| Parameter |
Value |
| Designation |
C/2014 Q1 (PANSTARRS) |
| Type |
C |
| Perihelion (tp_cal, UTC) |
2015-07-06T12:15:56.439360Z |
| Orbit solution date (soln_date, UTC) |
2021-04-15T23:32:58Z |
| Obs used |
704 |
| NEO |
- |
| M1 |
9.700 |
| K1 |
7.250 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2015-02-17.0000000 |
| e |
0.99972226 |
| q (au) |
0.314572 |
| a (au) |
1132.604359 |
| i (deg) |
43.106721 |
| Ω (om, deg) |
8.762539 |
| ω (w, deg) |
120.050113 |
| M (ma, deg) |
359.996393 |
Magnitude
Scatter + Global Linear
$$
M_a = (11.191 + 3.199\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
11.191 |
| n |
3.199 |
| gf |
0.996 |
| gb |
-0.807 |
| k |
0.944 |
| δ90 |
9.807 |
| 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 |
| 2014-08-16 |
2015-01-14 |
+6.2752 |
-4.022 |
| 2015-01-14 |
2015-06-22 |
+1.0263 |
-1.086 |
| 2015-07-06 |
2015-08-05 |
+6.6394 |
-2.106 |
| 2015-08-05 |
2015-08-20 |
+8.7741 |
-1.094 |
| 2015-08-20 |
2016-05-13 |
+2.6006 |
-0.134 |
log10 r = log10(heliocentric distance / AU), Δ = geocentric distance (AU)
Ephemeris
| Date/Time (UTC) |
RA (J2000) |
Dec (J2000) |
Nearest HIP |
Dist from HIP (arcmin) |
| 2026-06-01 00:00 |
21:39:26.79 |
-58:27:04.3 |
HIP 106797 |
14.01 |
| 2026-06-01 12:00 |
21:39:24.54 |
-58:27:51.2 |
HIP 106797 |
14.13 |
| 2026-06-02 00:00 |
21:39:22.22 |
-58:28:38.1 |
HIP 106797 |
14.29 |
| 2026-06-02 12:00 |
21:39:19.84 |
-58:29:25.0 |
HIP 106797 |
14.49 |
| 2026-06-03 00:00 |
21:39:17.39 |
-58:30:11.9 |
HIP 106797 |
14.73 |
| 2026-06-03 12:00 |
21:39:14.88 |
-58:30:58.8 |
HIP 106797 |
15.01 |
| 2026-06-04 00:00 |
21:39:12.30 |
-58:31:45.7 |
HIP 106797 |
15.32 |
| 2026-06-04 12:00 |
21:39:09.66 |
-58:32:32.5 |
HIP 106797 |
15.67 |
| 2026-06-05 00:00 |
21:39:06.95 |
-58:33:19.4 |
HIP 106797 |
16.05 |
| 2026-06-05 12:00 |
21:39:04.18 |
-58:34:06.3 |
HIP 106797 |
16.46 |
| 2026-06-06 00:00 |
21:39:01.34 |
-58:34:53.1 |
HIP 106797 |
16.90 |
| 2026-06-06 12:00 |
21:38:58.44 |
-58:35:39.9 |
HIP 106797 |
17.37 |
| 2026-06-07 00:00 |
21:38:55.47 |
-58:36:26.7 |
HIP 106797 |
17.87 |
| 2026-06-07 12:00 |
21:38:52.44 |
-58:37:13.4 |
HIP 106797 |
18.38 |
| 2026-06-08 00:00 |
21:38:49.35 |
-58:38:00.1 |
HIP 106797 |
18.93 |
| 2026-06-08 12:00 |
21:38:46.19 |
-58:38:46.8 |
HIP 106797 |
19.49 |
| 2026-06-09 00:00 |
21:38:42.97 |
-58:39:33.5 |
HIP 106797 |
20.07 |
| 2026-06-09 12:00 |
21:38:39.68 |
-58:40:20.0 |
HIP 106904 |
20.49 |
| 2026-06-10 00:00 |
21:38:36.33 |
-58:41:06.6 |
HIP 106904 |
19.80 |
| 2026-06-10 12:00 |
21:38:32.92 |
-58:41:53.1 |
HIP 106904 |
19.13 |
| 2026-06-11 00:00 |
21:38:29.44 |
-58:42:39.5 |
HIP 106904 |
18.48 |
| 2026-06-11 12:00 |
21:38:25.90 |
-58:43:25.8 |
HIP 106904 |
17.85 |
| 2026-06-12 00:00 |
21:38:22.30 |
-58:44:12.1 |
HIP 106904 |
17.25 |
| 2026-06-12 12:00 |
21:38:18.63 |
-58:44:58.4 |
HIP 106904 |
16.69 |
| 2026-06-13 00:00 |
21:38:14.90 |
-58:45:44.5 |
HIP 106904 |
16.15 |
| 2026-06-13 12:00 |
21:38:11.11 |
-58:46:30.6 |
HIP 106904 |
15.66 |
| 2026-06-14 00:00 |
21:38:07.26 |
-58:47:16.6 |
HIP 106904 |
15.21 |
| 2026-06-14 12:00 |
21:38:03.35 |
-58:48:02.5 |
HIP 106904 |
14.81 |
| 2026-06-15 00:00 |
21:37:59.37 |
-58:48:48.3 |
HIP 106904 |
14.46 |
| 2026-06-15 12:00 |
21:37:55.33 |
-58:49:34.0 |
HIP 106904 |
14.17 |
| 2026-06-16 00:00 |
21:37:51.23 |
-58:50:19.6 |
HIP 106904 |
13.94 |
| 2026-06-16 12:00 |
21:37:47.07 |
-58:51:05.1 |
HIP 106904 |
13.78 |
| 2026-06-17 00:00 |
21:37:42.85 |
-58:51:50.5 |
HIP 106904 |
13.68 |
| 2026-06-17 12:00 |
21:37:38.57 |
-58:52:35.8 |
HIP 106904 |
13.66 |
| 2026-06-18 00:00 |
21:37:34.23 |
-58:53:20.9 |
HIP 106904 |
13.70 |
| 2026-06-18 12:00 |
21:37:29.83 |
-58:54:06.0 |
HIP 106904 |
13.82 |
| 2026-06-19 00:00 |
21:37:25.37 |
-58:54:50.9 |
HIP 106904 |
14.00 |
| 2026-06-19 12:00 |
21:37:20.85 |
-58:55:35.7 |
HIP 106904 |
14.26 |
| 2026-06-20 00:00 |
21:37:16.27 |
-58:56:20.4 |
HIP 106904 |
14.58 |
| 2026-06-20 12:00 |
21:37:11.64 |
-58:57:04.9 |
HIP 106904 |
14.96 |
| 2026-06-21 00:00 |
21:37:06.94 |
-58:57:49.3 |
HIP 106904 |
15.39 |
| 2026-06-21 12:00 |
21:37:02.19 |
-58:58:33.5 |
HIP 106904 |
15.88 |
| 2026-06-22 00:00 |
21:36:57.39 |
-58:59:17.6 |
HIP 106904 |
16.42 |