List of stars in Cepheus
# List of stars in Cepheus

This is the list of notable stars in the constellation Cepheus, sorted by decreasing brightness.

| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| - | - | - | - | - | - | - | - | - | - | - | - | - |
| α Cep | α | 5 | | 203280 | 105199 | $21^h$ $18^m$ $34.58^s$ | +62° 35′ 07.6″ | 2.45 | 1.58 | 49 | A7IV-V | Alderamin; suspected variable |
| γ Cep | γ | 35 | | 222404 | 116727 | $23^h$ $39^m$ $20.98^s$ | +77° 37′ 55.1″ | 3.21 | 2.51 | 45 | K1IV | Arrai; binary star; has a planet (b); suspected variable |
| β Cep | β | 8 | | 205021 | 106032 | $21^h$ $28^m$ $39.58^s$ | +70° 33′ 38.5″ | 3.23 | −3.08 | 595 | B2IIIv SB | Alfirk; prototype β Cep variable, $V_{max}$ = $3.16^m,$ $V_{min}$ = $3.27^m,$ P = 0.19 d |
| ζ Cep | ζ | 21 | | 210745 | 109492 | $22^h$ $10^m$ $51.26^s$ | +58° 12′ 04.5″ | 3.39 | −3.35 | 726 | K1Ibv SB | eclipsing binary |
| η Cep | η | 3 | | 198149 | 102422 | $20^h$ $45^m$ $17.27^s$ | +61° 50′ 12.5″ | 3.41 | 2.63 | 47 | K0IV | Al Kidr |
| ι Cep | ι | 32 | | 216228 | 112724 | $22^h$ $49^m$ $40.91^s$ | +66° 12′ 02.6″ | 3.50 | 0.76 | 115 | K0III | |
| δ Cep A | δ | 27 | | 213306 | 110991 | $22^h$ $29^m$ $10.25^s$ | +58° 24′ 54.7″ | 4.07 | −3.47 | 887 | F5Iab + B7-8 | prototype Cepheid variable, $V_{max}$ = $3.49^m,$ $V_{min}$ = $4.36^m,$ P = 5.37 d; binary star |
| ε Cep | ε | 23 | | 211336 | 109857 | $22^h$ $15^m$ $01.68^s$ | +57° 02′ 36.5″ | 4.18 | 2.13 | 84 | F0IV | δ Sct variable, $V_{max}$ = $4.15^m,$ $V_{min}$ = $4.21^m,$ P = 0.04 d |
| θ Cep | θ | 2 | | 195725 | 101093 | $20^h$ $29^m$ $34.83^s$ | +62° 59′ 38.9″ | 4.21 | 1.11 | 136 | A7III | Al Kidr |
| μ Cep | μ | | | 206936 | 107259 | $21^h$ $43^m$ $30.45^s$ | +58° 46′ 48.2″ | 4.23 | −6.81 | 5258 | M2Ia | Garnet Star; in Trumpler 37; semiregular variable, $V_{max}$ = $3.43^m,$ $V_{min}$ = $5.1^m,$ P = 835 d |
| 2 UMi | | (2) | | 5848 | 5372 | $01^h$ $08^m$ $44.16^s$ | +86° 15′ 25.6″ | 4.24 | −0.67 | 313 | K2II-III | |
| ν Cep | ν | 10 | | 207260 | 107418 | $21^h$ $45^m$ $26.93^s$ | +61° 07′ 14.9″ | 4.25 | −6.72 | 5094 | A2Ia | α Cyg variable, $V_{max}$ = $4.25^m,$ $V_{min}$ = $4.35^m$ |
| κ Cep | κ | 1 | | 192907 | 99255 | $20^h$ $08^m$ $53.32^s$ | +77° 42′ 40.9″ | 4.38 | −0.63 | 327 | B9III | triple star |
| π Cep | π | 33 | | 218658 | 114222 | $23^h$ $07^m$ $53.84^s$ | +75° 23′ 15.3″ | 4.41 | 0.27 | 220 | G2III | triple star |
