List of comets by type

This is a list of comets listed by type. Comets are sorted into four categories: periodic comets, non-periodic comets, comets with no meaningful orbit, and lost comets, displayed as either P, C, X, and D.
Many of the earlier comets to be observed in history are designated with an X or D due to not having the tools to measure a comet's orbit accurately and eventually losing it. X/1106 C1 is a good example. The orbital elements for the older non-periodic comets in the list assume that the comet has an eccentricity of roughly 1, and therefore the calculations are only approximate.

Guide to comet lists

Hyperbolic comet list—Comets that are hyperbolic
Near-parabolic comet list—Comets that have a period of over 1000 years
Long-period comet list—Comets with a period between 200 and 1000 years
List of periodic comets—Unnumbered comets with a period of less than 200 years
List of numbered comets—Comets numbered by the Minor Planet Center
Sungrazing comets
*Kreutz sungrazers
*Meyer group
*Kracht group
*Marsden group
*Ungrouped sungrazers

After Edmond Halley recognized that several apparitions of a comet every 75.3 years dating back to 239 BC were the same comet, it gave way to a new designation of periodic comets, with the first being named 1P/Halley. To date, there are 380 of these periodic comets, with many more on the way to getting an official designation.

Non-periodic comets

Non-periodic comets are generally comets that have only been seen on one occasion, or comets that have periods of thousands of years, to comets that are truly non-periodic, and will only come around the Solar System. The following comets are organized by their described types:

Ejection-trajectory comets

These are comets with an eccentricity so large that they only made one pass through the Solar System. These comets are further divided into near-Parabolic and Hyperbolic comets. A hypothetical true parabolic comet would have an eccentricity of exactly 1, and hyperbolic comets are any comet with an eccentricity of over 1. Most of the comets marked with an X are from the material cited here and the other comets are sourced from JPL Small-Body Database. Due to their hyperbolic orbits, it is impossible to determine where they come from, but it is expected that they are from the Oort Cloud, a cloud of icy bodies several thousand Astronomical units away from the Sun. However a few of these may be Interstellar comets
Comets observed in early times, which were later found to be observations of numbered periodic comets, are marked with /. For instance, X/-239 K1 was an appearance of Halley's comet in 239 BC, and as such is written as 1P/-239 K1. A significant portion of the comets passing closer than 0.01 AU to the Sun are fragments of the comet of 371 BC, which fractured into several pieces on the 326 AD perihelion, which further fractured into thousands of pieces on the 1106 AD perihelion, creating the cometary group now known as the Kreutz sungrazers. Due to the sheer size, and the fact that none of the group members have been given a numbered designation, the members are not stated on this list, and instead are listed in a separate list further [|below].

Near-parabolic comets

Comets with a very high eccentricity and a period of over 1,000 years that don't quite have a high enough velocity to escape the Solar System. Often, these comets, due to their extreme semimajor axes and eccentricity, will have small orbital interactions with planets and minor planets, most often ending up with the comets fluctuating significantly in their orbital path. These comets probably come from the Oort cloud, a cloud of comets orbiting the Sun from ~10,000 to roughly 50,000 AU.

Lost comets

The following comets, assigned with a D before their name, were subsequently lost after their discovery, and often remain lost to this day:

Comet designation	Name	Eccentricity	Semimajor axis	Inclination	Perihelion distance	Perihelion date	Last observed
D/1766 G1	Helfenzrieder	0.848	2.665	7.865	0.406	1766/04/27	1766/05/03
D/1770 L1	Lexell's Comet	0.786	3.153	1.552	0.674	1770/08/14	1770/10/03
D/1884 O1	Barnard	0.583	3.07	5.47	1.279	1884/08/16	1884/11/08
D/1886 K1	Brooks	0.571	3.092	12.671	1.325	1886/06/07	1886/07/03
D/1894 F1	Denning	0.698	3.797	5.527	1.147	1894/02/09	1894/06/05
D/1895 Q1	Swift	0.652	3.729	2.992	1.298	1895/08/21	1896/02/06
D/1918 W1	Schorr	0.469	3.545	5.575	1.884	1918/09/30	1918/12/31
D/1952 B1	Harrington–Wilson	0.514	3.428	16.35	1.6649	1951/10/30	1952/02/25
D/1977 C1	Skiff–Kosai	0.259	3.847	3.201	2.85	1976/08/03	1977/03/12
D/1978 R1	Haneda-Campos	0.6652	3.2898	5.9472	1.101414	1978/10/09	1978/11/29

