List of stars in Cepheus


This is the list of notable stars in the constellation Cepheus, sorted by decreasing brightness.
NameBFVarHDHIPRADecvis.
mag.
abs.
mag.
Dist. Sp. classNotes
α Cepα52032801051992.451.5849A7IV-VAlderamin; suspected variable
γ Cepγ352224041167273.212.5145K1IVErrai; binary star; has a planet ; suspected variable
β Cepβ82050211060323.23−3.08595B2IIIv SBAlfirk; prototype β Cep variable,
ζ Cepζ212107451094923.39−3.35726K1Ibv SBeclipsing binary
η Cepη31981491024223.412.6347K0IVAl Kidr
ι Cepι322162281127243.500.76115K0III
δ Cep Aδ272133061109914.07−3.47887F5Iab + B7-8prototype Cepheid variable, ; binary star
ε Cepε232113361098574.182.1384F0IVδ Sct variable,
θ Cepθ21957251010934.211.11136A7IIIAl Kidr
μ Cepμ2069361072594.23−6.815258M2IaGarnet Star; in Trumpler 37; semiregular variable,
2 UMiω584853724.24−0.67313K2II-IIITarandus
ν Cepν102072601074184.25−6.725094A2Iaα Cyg variable,
κ Cepκ1192907992554.38−0.63327B9IIItriple star
π Cepπ332186581142224.410.27220G2IIItriple star
ξ Cep Aξ172097901089174.4596AmKurhah, component of the ξ Cep system; spectroscopic binary
HR 7955υ1980841024314.522.3588F8IV-Vspectroscopic binary
11 Cepτ112069521071194.550.89176K0III
HD 2173822173821131164.70−0.69390K4IIIvariable star,
ο Cepο342199161150884.750.70211K0IIImultiple star; suspected variable
9 Cep9V3372061651068014.76−5.954528B2Ibα Cyg variable,
HD 2164462164461125194.77−0.22324K3IIIdouble star
24 Cepφ242108071094004.79−0.53377G8III
16 Cep162093691085355.042.17122F5Vdouble star
OV Cep51OV51802373915.05−0.88499M2IIIsemiregular variable,
λ Cepλ222108391095565.05−3.471646O6Ifemission-line star; suspected variable
HD 223274ψ2232741173715.050.25297A1Vn
19 Cep192099751090175.07−6.045433O9.5Ibtriple star
31 Cep312144701115325.081.32184F3III-IV
HD 3033830338232655.09−0.03345K3III
HD 2500725007194615.10−0.03345G8III+...double star
VV CepVV2088161083175.11−6.938359M2 + B0Algol and semiregular variable, ; one of the largest stars known
78 Dra2071301072305.180.78247K0III
6 Cep6V3822034671052685.19−2.411079B3IVeBe star,
30 Cep302147341117975.190.23320A3IV
HD 2108552108551095725.242.40121F8V
HD 2180292180291138645.25−0.11384K3III
18 Cepχ18MO2097721089245.26−0.43448M5IIIslow irregular variable,
20 Cep202099601090055.270.32318K4IIIsuspected variable
HD 2127102127101096935.270.80256B9.5Vn
HD 2109392109391095925.370.08373K1III
HD 2683626836207765.42−1.87937G6III:
7 Cep72047701059725.42−1.45771B7V
HD 1997819978155475.440.90264A6Vsuspected variable
ρ2 Cepρ2292137981110565.451.14237A3VAl Kalb al Rai
HD 2665926659209825.470.63304G8III
HD 2130222130221107255.47−0.54520K2III
HD 1843818438144175.49−1.15695M1IIIsuspected variable
V408 CepV40826356208605.51−1.10685B5Vγ Cas variable
V381 CepV3812033381052595.51−4.743663M1Ibepslow irregular variable,
HD 2108842108841094745.522.95107F2V
26 Cep262130871108175.52−3.932527B0.5Ibsuspected variable
HD 2051392051391062275.53−3.802397B1II
12 Cep122075281075865.53−0.25467M1III
HD 2002052002051035985.54−0.73586K4III
14 Cep14LZ2094811087725.55−5.224657O9Vrotating ellipsoidal variable
V388 CepV3882195861148315.560.36356F0IVδ Sct variable,
HD 2215252215251157465.560.69307A7IV
HD 4853485342835.591.21245A4V
4 Cep41979501022535.592.44139A8V
HD 6798679856265.600.99272A3V
HD 2209742209741157705.601.59206A6IV
HD 2163802163801128645.611.39227G2IV+...
HD 2008420084164895.620.43355G3IIp...
