| Designation | Apps | Arc | Notes | Predictions (T) |
| D/1766 G1 (Helfenzrieder) | 1 | 17660308-17660315 | uncertain orbit, possibly perturbed by Jupiter after 1766, cf. Kronk | - |
| D/1770 L1 (Lexell) | 1 | 17700615-17701003 | perturbed by Jupiter (1779) into a different, larger orbit (even ejection from the solar system is possible), cf. Kronk | Kinoshita |
| D/1783 W1 (Pigott) | 1? | 17831119-17831221 | possibly rediscovered in January 2003 by LINEAR as P/2003 A1, unambiguous link still not possible, see also Kronk | Nakano (2003), Kinoshita |
| D/1819 W1 (Blanpain) | 1 | 18191214-18200115 | possibly identified with 2003 WY25 | Kinoshita |
| D/1827 M1 (Pons-Gambart) | 1 | 18270621-18270714 | uncertain orbital period, cf. Kronk, Kammerer, Kasten, Yoshida | Muraoka (1997), Nakano (2015), Hasegawa/Nakano (2022) |
| D/1884 O1 (Barnard 1) | 1 | 18840724-18841108 | outburst, possible secondary nucleus, cf. Kronk, q slightly increased | Nakano (2005), Kinoshita |
| D/1886 K1 (Brooks 1) | 1 | 18860525-18860703 | uncertain period, q increased from 1.3 AU to 1.9 AU | Nakano (2005), Kinoshita |
| D/1892 T1 (Barnard 3) | 1 | 18921014-18921208 | intrinsically faint, q increased from 1.43 AU to 1.56 AU | Nakano (2005), Kinoshita |
| D/1894 F1 (Denning) | 1 | 18940327-18940605 | intrinsically faint, q decreased slightly | Nakano (2007), Muraoka (1999), Kinoshita |
| D/1895 Q1 (Swift) | 1 | 18950824-18960206 | several perturbations by Jupiter, q increased from 1.3 AU to 1.5 AU | Nakano (2003), Muraoka (1996) |
| D/1896 R2 (Giacobini) | 1 | 18960904-18970105 | possible secondary nucleus, cf. Kronk, q increased slightly | Muraoka (1995), Kinoshita |
| D/1918 W1 (Schorr) | 1 | 19181123-19181231 | q increased from 1.9 AU to about 3 AU | Nakano (2007), Muraoka (1999), Kinoshita |
| D/1921 H1 (Dubiago) | 1 | 19210424-19210611 | - | - |
| D/1952 B1 (Harrington-Wilson) | 1 | 19520130-19520225 | intrinsically faint, q increased from 1.65 AU to 1.9 AU | Nakano (2004), Muraoka (1998), Kinoshita |
| D/1960 S1 (van Houten) | 1 | 19600924-19601026 | q inreases from 3.95 AU to < 4.2 AU | Meyer (2011/2012), Sitarski (1976), Kinoshita |
| D/1977 C1 (Skiff-Kosai) | 1 | 19770213-19770312 | q decreased slightly | Nakano (2006), Muraoka (1999), Kinoshita |
| D/1978 R1 (Haneda-Campos) | 1 | 19780730-19781129 | intrinsically faint, cf. Kronk, q increased from 1.1 AU to 1.3 AU | Nakano (2004), Muraoka (1997), Kinoshita |
| 3D/Biela | 6 | 1846-1852 | disintegrated | Nakano (2005), Nakano (2006), Nakano (2005), Muraoka (1997), Kinoshita |
| 5D/Brorsen | 5 | 1873-1879 | brightness decline at last apparition (1879), afterwards several approaches to Jupiter | Nakano (2006), Muraoka (1995), Kinoshita |
| 18D/Perrine-Mrkos | 5 | 1961-1969 | outbursts | Nakano (2002), Muraoka (2002), Kinoshita |
| 20D/Westphal | 2 | 1852-1913 | decline in brightness in 1913, probably disintegrated | Kazimirchak-Polonskaya (1975), Kinoshita |
| 25D/Neujmin | 2 | 1916-1927 | asymmetric lightcurve, q decreased slightly | Nakano (2003), Muraoka (2003), Kinoshita |
| 34D/Gale | 2 | 1927-1938 | outbursts | Nakano (2004), Muraoka (2004), Kinoshita |
| 72P/Denning-Fujikawa | 2 | 1881-1978 | intrinsically faint, outbursts | Muraoka (1996), Kinoshita |