| Parameter |
Value |
| Designation |
C/1989 W1 (Aarseth-Brewington) |
| Type |
C |
| Perihelion (tp_cal, UTC) |
1989-12-27T21:19:34.193280Z |
| Orbit solution date (soln_date, UTC) |
2021-04-15T23:29:38Z |
| Obs used |
73 |
| NEO |
- |
| M1 |
8.200 |
| K1 |
13.000 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
1989-12-05.0000000 |
| e |
1.00006499 |
| q (au) |
0.300689 |
| a (au) |
-4626.812393 |
| i (deg) |
88.386281 |
| Ω (om, deg) |
345.916879 |
| ω (w, deg) |
205.258893 |
| M (ma, deg) |
-0.000072 |
Magnitude
Scatter + Global Linear
$$
M_a = (7.015 + 3.263\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
7.015 |
| n |
3.263 |
| 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 |
| 1989-09-01 |
1989-11-19 |
+12.2046 |
-0.330 |
| 1989-11-19 |
1989-12-04 |
-0.1288 |
-0.034 |
| 1989-12-04 |
1989-12-27 |
-1.0628 |
-0.451 |
| 1989-12-28 |
1990-01-31 |
+0.3042 |
+0.326 |
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 |
22:42:06.83 |
+10:41:44.7 |
HIP 112056 |
11.59 |
| 2026-09-20 12:00 |
22:42:05.10 |
+10:41:32.3 |
HIP 112056 |
11.23 |
| 2026-09-21 00:00 |
22:42:03.38 |
+10:41:19.8 |
HIP 112056 |
10.89 |
| 2026-09-21 12:00 |
22:42:01.66 |
+10:41:07.2 |
HIP 112056 |
10.55 |
| 2026-09-22 00:00 |
22:41:59.94 |
+10:40:54.7 |
HIP 112056 |
10.22 |
| 2026-09-22 12:00 |
22:41:58.23 |
+10:40:42.0 |
HIP 112056 |
9.91 |
| 2026-09-23 00:00 |
22:41:56.53 |
+10:40:29.3 |
HIP 112056 |
9.61 |
| 2026-09-23 12:00 |
22:41:54.83 |
+10:40:16.6 |
HIP 112056 |
9.32 |
| 2026-09-24 00:00 |
22:41:53.14 |
+10:40:03.9 |
HIP 112056 |
9.04 |
| 2026-09-24 12:00 |
22:41:51.45 |
+10:39:51.1 |
HIP 112056 |
8.78 |
| 2026-09-25 00:00 |
22:41:49.77 |
+10:39:38.2 |
HIP 112056 |
8.54 |
| 2026-09-25 12:00 |
22:41:48.09 |
+10:39:25.3 |
HIP 112056 |
8.32 |
| 2026-09-26 00:00 |
22:41:46.43 |
+10:39:12.4 |
HIP 112056 |
8.12 |
| 2026-09-26 12:00 |
22:41:44.77 |
+10:38:59.5 |
HIP 112056 |
7.93 |
| 2026-09-27 00:00 |
22:41:43.11 |
+10:38:46.5 |
HIP 112056 |
7.77 |
| 2026-09-27 12:00 |
22:41:41.46 |
+10:38:33.5 |
HIP 112056 |
7.64 |
| 2026-09-28 00:00 |
22:41:39.82 |
+10:38:20.4 |
HIP 112056 |
7.52 |
| 2026-09-28 12:00 |
22:41:38.19 |
+10:38:07.3 |
HIP 112056 |
7.44 |
| 2026-09-29 00:00 |
22:41:36.56 |
+10:37:54.2 |
HIP 112056 |
7.38 |
| 2026-09-29 12:00 |
22:41:34.94 |
+10:37:41.0 |
HIP 112056 |
7.34 |
| 2026-09-30 00:00 |
22:41:33.33 |
+10:37:27.8 |
HIP 112056 |
7.33 |
| 2026-09-30 12:00 |
22:41:31.73 |
+10:37:14.6 |
HIP 112056 |
7.35 |
| 2026-10-01 00:00 |
22:41:30.13 |
+10:37:01.4 |
HIP 112056 |
7.40 |
| 2026-10-01 12:00 |
22:41:28.54 |
+10:36:48.1 |
HIP 112056 |
7.47 |
| 2026-10-02 00:00 |
22:41:26.96 |
+10:36:34.8 |
HIP 112056 |
7.56 |
| 2026-10-02 12:00 |
22:41:25.39 |
+10:36:21.5 |
HIP 112056 |
7.68 |
| 2026-10-03 00:00 |
22:41:23.82 |
+10:36:08.1 |
HIP 112056 |
7.82 |
| 2026-10-03 12:00 |
22:41:22.26 |
+10:35:54.8 |
HIP 112056 |
7.98 |
| 2026-10-04 00:00 |
22:41:20.71 |
+10:35:41.4 |
HIP 112056 |
8.16 |
| 2026-10-04 12:00 |
22:41:19.17 |
+10:35:28.0 |
HIP 112056 |
8.36 |
| 2026-10-05 00:00 |
22:41:17.64 |
+10:35:14.5 |
HIP 112056 |
8.57 |
| 2026-10-05 12:00 |
22:41:16.12 |
+10:35:01.1 |
HIP 112056 |
8.80 |
| 2026-10-06 00:00 |
22:41:14.61 |
+10:34:47.6 |
HIP 112056 |
9.04 |
| 2026-10-06 12:00 |
22:41:13.10 |
+10:34:34.1 |
HIP 112056 |
9.30 |
| 2026-10-07 00:00 |
22:41:11.60 |
+10:34:20.6 |
HIP 112056 |
9.56 |
| 2026-10-07 12:00 |
22:41:10.12 |
+10:34:07.1 |
HIP 112056 |
9.83 |
| 2026-10-08 00:00 |
22:41:08.64 |
+10:33:53.5 |
HIP 112056 |
10.11 |
| 2026-10-08 12:00 |
22:41:07.17 |
+10:33:40.0 |
HIP 112056 |
10.40 |
| 2026-10-09 00:00 |
22:41:05.71 |
+10:33:26.4 |
HIP 112056 |
10.70 |
| 2026-10-09 12:00 |
22:41:04.26 |
+10:33:12.9 |
HIP 112056 |
11.00 |
| 2026-10-10 00:00 |
22:41:02.83 |
+10:32:59.3 |
HIP 112056 |
11.31 |
| 2026-10-10 12:00 |
22:41:01.40 |
+10:32:45.7 |
HIP 112056 |
11.62 |
| 2026-10-11 00:00 |
22:40:59.98 |
+10:32:32.1 |
HIP 112056 |
11.94 |