HD 2022142022141046425.64−6.589056B0Vsuspected variable
HD 2252162252163795.680.74317K1III
HD 2080952080951079305.70−0.77643B6IV-Vsuspected variable
HD 2140352140351112425.70−1.07736A2V
HD 2062672062671068865.74−2.041173O6V)+O9Vin Trumpler 37; triple star; suspected variable
13 Cep132085011081655.74−3.712527B8Ibvarsuspected variable
25 Cep252118331101035.75−0.88689K3III
HD 2110292110291096205.76−1.36865M3IIIvariable star,
HR 77416458130555.80−0.12498G8p...Prototypical Barium star
HD 2147102147101116605.80−0.61623M1III
HD 192781192781996635.81−0.49594K5III
HD 2006142006141038105.83−0.92729B8III
ρ1 Cepρ1282134031107875.831.85204A2m
HD 2270122701194545.842.78133F5IV
HD 2086822086821082265.84−2.001203B2.5Vesuspected variable
HD 2218612218611163805.86−3.862860K0Ib
HD 2016362016361041715.882.42160F3IV
HD 2115542115541099725.88−0.86728G8III
HD 2171572171571128335.890.16457K5
HD 2194852194851147455.890.16455A0V
V414 CepV4141979391023585.91−1.45964M3IIIsemiregular variable
77 Dra2019081041055.910.40412B8Vn
HD 1877818778148445.921.96202A7III-IVsuspected variable
HD 2033992033991049685.92−1.12836K5IIIsuspected variable
HD 2071982071981073745.94−3.012012O9II
HD 2223862223861167145.951.42263A3V
HD 2231282231281172655.95−2.681734B2IV
HD 2091122091121085055.96−2.021283M3IIIvariable star,
HD 2050722050721057275.970.78355G6III:
HD 2223872223871167285.980.43419G8III
HD 2000392000391032195.990.37434G5III
HD 2029872029871050806.00−2.281475K3III
HD 4314317606.010.67381A7IV
HD 2139732139731113146.011.60249A9III
HD 2165952165951129986.01−1.991299K2V:
HD 1973731973731020116.023.41108F6IV
HD 120051200595686.04−1.551076K0
HD 2124952124951104986.04−0.66712A1V
HD 1246712467100546.051.87223A1V
HD 8065806565226.07−8.9332600A0Iabsuspected variable
HD 2161022161021126356.07−0.39639K0
HD 2068422068421071976.10−3.262433K1III
HD 2035742035741053706.110.51429G5III
V426 CepV4262045991059496.11−1.28982M3II-III...slow irregular variable
HD 2113002113001096596.11−1.05881A3V+...suspected variable
HD 2035012035011047566.120.14512A3IV
HD 2112422112421097466.13−1.23967B8Vn
HD 2047542047541060526.14−1.13929B8III
HD 3690536905285326.17−1.891336M0III
HD 1977341977341022166.17−0.56724A2IV
HD 2086062086061082096.17−6.059056G8Ib...
HD 2077802077801077236.18−0.96872M1II-IIIsuspected variable
HD 2124542124541104976.18−0.90851B8III-IV
HD 2161722161721126706.192.21204F5
HD 6319631959286.201.20326K2III:
HD 2185602185601142276.21−1.361065K0
HD 1996611996611033466.23−0.71795B2.5IVsuspected variable
HD 6473647354126.240.46468K0
HD 2185372185371142126.25−1.621221B3Vsuspected variable
HD 2140192140191113256.260.82400A0V
HD 7238723859476.271.98236F5Vs
HD 2109052109051095856.291.16345K0III
HD 2132322132421109196.300.99377K0
V398 CepV3982251363026.31−1.09985M4semiregular variable
δ Cep Cδ272133071109886.30887B7IVComponent of the δ Cep system; spectroscopic binary; suspected variable
HD 2092582092581084206.32−1.351113K5suspected variable
V379 CepV3791977701022586.32−5.106269B2IIIAlgol variable,
HD 2159072159071125086.33−1.01956B9.5IV
ξ Cep Bξ172097916.3496F8Vcomponent of the ξ Cep system; spectroscopic binary
HD 2102202102201091906.340.16560G6III
HD 1141114112966.35−0.04617B9Vn
HD 2198412198411149846.35−0.07628A2Vs
80 Dra2108731094346.360.38511B9MNp...
HR 90382237781177126.366.1935K3V
HD 2081322081321078936.371.86260Am+...
HD 3440344031326.383.83105F6V:
HD 2025822025821047886.383.30135G2IV+...suspected variable
V444 CepV4442100711091246.380.14576A0IIIrotating ellipsoidal variable
HD 2590425904200396.39−0.92945K0
HD 2089472089471083646.41−2.061614B2V
V421 CepV4212030251050916.42−3.032527B2IIIBe star
V422 CepV4222032651051936.43−2.031606M3slow irregular variable
V438 CepV4382091111081336.43−0.59825M3semiregular variable
RW CepRW2124661105046.44−3.182739G8Iasemiregular variable, ; one of the largest stars known
HD 1291812918106236.450.86428K0
HD 1987811987811027716.45−3.032567B0.5Vsuspected variable
HD 2076362076361075556.450.55492A0V
HD 2155882155881123246.453.68117F5
HD 1292712927103096.460.96410A3suspected variable
HD 2121362121361103146.460.15597G8III
HD 2173482173481134986.46−1.291156B9III
V431 CepV4312059381066046.470.08617Ap Siα² CVn variable
HD 2078262078261077106.491.57314F3IV
HD 2248902248901286.502.41214Am...
