| Parameter |
Value |
| Designation |
C/2000 WM1 (LINEAR) |
| Type |
C |
| Perihelion (tp_cal, UTC) |
2002-01-22T16:09:23.857920Z |
| Orbit solution date (soln_date, UTC) |
2021-04-15T23:30:08Z |
| Obs used |
2130 |
| NEO |
- |
| M1 |
11.200 |
| K1 |
4.750 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2002-01-24.0000000 |
| e |
1.00024278 |
| q (au) |
0.555348 |
| a (au) |
-2287.433616 |
| i (deg) |
72.550229 |
| Ω (om, deg) |
237.895729 |
| ω (w, deg) |
276.770906 |
| M (ma, deg) |
0.000012 |
Magnitude
Scatter + Global Linear
$$
M_a = (7.292 + 4.602\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
7.292 |
| n |
4.602 |
| gf |
0.800 |
| gb |
-0.500 |
| k |
0.800 |
| δ90 |
1.000 |
| 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 |
| 2000-12-22 |
2002-01-22 |
-2.0781 |
+0.678 |
| 2002-01-22 |
2002-02-04 |
-39.9944 |
-10.010 |
| 2002-02-04 |
2002-05-18 |
+3.0549 |
-0.945 |
| 2002-05-18 |
2003-06-05 |
+0.1428 |
+0.246 |
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 |
19:06:35.94 |
+51:05:14.3 |
HIP 93943 |
13.16 |
| 2026-09-20 12:00 |
19:06:34.83 |
+51:04:40.0 |
HIP 93943 |
12.95 |
| 2026-09-21 00:00 |
19:06:33.76 |
+51:04:05.6 |
HIP 93943 |
12.77 |
| 2026-09-21 12:00 |
19:06:32.71 |
+51:03:31.2 |
HIP 93943 |
12.60 |
| 2026-09-22 00:00 |
19:06:31.70 |
+51:02:56.7 |
HIP 93943 |
12.45 |
| 2026-09-22 12:00 |
19:06:30.72 |
+51:02:22.1 |
HIP 93943 |
12.33 |
| 2026-09-23 00:00 |
19:06:29.78 |
+51:01:47.5 |
HIP 93943 |
12.23 |
| 2026-09-23 12:00 |
19:06:28.87 |
+51:01:12.8 |
HIP 93943 |
12.15 |
| 2026-09-24 00:00 |
19:06:27.99 |
+51:00:38.0 |
HIP 93943 |
12.10 |
| 2026-09-24 12:00 |
19:06:27.15 |
+51:00:03.1 |
HIP 93943 |
12.07 |
| 2026-09-25 00:00 |
19:06:26.34 |
+50:59:28.2 |
HIP 93943 |
12.06 |
| 2026-09-25 12:00 |
19:06:25.56 |
+50:58:53.3 |
HIP 93943 |
12.08 |
| 2026-09-26 00:00 |
19:06:24.81 |
+50:58:18.3 |
HIP 93943 |
12.12 |
| 2026-09-26 12:00 |
19:06:24.10 |
+50:57:43.2 |
HIP 93943 |
12.19 |
| 2026-09-27 00:00 |
19:06:23.42 |
+50:57:08.1 |
HIP 93943 |
12.28 |
| 2026-09-27 12:00 |
19:06:22.78 |
+50:56:32.9 |
HIP 93943 |
12.39 |
| 2026-09-28 00:00 |
19:06:22.17 |
+50:55:57.7 |
HIP 93943 |
12.52 |
| 2026-09-28 12:00 |
19:06:21.59 |
+50:55:22.5 |
HIP 93943 |
12.68 |
| 2026-09-29 00:00 |
19:06:21.05 |
+50:54:47.2 |
HIP 93943 |
12.85 |
| 2026-09-29 12:00 |
19:06:20.54 |
+50:54:11.8 |
HIP 93943 |
13.05 |
| 2026-09-30 00:00 |
19:06:20.06 |
+50:53:36.5 |
HIP 93943 |
13.26 |
| 2026-09-30 12:00 |
19:06:19.62 |
+50:53:01.1 |
HIP 93943 |
13.50 |
| 2026-10-01 00:00 |
19:06:19.21 |
+50:52:25.7 |
HIP 93943 |
13.75 |
| 2026-10-01 12:00 |
19:06:18.84 |
+50:51:50.2 |
HIP 93943 |
14.01 |
| 2026-10-02 00:00 |
19:06:18.49 |
+50:51:14.7 |
HIP 93943 |
14.29 |
| 2026-10-02 12:00 |
19:06:18.19 |
+50:50:39.3 |
HIP 93943 |
14.59 |
| 2026-10-03 00:00 |
19:06:17.91 |
+50:50:03.7 |
HIP 93943 |
14.89 |
| 2026-10-03 12:00 |
19:06:17.67 |
+50:49:28.2 |
HIP 93943 |
15.21 |
| 2026-10-04 00:00 |
19:06:17.47 |
+50:48:52.7 |
HIP 93943 |
15.55 |
| 2026-10-04 12:00 |
19:06:17.29 |
+50:48:17.1 |
HIP 93943 |
15.89 |
| 2026-10-05 00:00 |
19:06:17.16 |
+50:47:41.5 |
HIP 93943 |
16.24 |
| 2026-10-05 12:00 |
19:06:17.05 |
+50:47:06.0 |
HIP 93943 |
16.60 |
| 2026-10-06 00:00 |
19:06:16.98 |
+50:46:30.4 |
HIP 93943 |
16.97 |
| 2026-10-06 12:00 |
19:06:16.95 |
+50:45:54.8 |
HIP 93943 |
17.35 |
| 2026-10-07 00:00 |
19:06:16.94 |
+50:45:19.2 |
HIP 93943 |
17.74 |
| 2026-10-07 12:00 |
19:06:16.98 |
+50:44:43.7 |
HIP 93943 |
18.14 |
| 2026-10-08 00:00 |
19:06:17.04 |
+50:44:08.1 |
HIP 93943 |
18.54 |
| 2026-10-08 12:00 |
19:06:17.14 |
+50:43:32.6 |
HIP 93943 |
18.94 |
| 2026-10-09 00:00 |
19:06:17.28 |
+50:42:57.0 |
HIP 93943 |
19.36 |
| 2026-10-09 12:00 |
19:06:17.45 |
+50:42:21.5 |
HIP 93943 |
19.77 |
| 2026-10-10 00:00 |
19:06:17.65 |
+50:41:46.0 |
HIP 93943 |
20.20 |
| 2026-10-10 12:00 |
19:06:17.89 |
+50:41:10.5 |
HIP 93943 |
20.62 |
| 2026-10-11 00:00 |
19:06:18.16 |
+50:40:35.1 |
HIP 93943 |
21.06 |