| Parameter |
Value |
| Designation |
153P/Ikeya-Zhang |
| Type |
P |
| Perihelion (tp_cal, UTC) |
2002-03-18T23:31:25.772160Z |
| Orbit solution date (soln_date, UTC) |
2020-06-17T10:40:41Z |
| Obs used |
1893 |
| NEO |
- |
| M1 |
4.000 |
| K1 |
15.000 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2002-05-08.0000000 |
| e |
0.99008066 |
| q (au) |
0.507070 |
| a (au) |
51.119322 |
| i (deg) |
28.120957 |
| Ω (om, deg) |
93.369457 |
| ω (w, deg) |
34.668179 |
| M (ma, deg) |
0.134887 |
Magnitude
Scatter + Global Linear
$$
M_a = (6.663 + 3.285\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
6.663 |
| n |
3.285 |
| gf |
0.800 |
| gb |
-0.500 |
| k |
0.926 |
| 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 |
| 2001-08-25 |
2002-02-03 |
+7.8285 |
+1.084 |
| 2002-02-03 |
2002-03-18 |
+3.0730 |
+0.799 |
| 2002-03-19 |
2002-06-13 |
+0.2070 |
+0.282 |
| 2002-06-13 |
2002-10-11 |
+6.0428 |
-0.737 |
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 |
19:55:55.14 |
-32:38:36.8 |
HIP 98012 |
26.35 |
| 2026-09-20 12:00 |
19:55:53.63 |
-32:38:33.3 |
HIP 98012 |
26.28 |
| 2026-09-21 00:00 |
19:55:52.15 |
-32:38:29.7 |
HIP 98012 |
26.21 |
| 2026-09-21 12:00 |
19:55:50.70 |
-32:38:25.9 |
HIP 98012 |
26.16 |
| 2026-09-22 00:00 |
19:55:49.27 |
-32:38:22.1 |
HIP 98012 |
26.11 |
| 2026-09-22 12:00 |
19:55:47.86 |
-32:38:18.3 |
HIP 98012 |
26.07 |
| 2026-09-23 00:00 |
19:55:46.48 |
-32:38:14.3 |
HIP 98012 |
26.03 |
| 2026-09-23 12:00 |
19:55:45.13 |
-32:38:10.2 |
HIP 98012 |
26.00 |
| 2026-09-24 00:00 |
19:55:43.80 |
-32:38:06.0 |
HIP 98012 |
25.98 |
| 2026-09-24 12:00 |
19:55:42.50 |
-32:38:01.7 |
HIP 98012 |
25.96 |
| 2026-09-25 00:00 |
19:55:41.22 |
-32:37:57.4 |
HIP 97896 |
25.79 |
| 2026-09-25 12:00 |
19:55:39.97 |
-32:37:52.9 |
HIP 97896 |
25.53 |
| 2026-09-26 00:00 |
19:55:38.75 |
-32:37:48.4 |
HIP 97896 |
25.28 |
| 2026-09-26 12:00 |
19:55:37.55 |
-32:37:43.8 |
HIP 97896 |
25.03 |
| 2026-09-27 00:00 |
19:55:36.38 |
-32:37:39.0 |
HIP 97896 |
24.79 |
| 2026-09-27 12:00 |
19:55:35.23 |
-32:37:34.2 |
HIP 97896 |
24.56 |
| 2026-09-28 00:00 |
19:55:34.11 |
-32:37:29.3 |
HIP 97896 |
24.33 |
| 2026-09-28 12:00 |
19:55:33.02 |
-32:37:24.3 |
HIP 97896 |
24.11 |
| 2026-09-29 00:00 |
19:55:31.95 |
-32:37:19.3 |
HIP 97896 |
23.89 |
| 2026-09-29 12:00 |
19:55:30.91 |
-32:37:14.1 |
HIP 97896 |
23.69 |
| 2026-09-30 00:00 |
19:55:29.90 |
-32:37:08.8 |
HIP 97896 |
23.48 |
| 2026-09-30 12:00 |
19:55:28.91 |
-32:37:03.5 |
HIP 97896 |
23.29 |
| 2026-10-01 00:00 |
19:55:27.95 |
-32:36:58.1 |
HIP 97896 |
23.10 |
| 2026-10-01 12:00 |
19:55:27.01 |
-32:36:52.6 |
HIP 97896 |
22.91 |
| 2026-10-02 00:00 |
19:55:26.11 |
-32:36:47.0 |
HIP 97896 |
22.74 |
| 2026-10-02 12:00 |
19:55:25.23 |
-32:36:41.3 |
HIP 97896 |
22.56 |
| 2026-10-03 00:00 |
19:55:24.38 |
-32:36:35.5 |
HIP 97896 |
22.40 |
| 2026-10-03 12:00 |
19:55:23.55 |
-32:36:29.6 |
HIP 97896 |
22.24 |
| 2026-10-04 00:00 |
19:55:22.75 |
-32:36:23.7 |
HIP 97896 |
22.09 |
| 2026-10-04 12:00 |
19:55:21.98 |
-32:36:17.7 |
HIP 97896 |
21.95 |
| 2026-10-05 00:00 |
19:55:21.24 |
-32:36:11.6 |
HIP 97896 |
21.81 |
| 2026-10-05 12:00 |
19:55:20.52 |
-32:36:05.4 |
HIP 97896 |
21.68 |
| 2026-10-06 00:00 |
19:55:19.83 |
-32:35:59.1 |
HIP 97896 |
21.55 |
| 2026-10-06 12:00 |
19:55:19.17 |
-32:35:52.7 |
HIP 97896 |
21.43 |
| 2026-10-07 00:00 |
19:55:18.54 |
-32:35:46.3 |
HIP 97896 |
21.32 |
| 2026-10-07 12:00 |
19:55:17.93 |
-32:35:39.8 |
HIP 97896 |
21.22 |
| 2026-10-08 00:00 |
19:55:17.36 |
-32:35:33.2 |
HIP 97896 |
21.12 |
| 2026-10-08 12:00 |
19:55:16.81 |
-32:35:26.5 |
HIP 97896 |
21.03 |
| 2026-10-09 00:00 |
19:55:16.29 |
-32:35:19.7 |
HIP 97896 |
20.95 |
| 2026-10-09 12:00 |
19:55:15.79 |
-32:35:12.9 |
HIP 97896 |
20.87 |
| 2026-10-10 00:00 |
19:55:15.33 |
-32:35:06.0 |
HIP 97896 |
20.80 |
| 2026-10-10 12:00 |
19:55:14.89 |
-32:34:59.0 |
HIP 97896 |
20.73 |
| 2026-10-11 00:00 |
19:55:14.48 |
-32:34:51.9 |
HIP 97896 |
20.68 |