| 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) |
| 2026-03-26 00:00 |
20:54:20.46 |
-27:02:01.7 |
HIP 103182 |
24.47 |
| 2026-03-26 12:00 |
20:54:21.26 |
-27:02:01.2 |
HIP 103182 |
24.47 |
| 2026-03-27 00:00 |
20:54:22.04 |
-27:02:00.7 |
HIP 103182 |
24.47 |
| 2026-03-27 12:00 |
20:54:22.82 |
-27:02:00.3 |
HIP 103182 |
24.46 |
| 2026-03-28 00:00 |
20:54:23.59 |
-27:02:00.0 |
HIP 103182 |
24.47 |
| 2026-03-28 12:00 |
20:54:24.35 |
-27:01:59.7 |
HIP 103182 |
24.47 |
| 2026-03-29 00:00 |
20:54:25.10 |
-27:01:59.4 |
HIP 103182 |
24.47 |
| 2026-03-29 12:00 |
20:54:25.84 |
-27:01:59.2 |
HIP 103182 |
24.48 |
| 2026-03-30 00:00 |
20:54:26.57 |
-27:01:59.1 |
HIP 103182 |
24.49 |
| 2026-03-30 12:00 |
20:54:27.29 |
-27:01:59.0 |
HIP 103182 |
24.50 |
| 2026-03-31 00:00 |
20:54:28.01 |
-27:01:58.9 |
HIP 103182 |
24.51 |
| 2026-03-31 12:00 |
20:54:28.71 |
-27:01:58.9 |
HIP 103182 |
24.53 |
| 2026-04-01 00:00 |
20:54:29.40 |
-27:01:58.9 |
HIP 103182 |
24.54 |
| 2026-04-01 12:00 |
20:54:30.09 |
-27:01:59.0 |
HIP 103182 |
24.56 |
| 2026-04-02 00:00 |
20:54:30.76 |
-27:01:59.2 |
HIP 103182 |
24.58 |
| 2026-04-02 12:00 |
20:54:31.43 |
-27:01:59.3 |
HIP 103182 |
24.60 |
| 2026-04-03 00:00 |
20:54:32.08 |
-27:01:59.6 |
HIP 103182 |
24.62 |
| 2026-04-03 12:00 |
20:54:32.73 |
-27:01:59.9 |
HIP 103182 |
24.64 |
| 2026-04-04 00:00 |
20:54:33.37 |
-27:02:00.2 |
HIP 103182 |
24.67 |
| 2026-04-04 12:00 |
20:54:33.99 |
-27:02:00.6 |
HIP 103182 |
24.69 |
| 2026-04-05 00:00 |
20:54:34.61 |
-27:02:01.0 |
HIP 103182 |
24.72 |
| 2026-04-05 12:00 |
20:54:35.22 |
-27:02:01.5 |
HIP 103182 |
24.75 |
| 2026-04-06 00:00 |
20:54:35.81 |
-27:02:02.0 |
HIP 103182 |
24.78 |
| 2026-04-06 12:00 |
20:54:36.40 |
-27:02:02.6 |
HIP 103182 |
24.81 |
| 2026-04-07 00:00 |
20:54:36.98 |
-27:02:03.2 |
HIP 103182 |
24.84 |
| 2026-04-07 12:00 |
20:54:37.55 |
-27:02:03.9 |
HIP 103182 |
24.87 |
| 2026-04-08 00:00 |
20:54:38.10 |
-27:02:04.6 |
HIP 103182 |
24.90 |
| 2026-04-08 12:00 |
20:54:38.65 |
-27:02:05.3 |
HIP 103182 |
24.94 |
| 2026-04-09 00:00 |
20:54:39.19 |
-27:02:06.2 |
HIP 103182 |
24.97 |
| 2026-04-09 12:00 |
20:54:39.72 |
-27:02:07.0 |
HIP 103182 |
25.01 |
| 2026-04-10 00:00 |
20:54:40.23 |
-27:02:07.9 |
HIP 103182 |
25.05 |
| 2026-04-10 12:00 |
20:54:40.74 |
-27:02:08.9 |
HIP 103182 |
25.08 |
| 2026-04-11 00:00 |
20:54:41.24 |
-27:02:09.9 |
HIP 103182 |
25.12 |
| 2026-04-11 12:00 |
20:54:41.72 |
-27:02:11.0 |
HIP 103182 |
25.16 |
| 2026-04-12 00:00 |
20:54:42.20 |
-27:02:12.1 |
HIP 103182 |
25.20 |
| 2026-04-12 12:00 |
20:54:42.66 |
-27:02:13.2 |
HIP 103182 |
25.24 |
| 2026-04-13 00:00 |
20:54:43.12 |
-27:02:14.4 |
HIP 103182 |
25.28 |
| 2026-04-13 12:00 |
20:54:43.57 |
-27:02:15.7 |
HIP 103182 |
25.33 |
| 2026-04-14 00:00 |
20:54:44.00 |
-27:02:17.0 |
HIP 103182 |
25.37 |
| 2026-04-14 12:00 |
20:54:44.42 |
-27:02:18.3 |
HIP 103182 |
25.41 |
| 2026-04-15 00:00 |
20:54:44.84 |
-27:02:19.7 |
HIP 103182 |
25.45 |
| 2026-04-15 12:00 |
20:54:45.24 |
-27:02:21.1 |
HIP 103182 |
25.50 |
| 2026-04-16 00:00 |
20:54:45.63 |
-27:02:22.6 |
HIP 103182 |
25.54 |