Short period comets

Halley-type comets

Comets with a period between 20 and 200 years, named after the first identified member, Halley's Comet. These comets orbit between the orbit of Jupiter and Pluto, and are thought to be long-period comets that slowly migrated inwards, or Jupiter family comets that had been slingshotted outwards by Jupiter's gravity

Unnumbered Jupiter-family comets

While Jupiter-family comets are officially defined by, they can also be loosely defined by any comet with a period of less than 20 years, a relatively low inclination, and an orbit coinciding loosely with that of Jupiter's. These comets are often patchily observed, as orbital interactions with the planet often cause comets' orbits to become perturbed, causing them to not be found at the expected position in the sky and subsequently lost.

D/1993 F2 (Shoemaker–Levy 9)

One such Jupiter-family comet, Comet Shoemaker–Levy 9, approached close enough to Jupiter sometime between the late 1960s and early 1970s, and was caught into orbit of it. By the comet's discovery, an extremely close approach with Jupiter one year previously had fractured the comet into many pieces, before it collided with Jupiter between 16 July and 22 July 1994. The fragments are listed separately here, at epoch 1994/05/08.

Fragment	Eccentricity	Semimajor axis	Period	Inclination	Perihelion distance	Jupiter impact date
A	0.216209	6.86479	17.99	6.00329	5.380563	1994/07/16 20:11
B	0.215620	6.85975	17.97	5.99022	5.380652	1994/07/17 02:50
C	0.215169	6.85550	17.95	5.98196	5.380411	1994/07/17 07:12
D	0.214725	6.85158	17.93	5.97297	5.380370	1994/07/17 11:54
E	0.214411	6.84877	17.92	5.96663	5.380318	1994/07/17 15:11
F	0.213585	6.84163	17.90	5.94846	5.380362	1994/07/18 00:33
G	0.212881	6.83520	17.87	5.93551	5.380112	1994/07/18 07:32
H	0.211779	6.82547	17.83	5.91287	5.379973	1994/07/18 19:32
K	0.210425	6.81351	17.79	5.88507	5.379775	1994/07/19 10:21
L	0.209361	6.80416	17.75	5.86313	5.379632	1994/07/19 22:17
N	0.208277	6.79472	17.71	5.84046	5.379536	1994/07/20 10:31
P1	0.207745	6.79035	17.69	5.82929	5.379689	1994/07/20 16:30
P2	0.207887	6.79147	17.70	5.83126	5.379608	1994/07/20 15:23
Q1	0.207405	6.78700	17.68	5.82282	5.379348	1994/07/20 20:12
Q2	0.207453	6.78749	17.68	5.82361	5.379403	1994/07/20 19:44
R	0.206581	6.77982	17.65	5.80587	5.379232	1994/07/21 05:33
S	0.205737	6.77248	17.63	5.78848	5.379129	1994/07/21 15:15
T	0.205504	6.77073	17.62	5.78300	5.379319	1994/07/21 18:10
U	0.205167	6.76764	17.61	5.77631	5.379141	1994/07/21 21:55
V	0.204616	6.76283	17.59	5.76489	5.379046	1994/07/22 04:22
W	0.204282	6.75982	17.58	5.75982	5.378919	1994/07/22 08:05

Sungrazing comets

These comets have perihelion distances of less than 0.055 AU. Most belong to the Kreutz Sungrazers, a group of comets split off from the great comet of 1106, and before that, the comet of 371 BC. There are also several other cometary groups, all much smaller, that occasionally pass through. This list covers all Sungrazing groups, including sporadic, or ungrouped sungrazers.

