| Parameter |
Value |
| Designation |
C/1969 Y1 (Bennett) |
| Type |
C |
| Perihelion (tp_cal, UTC) |
1970-03-20T01:05:24.547200Z |
| Orbit solution date (soln_date, UTC) |
2021-04-15T23:29:19Z |
| Obs used |
529 |
| NEO |
- |
| M1 |
4.600 |
| K1 |
12.000 |
| PC |
- |
Osculating Elements
| Parameter |
Value |
| Epoch (epoch_cal, TDB) |
1970-04-12.0000000 |
| e |
0.99629328 |
| q (au) |
0.537620 |
| a (au) |
145.039330 |
| i (deg) |
90.039811 |
| Ω (om, deg) |
224.657683 |
| ω (w, deg) |
354.149089 |
| M (ma, deg) |
0.012952 |
Magnitude
Scatter + Global Linear
$$
M_a = (4.085 + 3.365\cdot 2.5\log_{10} r) + \epsilon - 2.5\log_{10}\Phi(\theta) + 5\log_{10}\Delta
$$
$$
\theta = 180^\circ - \alpha
$$
$$
\Phi(\theta) = \frac{\delta_{90} D(\theta) + 1}{\delta_{90} + 1},\quad D(\theta) = k\cdot \Phi_{HG}(\theta; g_f) + (1-k)\cdot \Phi_{HG}(\theta; g_b)
$$
$$
\Phi_{HG}(\theta; g) = \left(\frac{1+g^2}{1+g^2-2g\cos\theta}\right)^{3/2},\quad \Phi_{HG}(90^\circ)=1
$$
Model Parameters
| Parameter |
Value |
| H0 |
4.085 |
| n |
3.365 |
| gf |
0.800 |
| gb |
-0.500 |
| k |
1.000 |
| 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 |
| 1969-12-28 |
1970-03-20 |
+3.0975 |
+0.766 |
| 1970-03-20 |
1970-04-13 |
-4.8648 |
-1.069 |
| 1970-04-13 |
1970-05-01 |
+0.0535 |
-0.380 |
| 1970-05-01 |
1970-11-20 |
+1.8732 |
-0.612 |
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 |
02:28:21.41 |
+29:19:58.5 |
HIP 11579 |
19.60 |
| 2026-03-26 12:00 |
02:28:22.77 |
+29:20:00.6 |
HIP 11579 |
19.46 |
| 2026-03-27 00:00 |
02:28:24.15 |
+29:20:02.8 |
HIP 11579 |
19.32 |
| 2026-03-27 12:00 |
02:28:25.53 |
+29:20:05.1 |
HIP 11579 |
19.18 |
| 2026-03-28 00:00 |
02:28:26.92 |
+29:20:07.4 |
HIP 11579 |
19.05 |
| 2026-03-28 12:00 |
02:28:28.32 |
+29:20:09.8 |
HIP 11579 |
18.92 |
| 2026-03-29 00:00 |
02:28:29.73 |
+29:20:12.3 |
HIP 11579 |
18.80 |
| 2026-03-29 12:00 |
02:28:31.14 |
+29:20:14.9 |
HIP 11579 |
18.68 |
| 2026-03-30 00:00 |
02:28:32.56 |
+29:20:17.5 |
HIP 11579 |
18.56 |
| 2026-03-30 12:00 |
02:28:33.99 |
+29:20:20.3 |
HIP 11579 |
18.46 |
| 2026-03-31 00:00 |
02:28:35.42 |
+29:20:23.0 |
HIP 11579 |
18.35 |
| 2026-03-31 12:00 |
02:28:36.86 |
+29:20:25.9 |
HIP 11579 |
18.25 |
| 2026-04-01 00:00 |
02:28:38.31 |
+29:20:28.8 |
HIP 11579 |
18.16 |
| 2026-04-01 12:00 |
02:28:39.77 |
+29:20:31.8 |
HIP 11579 |
18.07 |
| 2026-04-02 00:00 |
02:28:41.23 |
+29:20:34.9 |
HIP 11579 |
17.99 |
| 2026-04-02 12:00 |
02:28:42.69 |
+29:20:38.0 |
HIP 11579 |
17.91 |
| 2026-04-03 00:00 |
02:28:44.17 |
+29:20:41.2 |
HIP 11579 |
17.85 |
| 2026-04-03 12:00 |
02:28:45.65 |
+29:20:44.5 |
HIP 11579 |
17.78 |
| 2026-04-04 00:00 |
02:28:47.13 |
+29:20:47.9 |
HIP 11579 |
17.73 |
| 2026-04-04 12:00 |
02:28:48.62 |
+29:20:51.3 |
HIP 11579 |
17.68 |
| 2026-04-05 00:00 |
02:28:50.12 |
+29:20:54.8 |
HIP 11579 |
17.63 |
| 2026-04-05 12:00 |
02:28:51.62 |
+29:20:58.3 |
HIP 11579 |
17.60 |
| 2026-04-06 00:00 |
02:28:53.13 |
+29:21:02.0 |
HIP 11579 |
17.57 |
| 2026-04-06 12:00 |
02:28:54.65 |
+29:21:05.6 |
HIP 11579 |
17.54 |
| 2026-04-07 00:00 |
02:28:56.17 |
+29:21:09.4 |
HIP 11579 |
17.53 |
| 2026-04-07 12:00 |
02:28:57.69 |
+29:21:13.2 |
HIP 11579 |
17.52 |
| 2026-04-08 00:00 |
02:28:59.22 |
+29:21:17.1 |
HIP 11579 |
17.52 |
| 2026-04-08 12:00 |
02:29:00.76 |
+29:21:21.1 |
HIP 11579 |
17.53 |
| 2026-04-09 00:00 |
02:29:02.30 |
+29:21:25.1 |
HIP 11579 |
17.54 |
| 2026-04-09 12:00 |
02:29:03.85 |
+29:21:29.2 |
HIP 11579 |
17.57 |
| 2026-04-10 00:00 |
02:29:05.40 |
+29:21:33.4 |
HIP 11579 |
17.60 |
| 2026-04-10 12:00 |
02:29:06.95 |
+29:21:37.6 |
HIP 11579 |
17.63 |
| 2026-04-11 00:00 |
02:29:08.51 |
+29:21:41.9 |
HIP 11579 |
17.68 |
| 2026-04-11 12:00 |
02:29:10.08 |
+29:21:46.2 |
HIP 11579 |
17.73 |
| 2026-04-12 00:00 |
02:29:11.65 |
+29:21:50.6 |
HIP 11579 |
17.80 |
| 2026-04-12 12:00 |
02:29:13.22 |
+29:21:55.1 |
HIP 11579 |
17.86 |
| 2026-04-13 00:00 |
02:29:14.80 |
+29:21:59.7 |
HIP 11579 |
17.94 |
| 2026-04-13 12:00 |
02:29:16.38 |
+29:22:04.3 |
HIP 11579 |
18.03 |
| 2026-04-14 00:00 |
02:29:17.96 |
+29:22:09.0 |
HIP 11579 |
18.12 |
| 2026-04-14 12:00 |
02:29:19.55 |
+29:22:13.7 |
HIP 11579 |
18.22 |
| 2026-04-15 00:00 |
02:29:21.15 |
+29:22:18.5 |
HIP 11579 |
18.32 |
| 2026-04-15 12:00 |
02:29:22.74 |
+29:22:23.4 |
HIP 11579 |
18.44 |
| 2026-04-16 00:00 |
02:29:24.34 |
+29:22:28.3 |
HIP 11579 |
18.56 |