 |
-12:17:07.7 |
HIP 19948 |
26.00 |
| 2026-10-02 12:00 |
04:18:03.26 |
-12:17:28.4 |
HIP 19948 |
25.50 |
| 2026-10-03 00:00 |
04:18:01.80 |
-12:17:49.1 |
HIP 19948 |
25.01 |
| 2026-10-03 12:00 |
04:18:00.31 |
-12:18:09.7 |
HIP 19948 |
24.51 |
| 2026-10-04 00:00 |
04:17:58.81 |
-12:18:30.2 |
HIP 19948 |
24.01 |
| 2026-10-04 12:00 |
04:17:57.28 |
-12:18:50.7 |
HIP 19948 |
23.51 |
| 2026-10-05 00:00 |
04:17:55.74 |
-12:19:11.1 |
HIP 19948 |
23.00 |
| 2026-10-05 12:00 |
04:17:54.18 |
-12:19:31.4 |
HIP 19948 |
22.49 |
| 2026-10-06 00:00 |
04:17:52.60 |
-12:19:51.7 |
HIP 19948 |
21.98 |
| 2026-10-06 12:00 |
04:17:51.00 |
-12:20:11.9 |
HIP 19948 |
21.47 |
| 2026-10-07 00:00 |
04:17:49.39 |
-12:20:32.0 |
HIP 19948 |
20.95 |
| 2026-10-07 12:00 |
04:17:47.75 |
-12:20:52.1 |
HIP 19948 |
20.43 |
| 2026-10-08 00:00 |
04:17:46.10 |
-12:21:12.1 |
HIP 19948 |
19.90 |
| 2026-10-08 12:00 |
04:17:44.42 |
-12:21:32.0 |
HIP 19948 |
19.38 |
| 2026-10-09 00:00 |
04:17:42.73 |
-12:21:51.9 |
HIP 19948 |
18.85 |
| 2026-10-09 12:00 |
04:17:41.02 |
-12:22:11.6 |
HIP 19948 |
18.32 |
| 2026-10-10 00:00 |
04:17:39.30 |
-12:22:31.3 |
HIP 19948 |
17.78 |
| 2026-10-10 12:00 |
04:17:37.55 |
-12:22:50.9 |
HIP 19948 |
17.25 |
| 2026-10-11 00:00 |
04:17:35.79 |
-12:23:10.4 |
HIP 19948 |
16.71 |