Kreutz sungrazers

The largest group of them all, the Kreutz sungrazers are a group of comets descended from the breakup of a comet in 326 AD. They live up to their name, typically traveling less than 2 solar radii from the Sun. Because they travel so close, they often burn up, and it is the cause of their breakup. Many bright comets are members of the group, including Comet Ikeya–Seki, which broke in 3 pieces.

Meyer group

This is the second largest sungrazing group, and the only one with no discerned period. Further observations of this group may eventually find one, however.

Comet designation	Name	Eccentricity	Semimajor axis	Period	Inclination	Node	Perihelion distance	Perihelion date
C/1996 N3	SOHO	1.0	–	–	72.12	73.16	0.0351	1996/07/03
C/1997 G7	SOHO	1.0	–	–	70.33	73.94	0.0351	1997/04/08
C/1997 H4	SOHO	1.0	–	–	73.13	72.33	0.0356	1997/04/21
C/1997 H5	SOHO	1.0	–	–	79.18	69.13	0.0371	1997/04/29
C/1997 L2	SOHO	1.0	–	–	71.69	72.62	0.0381	1997/06/10
C/1997 O2	SOHO	1.0	–	–	71.92	73.07	0.0356	1997/07/25
C/1997 U8	SOHO	1.0	–	–	71.91	71.15	0.031	1997/10/19
C/1997 X7	SOHO	1.0	–	–	72.62	72.82	0.0346	1997/12/15
C/1998 G9	SOHO	1.0	–	–	84.26	67.91	0.037	1998/04/12
C/1998 V8	SOHO	1.0	–	–	72.01	72.88	0.0363	1998/11/03
C/1998 W7	SOHO	1.0	–	–	72.12	73.21	0.0362	1998/11/28
C/1999 F3	SOHO	1.0	–	–	73.31	72.36	0.0363	1999/03/17
C/1999 K16	SOHO	1.0	–	–	71.73	72.64	0.0339	1999/05/26
C/1999 L9	SOHO	1.0	–	–	70.73	70.16	0.038	1999/06/09
C/1999 P7	SOHO	1.0	–	–	71.32	73	0.0372	1999/08/13
C/2000 B8	SOHO	1.0	–	–	70.75	75.09	0.034	2000/01/16
C/2000 C2	SOHO	1.0	–	–	71.35	73.71	0.037	2000/02/03
C/2000 C5	SOHO	1.0	–	–	72.22	65.16	0.0358	2000/02/07
C/2000 J8	SOHO	1.0	–	–	72.5	73.65	0.0367	2000/05/06
C/2000 N4	SOHO	1.0	–	–	74.5	73.89	0.0351	2000/07/04
C/2000 X9	SOHO	1.0	–	–	72.66	73.96	0.0386	2000/12/03