| ξ Cep A | ξ | 17 | | 209790 | 108917 | $22^h$ $03^m$ $47.45^s$ | +64° 37′ 40.7″ | 4.45 | | 96 | Am | Kurhah, component of the ξ Cep system; spectroscopic binary |
| HR 7955 | | | | 198084 | 102431 | $20^h$ $45^m$ $21.20^s$ | +57° 34′ 49.1″ | 4.52 | 2.35 | 88 | F8IV-V | spectroscopic binary |
| 11 Cep | | 11 | | 206952 | 107119 | $21^h$ $41^m$ $55.08^s$ | +71° 18′ 40.3″ | 4.55 | 0.89 | 176 | K0III | |
| HD 217382 | | | | 217382 | 113116 | $22^h$ $54^m$ $24.38^s$ | +84° 20′ 46.0″ | 4.70 | −0.69 | 390 | K4III | variable star, ΔV = $0.004^m,$ P = 0.09 d |
| ο Cep | ο | 34 | | 219916 | 115088 | $23^h$ $18^m$ $37.41^s$ | +68° 06′ 41.1″ | 4.75 | 0.70 | 211 | K0III | multiple star; suspected variable |
| 9 Cep | | 9 | V337 | 206165 | 106801 | $21^h$ $37^m$ $55.23^s$ | +62° 04′ 55.0″ | 4.76 | −5.95 | 4528 | B2Ib | α Cyg variable, $V_{max}$ = $4.69^m,$ $V_{min}$ = $4.78^m$ |
| HD 216446 | | | | 216446 | 112519 | $22^h$ $47^m$ $28.95^s$ | +83° 09′ 13.4″ | 4.77 | −0.22 | 324 | K3III | double star |
| 24 Cep | | 24 | | 210807 | 109400 | $22^h$ $09^m$ $48.37^s$ | +72° 20′ 28.3″ | 4.79 | −0.53 | 377 | G8III | |
| 16 Cep | | 16 | | 209369 | 108535 | $21^h$ $59^m$ $15.10^s$ | +73° 10′ 49.0″ | 5.04 | 2.17 | 122 | F5V | double star |
| OV Cep | | 51 | OV | 51802 | 37391 | $07^h$ $40^m$ $31.09^s$ | +87° 01′ 12.6″ | 5.05 | −0.88 | 499 | M2III | semiregular variable, $V_{max}$ = $5.00^m,$ $V_{min}$ = $5.07^m$ |
| λ Cep | λ | 22 | | 210839 | 109556 | $22^h$ $11^m$ $30.58^s$ | +59° 24′ 52.3″ | 5.05 | −3.47 | 1646 | O6If(n) | emission-line star; suspected variable |
| HD 223274 | | | | 223274 | 117371 | $23^h$ $47^m$ $54.75^s$ | +67° 48′ 24.5″ | 5.05 | 0.25 | 297 | A1Vn | |
| 19 Cep | | 19 | | 209975 | 109017 | $22^h$ $05^m$ $08.79^s$ | +62° 16′ 47.4″ | 5.07 | −6.04 | 5433 | O9.5Ib | triple star |
| 31 Cep | | 31 | | 214470 | 111532 | $22^h$ $35^m$ $45.78^s$ | +73° 38′ 35.3″ | 5.08 | 1.32 | 184 | F3III-IV | |
| HD 30338 | | | | 30338 | 23265 | $05^h$ $00^m$ $20.72^s$ | +81° 11′ 38.5″ | 5.09 | −0.03 | 345 | K3III | |
| HD 25007 | | | | 25007 | 19461 | $04^h$ $10^m$ $02.79^s$ | +80° 41′ 55.2″ | 5.10 | −0.03 | 345 | G8III+... | double star |
| VV Cep | | | VV | 208816 | 108317 | $21^h$ $56^m$ $39.14^s$ | +63° 37′ 32.0″ | 5.11 | −6.93 | 8359 | M2 + B0 | Algol and semiregular variable, $V_{max}$ = $4.80^m,$ $V_{min}$ = $5.36^m,$ P = 7430 d; one of the largest stars known |