HD 3219632196259116.501.51324A5m
HD 1982361982361023706.500.89431G8III
V CepV2243091180276.571.75301A3Vnot variable
V419 CepV4192023801047196.625200M2Ibslow irregular variable
79 Dra2085091079956.652.21276A2V
15 Cepσ152097441089256.69−1.431370B1Vmultiple star
AH CepAH2160141125626.883330B0.5V+...β Lyr variable,
U CepU567948436.900.32674G8IIIAlgol variable,
HD 1264812648108006.98517G5has a planet
HD 2024322024321046327.00525K2 Dhas a planet
EM CepEM2083921080737.031610B1VnW UMa variable,
SS CepSS22689178817.16847M5IIIsemiregular variable,
DQ CepDQ1999081034717.26579F1IVδ Sct variable,
HD 2045212045211057667.2986G0V_Fe-08Will pass near the Sun in the future
HD 2075382075381075987.30O9.7IVpeculiar metal abundances
T CepT2020121044517.33612M6-9eMira variable,
V380 CepV3802007751037637.361720B2Vein NGC 7023; Orion variable,
VW CepVW1974331017507.3890G8V+K0VW UMa variable,
S CepS2063621065837.401330C7,4eMira variable,
HD 114227.42-0.011,190G9-K0IIIaspectroscopic binary
NY CepNY2173121134617.44B0IVAlgol variable,
V368 CepV3682201401151477.5463G9VRS CVn variable
W CepW2143691115927.59K0Iapev...semiregular variable,
EI CepEI2052341060247.61657F3V+F1mAlgol variable,
CW CepCW2180661139077.672080B0.5V+B1Vin Cepheus OB3; Algol variable,
IR CepIR2089601084267.862200G0classical Cepheid,
EK CepEK2068211070837.89528A0VAlgol variable
HD 2048272048271060597.94O9V+B0.5IIIin Trumpler 37; spectroscopic binary
XZ CepXZ1112578.511730O9.5Vβ Lyr variable,
HD 2118102118101100948.59199G5has a planet
ZZ CepZZ2156611123178.60430B7v+...Algol variable,
DH CepDH2158351124708.615000O5.5V+O6Vin NGC 7380; rotating ellipsoidal variable,
CQ CepCQ2144191116338.80WN6+O9II-Ibβ Lyr variable,
WX CepWX2136311111669.001520A5V+A2VAlgol variable,
HD 211853GP2118531001549.001450WN6o+O6Ieclipsing binary,
XX CepXX2222171166489.18799A7VAlgol variable,
RZ CepRZ1118399.19A0-F2RR Lyr variable,
IL CepIL1130179.312790B3IVe+A3UX Ori star,
EG CepEG1940899.49A7Vβ Lyr variable,
Kruger 60 A2399601108939.5911.5813.1M2.0Vone of the nearest known stars; member of the Kruger 60 system
HIP 1093841093849.63183G5has a planet
CR CepCR2400591124309.641760G0classical Cepheid,
PQ CepPQ9.82C6-,3eMira variable
HD 219460V4582194601147919.89WN5+B1IIIWolf–Rayet star
4U 2206+549.90O9.5Vephigh-mass X-ray binary,
SV CepSV10.35A2IVeUX Ori star,
V354 CepheiV35410.909000M2.5 IabOne of the largest known stars; slow irregular variable,
DO CepDO23996010.3013.1M4.0Vmember of the Kruger 60 system; flare star,
CP CepCP10842710.581360F5Ibclassical Cepheid,
AK CepAK11096410.86713F8classical Cepheid,
EE CepEE10.9B5:nevAlgol variable,
BH CepBH11.01F5IIIeUX Ori star,
GW CepGW11.21G3W UMa variable
WZ CepWZ11.23F5W UMa variable
BO CepBO11.55F5VeUX Ori star,
WR 15221156411.61WN3Wolf–Rayet star
DI CepDI11326911.95797G8IVeT Tauri star
CX CepCX12.12WN4+O5Vβ Lyr variable,
Wolf 110613.2379sdM1.5One of first three subdwarfs discovered
Cepheus X-4V490B1.5Vein IC 1396; high-mass X-ray binary
V350 CepV35016.20M2...WN4+O5Vin NGC 7129; T Tauri star
PV CepPV17.46A5in nebula GM 1-29; EXor
FR CepFRClassical Cepheid Variable
IV CepIVnova
Cepheus A HW 2B0.5in Cepheus A; massive protostar
S140 IRS 1in S140; protostar
IRAS 21391+5802in IC 1396N; protostar
NGC 7538 IRS 1Oin NGC 7538; massive protostar
NGC 7538 IRS 9in NGC 7538; massive protostar
OH 104.9+2.4OH/IR star
PSR B2224+65pulsar
PSR J2229+6114pulsar

; Notes