C/2001 C7	SOHO	1.0	–	–	73.68	54.75	0.035	2001/02/11
C/2001 E1	SOHO	1.0	–	–	73.37	72.24	0.0357	2001/03/15
C/2001 K11	SOHO	1.0	–	–	72.36	73.28	0.0339	2001/05/16
C/2001 L10	SOHO	1.0	–	–	71.7	72.4	0.0355	2001/06/01
C/2001 R7	SOHO	1.0	–	–	73.77	85.28	0.0372	2001/09/12
C/2001 T1	SOHO	1.0	–	–	72.87	72.56	0.0364	2001/10/09
C/2001 V6	SOHO	1.0	–	–	69.76	73.64	0.0374	2001/11/02
C/2001 X8	SOHO	1.0	–	–	72.28	74.35	0.0371	2001/12/12
C/2001 X10	SOHO	1.0	–	–	73.46	73.79	0.036	2001/12/15
C/2002 A4	SOHO	1.0	–	–	72.13	75.45	0.0366	2002/01/01
C/2002 H8	SOHO	1.0	–	–	69.34	73.71	0.0336	2002/04/20
C/2002 P3	SOHO	1.0	–	–	73.84	75.81	0.0359	2002/08/12
C/2002 R8	SOHO	1.0	–	–	75.95	59.71	0.0343	2002/09/15
C/2002 T2	SOHO	1.0	–	–	70.94	70.73	0.0369	2002/10/04
C/2002 U6	SOHO	1.0	–	–	73.06	74.62	0.0359	2002/10/28
C/2002 V4	SOHO	1.0	–	–	72.5	74.75	0.0357	2002/11/09
C/2002 X6	SOHO	1.0	–	–	72.55	74.75	0.0346	2002/12/02
C/2002 Y2	SOHO	1.0	–	–	73.52	74.51	0.04	2002/12/19
C/2003 B1	SOHO	1.0	–	–	73.36	74.15	0.0355	2003/01/17
C/2003 H5	SOHO	1.0	–	–	71.35	75.17	0.0351	2003/04/27
C/2003 K5	SOHO	1.0	–	–	72.5	74.11	0.0348	2003/05/21
C/2003 K6	SOHO	1.0	–	–	71.87	73.67	0.0372	2003/05/30
C/2003 U4	SOHO	1.0	–	–	74.94	73.97	0.0357	2003/10/21
C/2003 W2	SOHO	1.0	–	–	73.26	74.96	0.0314	2003/11/29
C/2003 Y1	SOHO	1.0	–	–	72.81	74.7	0.0354	2003/12/20
C/2004 B2	SOHO	1.0	–	–	73.1	74.89	0.0353	2004/01/29
C/2004 C2	SOHO	1.0	–	–	72.92	74.6	0.0325	2004/02/05
C/2004 G2	SOHO	1.0	–	–	72.62	74.01	0.0383	2004/04/10
C/2004 H4	SOHO	1.0	–	–	67.87	74.62	0.0343	2004/04/16
C/2004 H5	SOHO	1.0	–	–	68.62	76.03	0.0335	2004/04/30
C/2004 T2	SOHO	1.0	–	–	73.67	72.45	0.0346	2004/10/09
C/2004 U3	SOHO	1.0	–	–	73.25	74.01	0.0375	2004/10/18
C/2005 B4	SOHO	1.0	–	–	71.69	71.69	0.0353	2005/01/30
C/2005 C1	SOHO	1.0	–	–	67.47	75.84	0.0392	2005/02/02
