| Parameter |
Value |
| Designation |
217P/LINEAR |
| Type |
P |
| Perihelion (tp_cal, UTC) |
2009-09-08T16:04:53.149440Z |
| Orbit solution date (soln_date, UTC) |
2026-03-31T13:33:22Z |
| Obs used |
3339 |
| NEO |
Yes |
| M1 |
14.500 |
| K1 |
4.750 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2012-12-22.0000000 |
| e |
0.68884715 |
| q (au) |
1.228911 |
| a (au) |
3.949540 |
| i (deg) |
12.861819 |
| Ω (om, deg) |
125.539247 |
| ω (w, deg) |
246.939807 |
| M (ma, deg) |
150.724894 |
Magnitude
Scatter + Global Linear
$$
M_a = (9.170 + 6.000\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
9.170 |
| n |
6.000 |
| gf |
0.987 |
| gb |
-0.500 |
| k |
1.000 |
| δ90 |
9.996 |
| 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 |
| 2024-05-01 |
2025-11-02 |
+4.3332 |
-1.059 |
| 2025-11-02 |
2025-12-19 |
+3.0862 |
-0.542 |
| 2025-12-19 |
2026-02-14 |
-38.2612 |
+17.064 |
| 2026-02-14 |
2026-03-21 |
+21.2517 |
-12.231 |
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) |
| 2026-03-26 00:00 |
08:08:54.76 |
+22:54:03.8 |
HIP 39788 |
16.37 |
| 2026-03-26 12:00 |
08:08:59.26 |
+22:54:26.2 |
HIP 39788 |
17.46 |
| 2026-03-27 00:00 |
08:09:04.07 |
+22:54:47.2 |
HIP 39788 |
18.61 |
| 2026-03-27 12:00 |
08:09:09.19 |
+22:55:06.9 |
HIP 39788 |
19.82 |
| 2026-03-28 00:00 |
08:09:14.62 |
+22:55:25.4 |
HIP 39788 |
21.09 |
| 2026-03-28 12:00 |
08:09:20.35 |
+22:55:42.5 |
HIP 39788 |
22.42 |
| 2026-03-29 00:00 |
08:09:26.38 |
+22:55:58.5 |
HIP 39788 |
23.80 |
| 2026-03-29 12:00 |
08:09:32.71 |
+22:56:13.1 |
HIP 39788 |
25.24 |
| 2026-03-30 00:00 |
08:09:39.33 |
+22:56:26.5 |
HIP 39788 |
26.75 |
| 2026-03-30 12:00 |
08:09:46.25 |
+22:56:38.7 |
HIP 39788 |
28.31 |
| 2026-03-31 00:00 |
08:09:53.45 |
+22:56:49.7 |
HIP 39788 |
29.94 |
| 2026-03-31 12:00 |
08:10:00.95 |
+22:56:59.5 |
HIP 39788 |
31.62 |
| 2026-04-01 00:00 |
08:10:08.73 |
+22:57:08.0 |
HIP 39788 |
33.37 |
| 2026-04-01 12:00 |
08:10:16.79 |
+22:57:15.4 |
HIP 39788 |
35.18 |
| 2026-04-02 00:00 |
08:10:25.14 |
+22:57:21.6 |
HIP 40102 |
34.99 |
| 2026-04-02 12:00 |
08:10:33.76 |
+22:57:26.6 |
HIP 40102 |
34.10 |
| 2026-04-03 00:00 |
08:10:42.66 |
+22:57:30.5 |
HIP 40102 |
33.31 |
| 2026-04-03 12:00 |
08:10:51.84 |
+22:57:33.2 |
HIP 40102 |
32.63 |
| 2026-04-04 00:00 |
08:11:01.28 |
+22:57:34.7 |
HIP 40102 |
32.08 |
| 2026-04-04 12:00 |
08:11:11.00 |
+22:57:35.1 |
HIP 40102 |
31.68 |
| 2026-04-05 00:00 |
08:11:20.98 |
+22:57:34.4 |
HIP 40102 |
31.44 |
| 2026-04-05 12:00 |
08:11:31.23 |
+22:57:32.6 |
HIP 40102 |
31.39 |
| 2026-04-06 00:00 |
08:11:41.74 |
+22:57:29.6 |
HIP 40293 |
29.63 |
| 2026-04-06 12:00 |
08:11:52.51 |
+22:57:25.6 |
HIP 40293 |
27.36 |
| 2026-04-07 00:00 |
08:12:03.54 |
+22:57:20.4 |
HIP 40293 |
25.09 |
| 2026-04-07 12:00 |
08:12:14.83 |
+22:57:14.1 |
HIP 40293 |
22.83 |
| 2026-04-08 00:00 |
08:12:26.37 |
+22:57:06.8 |
HIP 40293 |
20.61 |
| 2026-04-08 12:00 |
08:12:38.16 |
+22:56:58.4 |
HIP 40293 |
18.47 |
| 2026-04-09 00:00 |
08:12:50.20 |
+22:56:48.9 |
HIP 40293 |
16.48 |
| 2026-04-09 12:00 |
08:13:02.49 |
+22:56:38.3 |
HIP 40293 |
14.72 |
| 2026-04-10 00:00 |
08:13:15.03 |
+22:56:26.7 |
HIP 40293 |
13.32 |
| 2026-04-10 12:00 |
08:13:27.81 |
+22:56:14.1 |
HIP 40293 |
12.45 |
| 2026-04-11 00:00 |
08:13:40.83 |
+22:56:00.4 |
HIP 40293 |
12.26 |
| 2026-04-11 12:00 |
08:13:54.09 |
+22:55:45.6 |
HIP 40293 |
12.83 |
| 2026-04-12 00:00 |
08:14:07.59 |
+22:55:29.8 |
HIP 40293 |
14.09 |
| 2026-04-12 12:00 |
08:14:21.32 |
+22:55:13.0 |
HIP 40293 |
15.92 |
| 2026-04-13 00:00 |
08:14:35.29 |
+22:54:55.2 |
HIP 40293 |
18.17 |
| 2026-04-13 12:00 |
08:14:49.49 |
+22:54:36.4 |
HIP 40293 |
20.73 |
| 2026-04-14 00:00 |
08:15:03.91 |
+22:54:16.5 |
HIP 40529 |
20.36 |
| 2026-04-14 12:00 |
08:15:18.57 |
+22:53:55.7 |
HIP 40529 |
17.06 |
| 2026-04-15 00:00 |
08:15:33.45 |
+22:53:33.9 |
HIP 40529 |
13.75 |
| 2026-04-15 12:00 |
08:15:48.55 |
+22:53:11.0 |
HIP 40529 |
10.48 |
| 2026-04-16 00:00 |
08:16:03.88 |
+22:52:47.2 |
HIP 40529 |
7.40 |