| Parameter |
Value |
| Designation |
101P/Chernykh |
| Type |
P |
| Perihelion (tp_cal, UTC) |
2020-01-07T18:38:07.975680Z |
| Orbit solution date (soln_date, UTC) |
2024-08-26T10:57:16Z |
| Obs used |
1211 |
| NEO |
- |
| M1 |
13.700 |
| K1 |
4.500 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2014-10-13.0000000 |
| e |
0.59774254 |
| q (au) |
2.325778 |
| a (au) |
5.781815 |
| i (deg) |
5.033943 |
| Ω (om, deg) |
116.589097 |
| ω (w, deg) |
277.434541 |
| M (ma, deg) |
224.396168 |
Magnitude
Scatter + Global Linear
$$
M_a = (12.453 + 2.000\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
12.453 |
| n |
2.000 |
| gf |
1.000 |
| gb |
-0.997 |
| 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 |
| 2019-07-04 |
2020-01-07 |
+34.8196 |
-13.263 |
| 2020-01-08 |
2021-01-03 |
+3.7173 |
-2.221 |
| 2021-01-03 |
2022-03-01 |
+4.6114 |
-3.220 |
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) |
| 2026-05-12 00:00 |
13:43:59.26 |
-04:45:24.1 |
HIP 67092 |
18.41 |
| 2026-05-12 12:00 |
13:43:49.85 |
-04:44:39.2 |
HIP 67092 |
20.25 |
| 2026-05-13 00:00 |
13:43:40.51 |
-04:43:54.8 |
HIP 67092 |
22.20 |
| 2026-05-13 12:00 |
13:43:31.21 |
-04:43:10.8 |
HIP 67092 |
24.23 |
| 2026-05-14 00:00 |
13:43:21.97 |
-04:42:27.4 |
HIP 66966 |
26.07 |
| 2026-05-14 12:00 |
13:43:12.79 |
-04:41:44.4 |
HIP 66966 |
25.65 |
| 2026-05-15 00:00 |
13:43:03.67 |
-04:41:01.8 |
HIP 66966 |
25.45 |
| 2026-05-15 12:00 |
13:42:54.60 |
-04:40:19.8 |
HIP 66966 |
25.47 |
| 2026-05-16 00:00 |
13:42:45.59 |
-04:39:38.2 |
HIP 66966 |
25.72 |
| 2026-05-16 12:00 |
13:42:36.65 |
-04:38:57.2 |
HIP 66966 |
26.17 |
| 2026-05-17 00:00 |
13:42:27.76 |
-04:38:16.6 |
HIP 66966 |
26.82 |
| 2026-05-17 12:00 |
13:42:18.94 |
-04:37:36.6 |
HIP 66966 |
27.64 |
| 2026-05-18 00:00 |
13:42:10.18 |
-04:36:57.0 |
HIP 66966 |
28.62 |
| 2026-05-18 12:00 |
13:42:01.48 |
-04:36:18.0 |
HIP 66966 |
29.74 |
| 2026-05-19 00:00 |
13:41:52.85 |
-04:35:39.5 |
HIP 66966 |
30.97 |
| 2026-05-19 12:00 |
13:41:44.29 |
-04:35:01.5 |
HIP 66966 |
32.30 |
| 2026-05-20 00:00 |
13:41:35.80 |
-04:34:24.0 |
HIP 66675 |
31.98 |
| 2026-05-20 12:00 |
13:41:27.37 |
-04:33:47.0 |
HIP 66675 |
30.10 |
| 2026-05-21 00:00 |
13:41:19.01 |
-04:33:10.6 |
HIP 66675 |
28.29 |
| 2026-05-21 12:00 |
13:41:10.72 |
-04:32:34.8 |
HIP 66675 |
26.55 |
| 2026-05-22 00:00 |
13:41:02.50 |
-04:31:59.4 |
HIP 66675 |
24.89 |
| 2026-05-22 12:00 |
13:40:54.36 |
-04:31:24.6 |
HIP 66675 |
23.33 |
| 2026-05-23 00:00 |
13:40:46.28 |
-04:30:50.4 |
HIP 66675 |
21.87 |
| 2026-05-23 12:00 |
13:40:38.28 |
-04:30:16.7 |
HIP 66675 |
20.54 |
| 2026-05-24 00:00 |
13:40:30.35 |
-04:29:43.6 |
HIP 66675 |
19.36 |
| 2026-05-24 12:00 |
13:40:22.50 |
-04:29:11.0 |
HIP 66675 |
18.34 |
| 2026-05-25 00:00 |
13:40:14.72 |
-04:28:38.9 |
HIP 66675 |
17.51 |
| 2026-05-25 12:00 |
13:40:07.02 |
-04:28:07.4 |
HIP 66675 |
16.89 |
| 2026-05-26 00:00 |
13:39:59.39 |
-04:27:36.5 |
HIP 66675 |
16.49 |
| 2026-05-26 12:00 |
13:39:51.85 |
-04:27:06.2 |
HIP 66675 |
16.33 |
| 2026-05-27 00:00 |
13:39:44.37 |
-04:26:36.4 |
HIP 66675 |
16.40 |
| 2026-05-27 12:00 |
13:39:36.98 |
-04:26:07.2 |
HIP 66675 |
16.70 |
| 2026-05-28 00:00 |
13:39:29.67 |
-04:25:38.5 |
HIP 66675 |
17.20 |
| 2026-05-28 12:00 |
13:39:22.43 |
-04:25:10.4 |
HIP 66675 |
17.88 |
| 2026-05-29 00:00 |
13:39:15.28 |
-04:24:42.9 |
HIP 66675 |
18.71 |
| 2026-05-29 12:00 |
13:39:08.21 |
-04:24:16.0 |
HIP 66675 |
19.68 |
| 2026-05-30 00:00 |
13:39:01.22 |
-04:23:49.7 |
HIP 66675 |
20.75 |
| 2026-05-30 12:00 |
13:38:54.31 |
-04:23:23.9 |
HIP 66675 |
21.90 |
| 2026-05-31 00:00 |
13:38:47.48 |
-04:22:58.7 |
HIP 66675 |
23.12 |
| 2026-05-31 12:00 |
13:38:40.74 |
-04:22:34.1 |
HIP 66675 |
24.39 |
| 2026-06-01 00:00 |
13:38:34.08 |
-04:22:10.1 |
HIP 66675 |
25.70 |
| 2026-06-01 12:00 |
13:38:27.50 |
-04:21:46.7 |
HIP 66675 |
27.03 |
| 2026-06-02 00:00 |
13:38:21.01 |
-04:21:23.9 |
HIP 66675 |
28.39 |