| 78 Dra | | (78) | | 207130 | 107230 | $21^h$ $43^m$ $04.13^s$ | +72° 19′ 12.7″ | 5.18 | 0.78 | 247 | K0III | |
| 6 Cep | | 6 | V382 | 203467 | 105268 | $21^h$ $19^m$ $22.21^s$ | +64° 52′ 18.6″ | 5.19 | −2.41 | 1079 | B3IVe | Be star, $V_{max}$ = $5.08^m,$ $V_{min}$ = $5.23^m$ |
| 30 Cep | | 30 | | 214734 | 111797 | $22^h$ $38^m$ $39.05^s$ | +63° 35′ 04.3″ | 5.19 | 0.23 | 320 | A3IV | |
| HD 210855 | | | | 210855 | 109572 | $22^h$ $11^m$ $48.52^s$ | +56° 50′ 20.6″ | 5.24 | 2.40 | 121 | F8V | |
| HD 218029 | | | | 218029 | 113864 | $23^h$ $03^m$ $32.85^s$ | +67° 12′ 33.1″ | 5.25 | −0.11 | 384 | K3III | |
| 18 Cep | | 18 | MO | 209772 | 108924 | $22^h$ $03^m$ $52.93^s$ | +63° 07′ 11.2″ | 5.26 | −0.43 | 448 | M5III | slow irregular variable, $V_{max}$ = $5.13^m,$ $V_{min}$ = $5.33^m$ |
| 20 Cep | | 20 | | 209960 | 109005 | $22^h$ $05^m$ $00.48^s$ | +62° 47′ 07.9″ | 5.27 | 0.32 | 318 | K4III | suspected variable |
| HD 212710 | | | | 212710 | 109693 | $22^h$ $13^m$ $10.17^s$ | +86° 06′ 28.3″ | 5.27 | 0.80 | 256 | B9.5Vn | |
| HD 210939 | | | | 210939 | 109592 | $22^h$ $12^m$ $02.01^s$ | +60° 45′ 32.7″ | 5.37 | 0.08 | 373 | K1III | |
| HD 26836 | | | | 26836 | 20776 | $04^h$ $27^m$ $02.89^s$ | +80° 49′ 27.2″ | 5.42 | −1.87 | 937 | G6III: | |
| 7 Cep | | 7 | | 204770 | 105972 | $21^h$ $27^m$ $46.16^s$ | +66° 48′ 32.9″ | 5.42 | −1.45 | 771 | B7V | |
| HD 19978 | | | | 19978 | 15547 | $03^h$ $20^m$ $19.58^s$ | +77° 44′ 05.6″ | 5.44 | 0.90 | 264 | A6V | suspected variable |
| $ρ^2$ Cep | $ρ^2$ | 29 | | 213798 | 111056 | $22^h$ $29^m$ $52.97^s$ | +78° 49′ 27.6″ | 5.45 | 1.14 | 237 | A3V | Al Kalb al Rai |
| HD 26659 | | | | 26659 | 20982 | $04^h$ $30^m$ $00.60^s$ | +83° 20′ 24.5″ | 5.47 | 0.63 | 304 | G8III | |
| HD 213022 | | | | 213022 | 110725 | $22^h$ $26^m$ $00.78^s$ | +70° 46′ 15.2″ | 5.47 | −0.54 | 520 | K2III | |
| HD 18438 | | | | 18438 | 14417 | $03^h$ $06^m$ $07.95^s$ | +79° 25′ 06.6″ | 5.49 | −1.15 | 695 | M1III | suspected variable |
| V408 Cep | | | V408 | 26356 | 20860 | $04^h$ $28^m$ $13.30^s$ | +83° 48′ 27.9″ | 5.51 | −1.10 | 685 | B5V | γ Cas variable |
| V381 Cep | | | V381 | 203338 | 105259 | $21^h$ $19^m$ $15.69^s$ | +58° 37′ 24.6″ | 5.51 | −4.74 | 3663 | M1Ibep | slow irregular variable, $V_{max}$ = $5.51^m,$ $V_{min}$ = $5.71^m$ |
