| 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) |
| 2026-07-29 00:00 |
17:10:20.80 |
-13:29:35.2 |
HIP 84023 |
13.68 |
| 2026-07-29 12:00 |
17:10:19.26 |
-13:32:15.1 |
HIP 84023 |
11.20 |
| 2026-07-30 00:00 |
17:10:18.05 |
-13:34:54.9 |
HIP 84023 |
8.80 |
| 2026-07-30 12:00 |
17:10:17.16 |
-13:37:34.7 |
HIP 84023 |
6.58 |
| 2026-07-31 00:00 |
17:10:16.60 |
-13:40:14.4 |
HIP 84023 |
4.77 |
| 2026-07-31 12:00 |
17:10:16.36 |
-13:42:54.0 |
HIP 84023 |
3.98 |
| 2026-08-01 00:00 |
17:10:16.45 |
-13:45:33.4 |
HIP 84023 |
4.74 |
| 2026-08-01 12:00 |
17:10:16.86 |
-13:48:12.8 |
HIP 83997 |
3.53 |
| 2026-08-02 00:00 |
17:10:17.59 |
-13:50:52.1 |
HIP 83997 |
1.28 |
| 2026-08-02 12:00 |
17:10:18.64 |
-13:53:31.2 |
HIP 83997 |
2.27 |
| 2026-08-03 00:00 |
17:10:20.01 |
-13:56:10.2 |
HIP 83997 |
4.80 |
| 2026-08-03 12:00 |
17:10:21.69 |
-13:58:49.0 |
HIP 83997 |
7.45 |
| 2026-08-04 00:00 |
17:10:23.70 |
-14:01:27.7 |
HIP 83997 |
10.13 |
| 2026-08-04 12:00 |
17:10:26.02 |
-14:04:06.2 |
HIP 83997 |
12.83 |
| 2026-08-05 00:00 |
17:10:28.66 |
-14:06:44.5 |
HIP 83997 |
15.54 |
| 2026-08-05 12:00 |
17:10:31.61 |
-14:09:22.7 |
HIP 83997 |
18.27 |
| 2026-08-06 00:00 |
17:10:34.87 |
-14:12:00.6 |
HIP 83997 |
21.02 |
| 2026-08-06 12:00 |
17:10:38.45 |
-14:14:38.4 |
HIP 83997 |
23.78 |
| 2026-08-07 00:00 |
17:10:42.34 |
-14:17:15.9 |
HIP 83997 |
26.56 |
| 2026-08-07 12:00 |
17:10:46.53 |
-14:19:53.3 |
HIP 84132 |
24.60 |
| 2026-08-08 00:00 |
17:10:51.04 |
-14:22:30.4 |
HIP 84132 |
22.00 |
| 2026-08-08 12:00 |
17:10:55.85 |
-14:25:07.2 |
HIP 84132 |
19.42 |
| 2026-08-09 00:00 |
17:11:00.97 |
-14:27:43.9 |
HIP 84132 |
16.87 |
| 2026-08-09 12:00 |
17:11:06.40 |
-14:30:20.2 |
HIP 84132 |
14.39 |
| 2026-08-10 00:00 |
17:11:12.13 |
-14:32:56.4 |
HIP 84132 |
12.04 |
| 2026-08-10 12:00 |
17:11:18.17 |
-14:35:32.2 |
HIP 84132 |
9.94 |
| 2026-08-11 00:00 |
17:11:24.50 |
-14:38:07.8 |
HIP 84132 |
8.31 |
| 2026-08-11 12:00 |
17:11:31.14 |
-14:40:43.0 |
HIP 84132 |
7.52 |
| 2026-08-12 00:00 |
17:11:38.08 |
-14:43:18.0 |
HIP 84132 |
7.86 |
| 2026-08-12 12:00 |
17:11:45.32 |
-14:45:52.7 |
HIP 84132 |
9.24 |
| 2026-08-13 00:00 |
17:11:52.85 |
-14:48:27.1 |
HIP 84132 |
11.32 |
| 2026-08-13 12:00 |
17:12:00.68 |
-14:51:01.1 |
HIP 84132 |
13.81 |
| 2026-08-14 00:00 |
17:12:08.80 |
-14:53:34.8 |
HIP 84132 |
16.55 |
| 2026-08-14 12:00 |
17:12:17.22 |
-14:56:08.2 |
HIP 84190 |
14.34 |
| 2026-08-15 00:00 |
17:12:25.92 |
-14:58:41.2 |
HIP 84190 |
11.34 |
| 2026-08-15 12:00 |
17:12:34.92 |
-15:01:13.8 |
HIP 84190 |
8.58 |
| 2026-08-16 00:00 |
17:12:44.20 |
-15:03:46.1 |
HIP 84190 |
6.44 |
| 2026-08-16 12:00 |
17:12:53.77 |
-15:06:18.0 |
HIP 84190 |
5.72 |
| 2026-08-17 00:00 |
17:13:03.63 |
-15:08:49.6 |
HIP 84190 |
6.97 |
| 2026-08-17 12:00 |
17:13:13.76 |
-15:11:20.7 |
HIP 84190 |
9.47 |
| 2026-08-18 00:00 |
17:13:24.18 |
-15:13:51.5 |
HIP 84190 |
12.53 |
| 2026-08-18 12:00 |
17:13:34.87 |
-15:16:21.8 |
HIP 84190 |
15.85 |
| 2026-08-19 00:00 |
17:13:45.84 |
-15:18:51.7 |
HIP 84269 |
14.92 |