C/2014 Q1 (PANSTARRS)
| 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 |
2014-12-17 |
+8.1822 |
-5.233 |
| 2014-12-17 |
2015-05-14 |
-1.1668 |
-0.020 |
| 2015-05-14 |
2015-06-22 |
+7.0841 |
-1.117 |
| 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) |
| 2026-02-03 00:00 |
21:22:49.43 |
-57:07:49.5 |
HIP 105719 |
17.50 |
| 2026-02-03 12:00 |
21:22:57.26 |
-57:07:30.1 |
HIP 105719 |
16.70 |
| 2026-02-04 00:00 |
21:23:05.08 |
-57:07:11.0 |
HIP 105719 |
15.94 |
| 2026-02-04 12:00 |
21:23:12.91 |
-57:06:52.3 |
HIP 105719 |
15.22 |
| 2026-02-05 00:00 |
21:23:20.73 |
-57:06:34.0 |
HIP 105719 |
14.54 |
| 2026-02-05 12:00 |
21:23:28.56 |
-57:06:15.9 |
HIP 105719 |
13.91 |
| 2026-02-06 00:00 |
21:23:36.39 |
-57:05:58.2 |
HIP 105719 |
13.34 |
| 2026-02-06 12:00 |
21:23:44.22 |
-57:05:40.9 |
HIP 105719 |
12.83 |
| 2026-02-07 00:00 |
21:23:52.04 |
-57:05:23.9 |
HIP 105719 |
12.39 |
| 2026-02-07 12:00 |
21:23:59.87 |
-57:05:07.3 |
HIP 105719 |
12.04 |
| 2026-02-08 00:00 |
21:24:07.69 |
-57:04:51.0 |
HIP 105719 |
11.77 |
| 2026-02-08 12:00 |
21:24:15.51 |
-57:04:35.0 |
HIP 105719 |
11.59 |
| 2026-02-09 00:00 |
21:24:23.33 |
-57:04:19.4 |
HIP 105719 |
11.51 |
| 2026-02-09 12:00 |
21:24:31.15 |
-57:04:04.2 |
HIP 105719 |
11.53 |
| 2026-02-10 00:00 |
21:24:38.96 |
-57:03:49.3 |
HIP 105719 |
11.64 |
| 2026-02-10 12:00 |
21:24:46.77 |
-57:03:34.8 |
HIP 105719 |
11.85 |
| 2026-02-11 00:00 |
21:24:54.57 |
-57:03:20.6 |
HIP 105719 |
12.14 |
| 2026-02-11 12:00 |
21:25:02.37 |
-57:03:06.8 |
HIP 105719 |
12.51 |
| 2026-02-12 00:00 |
21:25:10.16 |
-57:02:53.3 |
HIP 105719 |
12.96 |
| 2026-02-12 12:00 |
21:25:17.95 |
-57:02:40.2 |
HIP 105719 |
13.48 |
| 2026-02-13 00:00 |
21:25:25.73 |
-57:02:27.5 |
HIP 105719 |
14.05 |
| 2026-02-13 12:00 |
21:25:33.50 |
-57:02:15.1 |
HIP 105719 |
14.67 |
| 2026-02-14 00:00 |
21:25:41.27 |
-57:02:03.1 |
HIP 105719 |
15.34 |
| 2026-02-14 12:00 |
21:25:49.02 |
-57:01:51.4 |
HIP 105719 |
16.05 |
| 2026-02-15 00:00 |
21:25:56.77 |
-57:01:40.1 |
HIP 105719 |
16.79 |
| 2026-02-15 12:00 |
21:26:04.51 |
-57:01:29.2 |
HIP 105719 |
17.56 |
| 2026-02-16 00:00 |
21:26:12.24 |
-57:01:18.7 |
HIP 105719 |
18.35 |
| 2026-02-16 12:00 |
21:26:19.96 |
-57:01:08.5 |
HIP 105719 |
19.16 |
| 2026-02-17 00:00 |
21:26:27.67 |
-57:00:58.7 |
HIP 105719 |
19.99 |
| 2026-02-17 12:00 |
21:26:35.37 |
-57:00:49.2 |
HIP 105719 |
20.84 |
| 2026-02-18 00:00 |
21:26:43.06 |
-57:00:40.1 |
HIP 105719 |
21.70 |
| 2026-02-18 12:00 |
21:26:50.74 |
-57:00:31.4 |
HIP 105719 |
22.57 |
| 2026-02-19 00:00 |
21:26:58.40 |
-57:00:23.1 |
HIP 105719 |
23.45 |
| 2026-02-19 12:00 |
21:27:06.05 |
-57:00:15.1 |
HIP 105719 |
24.34 |
| 2026-02-20 00:00 |
21:27:13.69 |
-57:00:07.5 |
HIP 105719 |
25.23 |
| 2026-02-20 12:00 |
21:27:21.31 |
-57:00:00.3 |
HIP 105719 |
26.13 |
| 2026-02-21 00:00 |
21:27:28.92 |
-56:59:53.4 |
HIP 105719 |
27.04 |
| 2026-02-21 12:00 |
21:27:36.51 |
-56:59:46.9 |
HIP 106105 |
26.77 |
| 2026-02-22 00:00 |
21:27:44.09 |
-56:59:40.8 |
HIP 106105 |
26.25 |
| 2026-02-22 12:00 |
21:27:51.65 |
-56:59:35.1 |
HIP 106105 |
25.75 |
| 2026-02-23 00:00 |
21:27:59.19 |
-56:59:29.7 |
HIP 106105 |
25.28 |
| 2026-02-23 12:00 |
21:28:06.72 |
-56:59:24.7 |
HIP 106237 |
24.53 |
| 2026-02-24 00:00 |
21:28:14.23 |
-56:59:20.1 |
HIP 106237 |
23.51 |