C/1942 X1 (Whipple-Fedtke-Tevzadze)
| Parameter |
Value |
| Designation |
C/1942 X1 (Whipple-Fedtke-Tevzadze) |
| Type |
C |
| Perihelion (tp_cal, UTC) |
1943-02-06T17:18:23.040000Z |
| Orbit solution date (soln_date, UTC) |
- |
| Obs used |
166 |
| NEO |
- |
| M1 |
- |
| K1 |
- |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
1943-02-05.0000000 |
| e |
0.99219600 |
| q (au) |
1.353647 |
| a (au) |
173.455536 |
| i (deg) |
19.712700 |
| Ω (om, deg) |
100.799000 |
| ω (w, deg) |
39.843200 |
| M (ma, deg) |
-0.000743 |
Magnitude


Scatter + Global Linear
$$
M_a = (3.857 + 3.863\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
3.857 |
| n |
3.863 |
| gf |
1.000 |
| gb |
-0.500 |
| 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 |
| 1942-12-15 |
1943-02-06 |
+38.1961 |
-4.915 |
| 1943-02-06 |
1943-04-13 |
+2.8278 |
-0.764 |
| 1943-04-13 |
1943-06-05 |
-2.7997 |
+0.823 |
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 |
20:52:24.80 |
-27:06:46.2 |
HIP 102954 |
13.86 |
| 2026-02-03 12:00 |
20:52:26.13 |
-27:06:41.6 |
HIP 102954 |
14.15 |
| 2026-02-04 00:00 |
20:52:27.45 |
-27:06:36.9 |
HIP 102978 |
14.27 |
| 2026-02-04 12:00 |
20:52:28.78 |
-27:06:32.3 |
HIP 102978 |
14.39 |
| 2026-02-05 00:00 |
20:52:30.10 |
-27:06:27.7 |
HIP 102978 |
14.51 |
| 2026-02-05 12:00 |
20:52:31.42 |
-27:06:23.1 |
HIP 102978 |
14.64 |
| 2026-02-06 00:00 |
20:52:32.74 |
-27:06:18.6 |
HIP 102978 |
14.77 |
| 2026-02-06 12:00 |
20:52:34.06 |
-27:06:14.1 |
HIP 102978 |
14.91 |
| 2026-02-07 00:00 |
20:52:35.38 |
-27:06:09.6 |
HIP 102978 |
15.05 |
| 2026-02-07 12:00 |
20:52:36.69 |
-27:06:05.2 |
HIP 102978 |
15.20 |
| 2026-02-08 00:00 |
20:52:38.01 |
-27:06:00.7 |
HIP 102978 |
15.35 |
| 2026-02-08 12:00 |
20:52:39.32 |
-27:05:56.4 |
HIP 102978 |
15.51 |
| 2026-02-09 00:00 |
20:52:40.63 |
-27:05:52.0 |
HIP 102978 |
15.67 |
| 2026-02-09 12:00 |
20:52:41.94 |
-27:05:47.7 |
HIP 102978 |
15.84 |
| 2026-02-10 00:00 |
20:52:43.25 |
-27:05:43.4 |
HIP 102978 |
16.01 |
| 2026-02-10 12:00 |
20:52:44.56 |
-27:05:39.1 |
HIP 102978 |
16.18 |
| 2026-02-11 00:00 |
20:52:45.86 |
-27:05:34.9 |
HIP 102978 |
16.36 |
| 2026-02-11 12:00 |
20:52:47.16 |
-27:05:30.7 |
HIP 102978 |
16.54 |
| 2026-02-12 00:00 |
20:52:48.46 |
-27:05:26.5 |
HIP 102978 |
16.72 |
| 2026-02-12 12:00 |
20:52:49.76 |
-27:05:22.4 |
HIP 102978 |
16.91 |
| 2026-02-13 00:00 |
20:52:51.06 |
-27:05:18.3 |
HIP 102978 |
17.10 |
| 2026-02-13 12:00 |
20:52:52.35 |
-27:05:14.3 |
HIP 102978 |
17.29 |
| 2026-02-14 00:00 |
20:52:53.64 |
-27:05:10.2 |
HIP 102978 |
17.49 |
| 2026-02-14 12:00 |
20:52:54.93 |
-27:05:06.3 |
HIP 102978 |
17.69 |
| 2026-02-15 00:00 |
20:52:56.21 |
-27:05:02.3 |
HIP 102978 |
17.89 |
| 2026-02-15 12:00 |
20:52:57.49 |
-27:04:58.4 |
HIP 102978 |
18.09 |
| 2026-02-16 00:00 |
20:52:58.77 |
-27:04:54.5 |
HIP 102978 |
18.30 |
| 2026-02-16 12:00 |
20:53:00.04 |
-27:04:50.7 |
HIP 102978 |
18.50 |
| 2026-02-17 00:00 |
20:53:01.32 |
-27:04:46.8 |
HIP 102978 |
18.71 |
| 2026-02-17 12:00 |
20:53:02.58 |
-27:04:43.1 |
HIP 102978 |
18.92 |
| 2026-02-18 00:00 |
20:53:03.85 |
-27:04:39.3 |
HIP 102978 |
19.14 |
| 2026-02-18 12:00 |
20:53:05.11 |
-27:04:35.6 |
HIP 102978 |
19.35 |
| 2026-02-19 00:00 |
20:53:06.37 |
-27:04:32.0 |
HIP 102978 |
19.57 |
| 2026-02-19 12:00 |
20:53:07.62 |
-27:04:28.3 |
HIP 102978 |
19.78 |
| 2026-02-20 00:00 |
20:53:08.87 |
-27:04:24.8 |
HIP 102978 |
20.00 |
| 2026-02-20 12:00 |
20:53:10.12 |
-27:04:21.2 |
HIP 102978 |
20.22 |
| 2026-02-21 00:00 |
20:53:11.36 |
-27:04:17.7 |
HIP 102978 |
20.44 |
| 2026-02-21 12:00 |
20:53:12.60 |
-27:04:14.2 |
HIP 102978 |
20.66 |
| 2026-02-22 00:00 |
20:53:13.83 |
-27:04:10.8 |
HIP 102978 |
20.89 |
| 2026-02-22 12:00 |
20:53:15.06 |
-27:04:07.4 |
HIP 102978 |
21.11 |
| 2026-02-23 00:00 |
20:53:16.29 |
-27:04:04.1 |
HIP 102978 |
21.33 |
| 2026-02-23 12:00 |
20:53:17.51 |
-27:04:00.7 |
HIP 102978 |
21.56 |
| 2026-02-24 00:00 |
20:53:18.73 |
-27:03:57.5 |
HIP 102978 |
21.78 |