| Parameter |
Value |
| Designation |
40P/Vaisala 1 |
| Type |
P |
| Perihelion (tp_cal, UTC) |
2014-11-17T19:36:24.168960Z |
| Orbit solution date (soln_date, UTC) |
2026-07-17T07:41:43Z |
| Obs used |
1268 |
| NEO |
- |
| M1 |
11.500 |
| K1 |
13.500 |
| PC |
0.030 |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2011-08-15.0000000 |
| e |
0.63250898 |
| q (au) |
1.802114 |
| a (au) |
4.903831 |
| i (deg) |
11.500129 |
| Ω (om, deg) |
134.484162 |
| ω (w, deg) |
47.307718 |
| M (ma, deg) |
251.919874 |
Magnitude
Scatter + Global Linear
$$
M_a = (9.768 + 6.000\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
9.768 |
| n |
6.000 |
| gf |
0.800 |
| gb |
-0.604 |
| 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 |
| 2024-11-29 |
2026-02-13 |
+2.9361 |
-1.469 |
| 2026-02-13 |
2026-04-06 |
+21.0703 |
-6.799 |
| 2026-04-06 |
2026-07-20 |
-3.3238 |
+1.714 |
log10 r = log10(heliocentric distance / AU), Δ = geocentric distance (AU)
Finding Chart
Ephemeris
| Date/Time (UTC) |
RA (J2000) |
Dec (J2000) |
Nearest HIP |
Dist from HIP (arcmin) |
| 2026-09-20 00:00 |
17:33:42.49 |
-17:40:12.4 |
HIP 85952 |
10.71 |
| 2026-09-20 12:00 |
17:34:07.75 |
-17:42:04.1 |
HIP 85952 |
8.37 |
| 2026-09-21 00:00 |
17:34:33.19 |
-17:43:55.2 |
HIP 85952 |
10.27 |
| 2026-09-21 12:00 |
17:34:58.78 |
-17:45:45.5 |
HIP 85952 |
14.91 |
| 2026-09-22 00:00 |
17:35:24.54 |
-17:47:35.1 |
HIP 86142 |
12.36 |
| 2026-09-22 12:00 |
17:35:50.46 |
-17:49:23.9 |
HIP 86142 |
5.95 |
| 2026-09-23 00:00 |
17:36:16.54 |
-17:51:12.1 |
HIP 86142 |
0.98 |
| 2026-09-23 12:00 |
17:36:42.78 |
-17:52:59.4 |
HIP 86196 |
4.83 |
| 2026-09-24 00:00 |
17:37:09.18 |
-17:54:46.1 |
HIP 86196 |
4.59 |
| 2026-09-24 12:00 |
17:37:35.73 |
-17:56:32.0 |
HIP 86271 |
6.96 |
| 2026-09-25 00:00 |
17:38:02.44 |
-17:58:17.1 |
HIP 86271 |
10.29 |
| 2026-09-25 12:00 |
17:38:29.30 |
-18:00:01.5 |
HIP 86271 |
15.84 |
| 2026-09-26 00:00 |
17:38:56.31 |
-18:01:45.2 |
HIP 86271 |
22.01 |
| 2026-09-26 12:00 |
17:39:23.47 |
-18:03:28.1 |
HIP 86402 |
21.26 |
| 2026-09-27 00:00 |
17:39:50.78 |
-18:05:10.2 |
HIP 86402 |
21.01 |
| 2026-09-27 12:00 |
17:40:18.23 |
-18:06:51.6 |
HIP 86402 |
22.85 |
| 2026-09-28 00:00 |
17:40:45.83 |
-18:08:32.2 |
HIP 86605 |
21.48 |
| 2026-09-28 12:00 |
17:41:13.58 |
-18:10:12.1 |
HIP 86605 |
18.72 |
| 2026-09-29 00:00 |
17:41:41.47 |
-18:11:51.2 |
HIP 86605 |
18.20 |
| 2026-09-29 12:00 |
17:42:09.50 |
-18:13:29.5 |
HIP 86605 |
20.14 |
| 2026-09-30 00:00 |
17:42:37.67 |
-18:15:07.1 |
HIP 86605 |
23.96 |
| 2026-09-30 12:00 |
17:43:05.98 |
-18:16:43.9 |
HIP 86605 |
28.95 |
| 2026-10-01 00:00 |
17:43:34.43 |
-18:18:19.9 |
HIP 86873 |
28.70 |
| 2026-10-01 12:00 |
17:44:03.02 |
-18:19:55.2 |
HIP 86873 |
23.27 |
| 2026-10-02 00:00 |
17:44:31.74 |
-18:21:29.7 |
HIP 86873 |
18.88 |
| 2026-10-02 12:00 |
17:45:00.60 |
-18:23:03.4 |
HIP 86873 |
16.41 |
| 2026-10-03 00:00 |
17:45:29.59 |
-18:24:36.3 |
HIP 86873 |
16.78 |
| 2026-10-03 12:00 |
17:45:58.71 |
-18:26:08.5 |
HIP 86873 |
19.86 |
| 2026-10-04 00:00 |
17:46:27.97 |
-18:27:39.8 |
HIP 86873 |
24.67 |
| 2026-10-04 12:00 |
17:46:57.36 |
-18:29:10.4 |
HIP 87129 |
20.17 |
| 2026-10-05 00:00 |
17:47:26.88 |
-18:30:40.2 |
HIP 87129 |
16.22 |
| 2026-10-05 12:00 |
17:47:56.52 |
-18:32:09.2 |
HIP 87129 |
14.87 |
| 2026-10-06 00:00 |
17:48:26.29 |
-18:33:37.4 |
HIP 87129 |
16.81 |
| 2026-10-06 12:00 |
17:48:56.19 |
-18:35:04.8 |
HIP 87176 |
19.15 |
| 2026-10-07 00:00 |
17:49:26.22 |
-18:36:31.5 |
HIP 87176 |
20.60 |
| 2026-10-07 12:00 |
17:49:56.37 |
-18:37:57.3 |
HIP 87176 |
24.27 |
| 2026-10-08 00:00 |
17:50:26.64 |
-18:39:22.3 |
HIP 87388 |
24.73 |
| 2026-10-08 12:00 |
17:50:57.03 |
-18:40:46.5 |
HIP 87388 |
20.05 |
| 2026-10-09 00:00 |
17:51:27.55 |
-18:42:09.9 |
HIP 87388 |
17.32 |
| 2026-10-09 12:00 |
17:51:58.18 |
-18:43:32.5 |
HIP 87388 |
17.52 |
| 2026-10-10 00:00 |
17:52:28.93 |
-18:44:54.3 |
HIP 87568 |
14.69 |
| 2026-10-10 12:00 |
17:52:59.80 |
-18:46:15.2 |
HIP 87568 |
8.19 |
| 2026-10-11 00:00 |
17:53:30.78 |
-18:47:35.4 |
HIP 87568 |
5.40 |