C/2005 H2	SOHO	1.0	–	–	78.83	72.43	0.0362	2005/04/17
C/2005 H9	SOHO	1.0	–	–	73.54	73.96	0.0352	2005/04/29
C/2005 K4	SOHO	1.0	–	–	73.25	74.48	0.0373	2005/05/16
C/2005 K9	SOHO	1.0	–	–	73.06	74.47	0.0354	2005/05/28
C/2005 O5	SOHO	1.0	–	–	74.41	67.93	0.0361	2005/07/26
C/2005 Q2	SOHO	1.0	–	–	74.51	76.48	0.0377	2005/08/23
C/2005 Q8	SOHO	1.0	–	–	72.42	77.2	0.0377	2005/08/25
C/2005 T9	SOHO	1.0	–	–	72.51	75.23	0.0368	2005/10/08
C/2005 W9	SOHO	1.0	–	–	72.63	73.13	0.037	2005/11/19
C/2005 W11	SOHO	1.0	–	–	76.08	72.71	0.0396	2005/11/20
C/2005 Y8	SOHO	1.0	–	–	73.75	74.29	0.0338	2005/12/25
C/2006 B4	SOHO	1.0	–	–	73.15	73.89	0.0345	2006/01/26
C/2006 F6	SOHO	1.0	–	–	74.13	75.03	0.0333	2006/03/23
C/2006 J5	SOHO	1.0	–	–	72.12	71.46	0.0387	2006/05/08
C/2006 R3	SOHO	1.0	–	–	75.14	66.29	0.0337	2006/09/02
C/2006 T6	SOHO	1.0	–	–	67.07	100.84	0.0353	2006/10/10
C/2006 U10	SOHO	1.0	–	–	71.68	74.91	0.0346	2006/10/20
C/2006 X10	SOHO	1.0	–	–	72.63	74.2	0.0348	2006/12/15
C/2007 A6	SOHO	1.0	–	–	70.57	70.67	0.0382	2007/01/11
C/2007 C10	SOHO	1.0	–	–	72.77	73.19	0.0351	2007/02/07
C/2007 F4	SOHO	1.0	–	–	71.41	76.09	0.0347	2007/03/28
C/2007 J1	SOHO	1.0	–	–	72.59	73.87	0.0348	2007/05/02
C/2007 K12	SOHO	1.0	–	–	72.52	73.94	0.0346	2007/05/18
C/2007 R10	SOHO	1.0	–	–	75.8	73.16	0.037	2007/09/15
C/2007 U7	SOHO	1.0	–	–	73.43	71.48	0.0325	2007/10/27
C/2007 V10	SOHO	1.0	–	–	76.95	73.51	0.035	2007/11/09
C/2007 X7	SOHO	1.0	–	–	71.98	73.58	0.0378	2007/12/10
C/2007 X14	SOHO	1.0	–	–	72.47	73.79	0.0345	2007/12/14
C/2007 Y8	SOHO	1.0	–	–	72.77	73.61	0.0344	2007/12/28
C/2008 D6	SOHO	1.0	–	–	70.85	72.5	0.0338	2008/02/19
C/2008 F1	SOHO	1.0	–	–	66.71	94.56	0.0318	2008/03/20
C/2008 H4	SOHO	1.0	–	–	73.46	72.35	0.0373	2008/04/18
C/2008 J10	SOHO	1.0	–	–	72.18	73.31	0.0369	2008/05/07
C/2008 J12	SOHO	1.0	–	–	70.94	71.57	0.0379	2008/05/08

