| Parameter |
Value |
| Designation |
C/2002 T7 (LINEAR) |
| Type |
C |
| Perihelion (tp_cal, UTC) |
2004-04-23T01:29:19.495680Z |
| Orbit solution date (soln_date, UTC) |
2021-04-15T23:30:22Z |
| Obs used |
4397 |
| NEO |
- |
| M1 |
7.600 |
| K1 |
6.500 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
2003-11-16.0000000 |
| e |
1.00048628 |
| q (au) |
0.614546 |
| a (au) |
-1263.766985 |
| i (deg) |
160.582715 |
| Ω (om, deg) |
94.856573 |
| ω (w, deg) |
157.739084 |
| M (ma, deg) |
-0.003490 |
Magnitude
Scatter + Global Linear
$$
M_a = (6.176 + 3.575\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
6.176 |
| n |
3.575 |
| gf |
0.800 |
| gb |
-0.500 |
| k |
0.800 |
| 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 |
| 2001-01-14 |
2002-10-29 |
-50.9308 |
+42.214 |
| 2002-10-29 |
2004-04-22 |
+0.0934 |
-0.200 |
| 2004-04-23 |
2004-05-22 |
+11.1569 |
+2.707 |
| 2004-05-22 |
2006-03-20 |
-0.3710 |
+1.312 |
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 |
08:38:33.13 |
+07:04:35.7 |
HIP 42418 |
9.88 |
| 2026-09-20 12:00 |
08:38:34.69 |
+07:04:24.0 |
HIP 42418 |
9.48 |
| 2026-09-21 00:00 |
08:38:36.23 |
+07:04:12.4 |
HIP 42418 |
9.08 |
| 2026-09-21 12:00 |
08:38:37.75 |
+07:04:00.7 |
HIP 42418 |
8.69 |
| 2026-09-22 00:00 |
08:38:39.26 |
+07:03:49.1 |
HIP 42418 |
8.30 |
| 2026-09-22 12:00 |
08:38:40.75 |
+07:03:37.5 |
HIP 42418 |
7.92 |
| 2026-09-23 00:00 |
08:38:42.22 |
+07:03:25.9 |
HIP 42418 |
7.54 |
| 2026-09-23 12:00 |
08:38:43.67 |
+07:03:14.3 |
HIP 42418 |
7.17 |
| 2026-09-24 00:00 |
08:38:45.11 |
+07:03:02.8 |
HIP 42418 |
6.81 |
| 2026-09-24 12:00 |
08:38:46.53 |
+07:02:51.3 |
HIP 42418 |
6.46 |
| 2026-09-25 00:00 |
08:38:47.93 |
+07:02:39.8 |
HIP 42418 |
6.12 |
| 2026-09-25 12:00 |
08:38:49.32 |
+07:02:28.3 |
HIP 42418 |
5.78 |
| 2026-09-26 00:00 |
08:38:50.69 |
+07:02:16.9 |
HIP 42418 |
5.46 |
| 2026-09-26 12:00 |
08:38:52.04 |
+07:02:05.5 |
HIP 42418 |
5.15 |
| 2026-09-27 00:00 |
08:38:53.37 |
+07:01:54.1 |
HIP 42418 |
4.85 |
| 2026-09-27 12:00 |
08:38:54.68 |
+07:01:42.8 |
HIP 42418 |
4.56 |
| 2026-09-28 00:00 |
08:38:55.98 |
+07:01:31.5 |
HIP 42418 |
4.29 |
| 2026-09-28 12:00 |
08:38:57.26 |
+07:01:20.2 |
HIP 42418 |
4.04 |
| 2026-09-29 00:00 |
08:38:58.52 |
+07:01:08.9 |
HIP 42418 |
3.80 |
| 2026-09-29 12:00 |
08:38:59.76 |
+07:00:57.7 |
HIP 42418 |
3.59 |
| 2026-09-30 00:00 |
08:39:00.98 |
+07:00:46.5 |
HIP 42418 |
3.41 |
| 2026-09-30 12:00 |
08:39:02.19 |
+07:00:35.4 |
HIP 42418 |
3.25 |
| 2026-10-01 00:00 |
08:39:03.38 |
+07:00:24.3 |
HIP 42418 |
3.13 |
| 2026-10-01 12:00 |
08:39:04.54 |
+07:00:13.2 |
HIP 42418 |
3.04 |
| 2026-10-02 00:00 |
08:39:05.69 |
+07:00:02.1 |
HIP 42418 |
2.98 |
| 2026-10-02 12:00 |
08:39:06.82 |
+06:59:51.1 |
HIP 42418 |
2.96 |
| 2026-10-03 00:00 |
08:39:07.93 |
+06:59:40.2 |
HIP 42418 |
2.98 |
| 2026-10-03 12:00 |
08:39:09.02 |
+06:59:29.2 |
HIP 42418 |
3.03 |
| 2026-10-04 00:00 |
08:39:10.09 |
+06:59:18.4 |
HIP 42418 |
3.11 |
| 2026-10-04 12:00 |
08:39:11.15 |
+06:59:07.5 |
HIP 42418 |
3.21 |
| 2026-10-05 00:00 |
08:39:12.18 |
+06:58:56.7 |
HIP 42418 |
3.34 |
| 2026-10-05 12:00 |
08:39:13.19 |
+06:58:46.0 |
HIP 42418 |
3.49 |
| 2026-10-06 00:00 |
08:39:14.19 |
+06:58:35.3 |
HIP 42418 |
3.65 |
| 2026-10-06 12:00 |
08:39:15.16 |
+06:58:24.6 |
HIP 42418 |
3.83 |
| 2026-10-07 00:00 |
08:39:16.12 |
+06:58:14.0 |
HIP 42418 |
4.02 |
| 2026-10-07 12:00 |
08:39:17.05 |
+06:58:03.4 |
HIP 42418 |
4.21 |
| 2026-10-08 00:00 |
08:39:17.96 |
+06:57:52.9 |
HIP 42418 |
4.41 |
| 2026-10-08 12:00 |
08:39:18.86 |
+06:57:42.4 |
HIP 42418 |
4.62 |
| 2026-10-09 00:00 |
08:39:19.73 |
+06:57:32.0 |
HIP 42418 |
4.82 |
| 2026-10-09 12:00 |
08:39:20.58 |
+06:57:21.6 |
HIP 42418 |
5.03 |
| 2026-10-10 00:00 |
08:39:21.41 |
+06:57:11.3 |
HIP 42418 |
5.24 |
| 2026-10-10 12:00 |
08:39:22.23 |
+06:57:01.0 |
HIP 42418 |
5.45 |
| 2026-10-11 00:00 |
08:39:23.02 |
+06:56:50.8 |
HIP 42418 |
5.66 |