Artist's concept of an "uneven ring of dust" orbiting KIC 8462852, also known as Tabby's Star

This list of stars that have unusual dimming periods is a table of stars that have been observed to darken and brighten and do not appear to be eclipsing binaries or intrinsic variables. It is based on studies searching for analogs of Tabby's Star.[1][2]

The listing here is ordered alphabetically.

List

Tabby's Star (KIC 8462852) – Consolidated plot of all known dimmings (1 March 2020)
Star designation Stellar
class 		Magnitude Right ascension
(J2000) 		Declination
(J2000) 		Distance
(light-years) 		Reason for dimming
Apparent Absolute
ASASSN-V J193622.23+115244.1 — 14.0–15.5[3] — 19h 36m 22.23s[3] +11° 52′ 44.1″[3] 6592[3] Unknown
ASASSN-V J213939.3-702817.4 F0V[4] 12.95–14.22[5] 2.5[5] 21h 39m 39.3s[5] −70° 28′ 17.4″[5] 3630[4] Unknown
Betelgeuse M1-2[6] +0.50[7] — 05h 55m 10.30536s[8] +07° 24′ 25.4304″[8] — "large-grain circumstellar dust"[9][10]
EPIC 204278916 M1[11] 13.7[12] — 16h 02m 07.576s[13] −22° 57′ 46.89″[13] — Dust disk
EPIC 204376071 M[14] — — 16h 04m 10.1267s[15] −22° 34′ 45.5503″[15] 440[14] Possibly giant planet or brown dwarf with rings
HD 139139
(EPIC 249706694) 		G3/5V 9.84;[16] 9.677[17] — 15h 37m 06.215s[17] −19° 08′ 32.96″[17] 350[18]
572[17] 		Unknown
KH 15D K7[19] 15.5–21.5[20] 6.226[21] 06h 41m 10.31s[22] +09° 28′ 33.2″[22] 773[23] Possibly circumbinary disk
KIC 4150611
(HD 181469) 		Pulsator/K/M/G — — 19h 18m 58.21759s[24] +39° 16′ 01.7913″[24] — Five-star system
PDS 110 keF6 IVeb[25] 10.422[25] 2.54[25] 05h 23m 31.008s[25] –01° 04′ 23.68″[25] 1090[25] Possibly giant planet or brown dwarf with disc of dust or large ring system
RW Cephei K2 0-Ia[26] 6.0–7.6[27] — 22h 23m 07.01521s[28] +55° 57′ 47.6244″[28] 11,000[29][a] Unknown
RZ Piscium K0 IV[30] 11.29–13.82[30] — 01h 09m 42.056s[31] +27° 57′ 1.95″[31] 550[32] Substantial mass of gas and dust, possibly from disrupted planet
Tabby's Star
(KIC 8462852) 		F3V[33][34] 11.705[34] 3.08[33] 20h 06m 15.4527s[33] +44° 27′ 24.791″[33] 1470[33] Unknown
TIC 400799224 — — — — — — "probably from an orbiting body that periodically emits clouds of dust that occult the star"[35][36]
V1400 Centauri K5 IV(e) Li[37] 12.31[37] — 14h 07m 47.93s[37] −39° 45′ 42.7″[37] 434[38] Planet with gigantic ring system
VVV-WIT-07 — 14.35–16.164[39] — 17h 26m 29.387s[39] −35° 40′ 6.20″[39] 23000/?[39] Unknown
WD 1145+017
(EPIC 201563164) 		DB[40] 17.0[41] — 11h 48m 33.63s[40] +01° 28′ 59.4″[40] 570[42] Dust disk
ZTF J0139+5245
(ZTF J013906.17+524536.89) 		DA[43] 18.4[43] — 01h 39m 06.17s +52° 45′ 36.89″ 564[43] Dust disk
Gaia17bpp M0-III 16.13 - 20.48[44] — 19h 37m 23.16s +17° 59′ 02.90 27,600[45] Dust disk

See also

Notes

  1. ^ Assuming membership to Cepheus OB1

References

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