Kracht group

This and the Marsden group, both are periodic, both with periods of approximately 3 years. They contain fewer members than the Meyer and Kreutz groups, probably as a result of their periodic nature, leading them to burn up more frequently. They are believed to be the parent bodies of the Southern Delta Aquariids meteor shower, occurring between July and August and usually having 15–20 meteors an hour.

Comet designation	Name	Eccentricity	Semimajor axis	Period	Inclination	Node	Perihelion distance	Perihelion date
C/1996 X3	SOHO	1.0	–	–	14.78	51	0.0426	1996/12/06
C/1996 X4	SOHO	1.0	–	–	13.7	50.79	0.0492	1996/12/06
C/1996 X5	SOHO	1.0	–	–	13.78	51.28	0.049	1996/12/06
C/1999 M3	SOHO	1.0	–	–	12.35	36.33	0.0441	1999/06/30
C/1999 N6	SOHO	1.0	–	–	12.15	32.5	0.0435	1999/07/12
C/2001 Q7	SOHO	1.0	–	–	13.28	43.95	0.0445	2001/08/21
C/2001 Q8	SOHO	1.0	–	–	13.07	44.76	0.0451	2001/08/24
C/2001 R8	SOHO	1.0	–	–	13.58	42.19	0.0437	2001/09/06
C/2001 R9	SOHO	1.0	–	–	12.47	48.9	0.0472	2001/09/07
C/2002 N2	SOHO	1.0	–	–	13.8	52.93	0.049	2002/07/11
C/2002 Q8	SOHO	1.0	–	–	13.7	50.38	0.0479	2002/08/25
C/2002 Q10	SOHO	1.0	–	–	13.54	50.99	0.0484	2002/08/27
C/2002 R5	SOHO	0.98526	3.21612	5.77	14.12	13.2	0.0474	2002/09/05
C/2002 S4	SOHO	1.0	–	–	13.51	50.81	0.0484	2002/09/18
C/2002 S5	SOHO	1.0	–	–	14.03	49.01	0.0467	2002/09/19
P/2002 S7	SOHO	0.98496	3.22344	5.79	13.6	50.3	0.04849	2002/09/21
C/2002 S11	SOHO	1.0	–	–	13.68	50.7	0.0482	2002/09/30
C/2004 A3	SOHO	1.0	–	–	14.75	44.75	0.0433	2004/01/16
C/2004 B3	SOHO	1.0	–	–	13.28	44.9	0.0515	2004/01/18
C/2004 J4	SOHO	1.0	–	–	12.35	34.3	0.0417	2004/05/05
C/2004 J12	SOHO	1.0	–	–	12.68	33.75	0.0398	2004/05/12
C/2004 J13	SOHO	1.0	–	–	12.47	36.12	0.0441	2004/05/13
C/2004 J15	SOHO	1.0	–	–	12.28	34.56	0.0438	2004/05/14
C/2004 J16	SOHO	1.0	–	–	14.63	34.39	0.0314	2004/05/14
C/2004 J17	SOHO	1.0	–	–	13.79	35.6	0.0356	2004/05/15
C/2004 J18	SOHO	1.0	–	–	11.89	34.23	0.0461	2004/05/15
C/2004 J20	SOHO	1.0	–	–	12.76	35.86	0.0419	2004/05/13
C/2004 L10	SOHO	1.0	–	–	12.54	35.76	0.0431	2004/06/14
342P/SOHO	SOHO	0.98260	3.04300	5.31	13.27	43.4	0.0529	2016/07/01
C/2008 E4	SOHO	1.0	–	–	13.13	51.85	0.0499	2008/03/03
C/2008 G6	SOHO	1.0	–	–	14.35	49.13	0.0483	2008/04/13

