4P/Faye (0004P)
TRY AGAIN 2028
Type: Periodic
Perihelion date: 8 September 2021
Perihelion distance (q): 1.6
Aphelion distance (Q) : 6.0
Period (years): 7.5
Eccentricity (e): 0.58
Inclination (i): 8.0
JPL orbit diagram
COBS lightcurve
Hervé Faye (Royal Observatory, Paris) discovered this comet on 23 November 1843,
near Gamma Orionis. The comet exhibited a distinct nucleus, which emitted faint
indications of a tail extending 4 arcmin away from the sun. Due to cloudy weather,
Faye was not able to confirm his discovery until 25 November. The comet was kept
under observation until 10 April 1844 during the discovery apparition, or for more
than 4 months. The comet had passed perihelion one month prior to discovery, but
was discovered about a day before its closest passage by Earth (0.79 AU). T.
Henderson (Edinburgh) became the first to realize this comet was moving in a short-
period orbit. Although his initial computed orbital period was 6.58 years, additional
observations allowed both John. R. Hind and himself to independently revise the orbit
during the next few months. Ultimately, by May, the period had been refined to 7.43
years.
As the comet's expected apparition of 1851 approached, astronomers needed as
accurate a prediction as possible to guarantee recovery. Urbain Jean Joseph
Leverrier undertook this task. He found the comet had passed 0.25 AU from Jupiter
during 1841, which acted to decrease the perihelion distance from 1.81 AU to the
discovery value of 1.69 AU. He then determined the comet's next perihelion would fall
during early April 1851. James Challis (Cambridge, England) recovered the comet
very close to Leverrier's predicted position on 28 November 1850.
This comet has been seen at every return since its discovery, except for those of
1903 and 1918, which were especially unfavorable. The comet's having been missed
during 1903 brought problems for the 1910 return. Initially searches during the 1910
apparition were failing to locate the comet. Interestingly, Cerulli (Teramo, Italy) found
a 10th-magnitude comet on 8 November 1910. After observations were obtained for
the next two weeks, the first orbital computations revealed this was Faye's periodic
comet.
Close approaches to planets:
•
1.32 AU from Jupiter on 25 October 1993 - decreased perihelion distance from
1.59 AU to 1.66 AU; decreased orbital period from 7.34 to 7.52 years
•
0.69 AU from Earth on 30 October 2006 0.63 AU from Jupiter on 7 March 2018 -
decreased perihelion distance from 1.66 AU to 1.62 AU; decreased orbital period
from 7.51 to 7.48 years
•
0.94 AU from Earth on 5 December 2021 0.98 AU from Earth on 8 December
2036
Observations (VEMag = visual equivalent magnitude)
Date
10x10 mag
Error
VEmag
Coma '
25 Oct 14
15.93
0.03
14.3
0.4
02 Nov 14
15.91
0.01
14.3
0.4
09 Nov 14
16.12
0.07
14.1
0.3
16 Nov 14
16.02
0.03
14.8
0.2
24 Nov 14
16.20
0.02
15.2
0.2
01 Dec 14
16.12
0.06
14.7
0.2
16 Dec 14
16.24
0.05
14.4
0.3
23 Dec 14
16.23
0.02
14.2
0.3
30 Dec 14
16.27
0.05
14.8
0.3
14 Jan 15
16.24
0.03
14.6
0.3
21 Jan 15
16.21
0.04
14.2
0.3
28 Jan 15
16.20
0.02
14.4
0.4
08 Feb 15
16.11
0.04
14.2
0.2
16 Feb 15
16.17
0.04
14.4
0.3
11 Mar 15
16.69
0.03
14.9
0.2
18 Mar 15
16.93
0.03
14.8
0.3
08 Apr 15
17.38
0.06
15.0
0.2
19 Apr 15
17.76
0.04
15.8
0.2
21-Aug-21
12.9
0.8
05-Sep-21
12.4
1.5
09-Sep-21
13.57
0.01
10.5
6.4
16-Sep-21
14.15
0.10
12.3
1.7