Marsden group

Ungrouped sungrazers

Comet designation	Name	Eccentricity	Semimajor axis	Period	Inclination	Node	Perihelion distance	Perihelion date
C/1680 V1	Great Comet of 1680	0.999986	444.4285	9370	60.6784	276.6339	0.006222	1680/12/18
C/1695 U1		1.0	–	–	93.589	286.018	0.0423	1695/10/23
C/1816 B1	Pons	1.0	–	–	43.111	325.829	0.0485	1816/03/01
C/1826 U1	Pons	1.0	–	–	90.6234	237.5505	0.026904	1826/11/18
C/1847 C1	Hind	0.99991	473.2556	10300	48.6636	23.824	0.042593	1847/03/30
C/1865 B1	Great Southern Comet	1.0	–	–	92.4945	254.8252	0.025844	1865/01/14
C/1961 O1	Wilson	0.999962	1057.8684	34410	24.2116	298.9545	0.040199	1961/07/17
C/1962 C1	Seki–Lines	1.000003	–	–	65.0142	304.6776	0.031397	1962/04/01
C/1996 V2	SOHO	1.0	–	–	33.41	89.36	0.0488	1996/11/11
C/1997 S4	SOHO	1.0	–	–	154.63	135.76	0.026	1997/09/29
C/1997 V7	SOHO	1.0	–	–	137.4	157.78	0.0216	1997/11/03
C/1998 G3	SOHO	1.0	–	–	53.86	322.5	0.0354	1998/04/12
C/1999 Y2	SOHO	1.0	–	–	111.42	235.5	0.0483	1999/12/28
C/2000 J2	SOHO	1.0	–	–	146.61	32.19	0.0335	2000/05/08
C/2000 V4	SOHO	1.0	–	–	54.97	324.91	0.0503	2000/11/11
C/2000 Y6	SOHO	1.0	–	–	87.3	229.47	0.0252	2000/12/20
C/2000 Y7	SOHO	1.0	–	–	89.02	228.93	0.0245	2000/12/20
C/2001 C5	SOHO	1.0	–	–	166.26	322.52	0.0256	2001/02/13
321P/SOHO	SOHO	0.98108	2.425409	3.78	20.1	165.2	0.04589	2016/04/10
C/2001 N1	SOHO	1.0	–	–	95.09	302.92	0.0052	2001/07/06
C/2001 P1	SOHO	1.0	–	–	29.9	140.14	0.0113	2001/08/05
C/2001 Q3	SOHO	1.0	–	–	106.63	155.03	0.0373	2001/08/26
C/2001 T5	SOHO	1.0	–	–	55.26	327.74	0.0476	2001/10/15
C/2002 G1	SOHO	1.0	–	–	133.92	106.02	0.0339	2002/04/02
C/2002 Q6	SOHO	1.0	–	–	65.96	70.92	0.0103	2002/08/23
C/2002 Q9	SOHO	1.0	–	–	22.45	19.58	0.0304	2002/08/19
C/2003 G3	SOHO	1.0	–	–	169.7	87.61	0.0168	2003/04/05
C/2003 H6	SOHO	1.0	–	–	27.05	243.47	0.0264	2003/04/30
C/2003 H7	SOHO	1.0	–	–	27.9	242.66	0.0266	2003/04/30
C/2003 K3	SOHO	1.0	–	–	39.529	79.076	0.13918	2003/06/01
C/2003 Q1	SOHO	1.0	–	–	29.33	43.43	0.032	2003/08/20
C/2003 Q6	SOHO	1.0	–	–	25.43	56.3	0.0366	2003/08/26
C/2003 R4	SOHO	1.0	–	–	92.36	173.06	0.0316	2003/09/06
C/2003 S9	SOHO	1.0	–	–	28.79	59.32	0.0154	2003/09/25
C/2004 Y10	SOHO	1.0	–	–	131.61	129.68	0.0322	2004/12/28
C/2005 C4	SOHO	1.0	–	–	40.06	7.79	0.0391	2005/02/13
C/2005 D1	SOHO	1.0	–	–	121.76	284.06	0.0468	2005/02/23
C/2007 C12	SOHO	1.0	–	–	122.22	285.89	0.0408	2007/02/09
C/2005 H7	SOHO	1.0	–	–	73.07	354.66	0.0127	2005/04/25
C/2005 M3	SOHO	1.0	–	–	88.99	140.98	0.0355	2005/06/19
C/2005 Q3	SOHO	1.0	–	–	43.52	70.89	0.0253	2005/08/30
C/2005 Q6	SOHO	1.0	–	–	50.4	156.59	0.0387	2005/08/19
C/2005 V8	SOHO	1.0	–	–	75.64	341.92	0.0266	2005/11/09
C/2006 K5	SOHO	1.0	–	–	117.6	169.23	0.0512	2006/05/23
C/2007 A7	SOHO	1.0	–	–	144.23	284.7	0.0191	2007/01/10
C/2007 C7	SOHO	1.0	–	–	70.99	309.4	0.0172	2007/02/02
C/2007 M8	SOHO	1.0	–	–	82.04	288.26	0.0478	2007/06/25
C/2007 X1	SOHO	1.0	–	–	129.2	156.13	0.0272	2007/12/03
C/2008 C3	SOHO	1.0	–	–	158.24	30.07	0.0346	2008/02/03
C/2008 E7	SOHO	1.0	–	–	143.28	12.08	0.0548	2008/03/05
323P/SOHO	SOHO	0.98173	2.610537	4.22	6.5	322.2	0.04770	2008/05/31
P/2008 Y12	SOHO	0.9787	3.07822	5.4	23.35	312.6	0.0654	2008/12/22
P/2015 D1	SOHO	0.9943	4.9	11	69.92	95.88	0.02832	2015/02/19

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