| HD 210884 | | | | 210884 | 109474 | $22^h$ $10^m$ $38.90^s$ | +70° 07′ 57.1″ | 5.52 | 2.95 | 107 | F2V | |
| 26 Cep | | 26 | | 213087 | 110817 | $22^h$ $27^m$ $05.31^s$ | +65° 07′ 56.2″ | 5.52 | −3.93 | 2527 | B0.5Ib | suspected variable |
| HD 205139 | | | | 205139 | 106227 | $21^h$ $30^m$ $59.29^s$ | +60° 27′ 34.0″ | 5.53 | −3.80 | 2397 | B1II | |
| 12 Cep | | 12 | | 207528 | 107586 | $21^h$ $47^m$ $25.31^s$ | +60° 41′ 33.7″ | 5.53 | −0.25 | 467 | M1III | |
| HD 200205 | | | | 200205 | 103598 | $20^h$ $59^m$ $25.33^s$ | +59° 26′ 18.8″ | 5.54 | −0.73 | 586 | K4III | |
| 14 Cep | | 14 | LZ | 209481 | 108772 | $22^h$ $02^m$ $04.58^s$ | +58° 00′ 01.3″ | 5.55 | −5.22 | 4657 | O9V | rotating ellipsoidal variable |
| V388 Cep | | | V388 | 219586 | 114831 | $23^h$ $15^m$ $37.71^s$ | +70° 53′ 17.1″ | 5.56 | 0.36 | 356 | F0IV | δ Sct variable, ΔV = $0.07^m,$ P = 0.28 d |
| HD 221525 | | | | 221525 | 115746 | $23^h$ $26^m$ $59.92^s$ | +87° 18′ 26.8″ | 5.56 | 0.69 | 307 | A7IV | |
| HD 4853 | | | | 4853 | 4283 | $00^h$ $54^m$ $52.76^s$ | +83° 42′ 26.9″ | 5.59 | 1.21 | 245 | A4V | |
| 4 Cep | | 4 | | 197950 | 102253 | $20^h$ $43^m$ $10.98^s$ | +66° 39′ 26.5″ | 5.59 | 2.44 | 139 | A8V | |
| HD 6798 | | | | 6798 | 5626 | $01^h$ $12^m$ $16.51^s$ | +79° 40′ 26.3″ | 5.60 | 0.99 | 272 | A3V | |
| HD 220974 | | | | 220974 | 115770 | $23^h$ $27^m$ $16.42^s$ | +70° 21′ 35.3″ | 5.60 | 1.59 | 206 | A6IV | |
| HD 216380 | | | | 216380 | 112864 | $22^h$ $51^m$ $22.51^s$ | +61° 41′ 47.9″ | 5.61 | 1.39 | 227 | G2IV+... | |
| HD 20084 | | | | 20084 | 16489 | $03^h$ $32^m$ $19.72^s$ | +84° 54′ 40.9″ | 5.62 | 0.43 | 355 | G3IIp... | |
| HD 202214 | | | | 202214 | 104642 | $21^h$ $11^m$ $48.24^s$ | +59° 59′ 11.8″ | 5.64 | −6.58 | 9056 | B0V | suspected variable |
| HD 225216 | | | | 225216 | 379 | $00^h$ $04^m$ $41.84^s$ | +67° 09′ 59.0″ | 5.68 | 0.74 | 317 | K1III | |
| HD 208095 | | | | 208095 | 107930 | $21^h$ $52^m$ $01.02^s$ | +55° 47′ 48.3″ | 5.70 | −0.77 | 643 | B6IV-V | suspected variable |
| HD 214035 | | | | 214035 | 111242 | $22^h$ $32^m$ $16.27^s$ | +76° 13′ 35.3″ | 5.70 | −1.07 | 736 | A2V | |
| HD 206267 | | | | 206267 | 106886 | $21^h$ $38^m$ $57.62^s$ | +57° 29′ 20.6″ | 5.74 | −2.04 | 1173 | O6V((f))+O9V | in Trumpler 37; triple star; suspected variable |
| 13 Cep | | 13 | | 208501 | 108165 | $21^h$ $54^m$ $53.16^s$ | +56° 36′ 40.4″ | 5.74 | −3.71 | 2527 | B8Ibvar | suspected variable |
| 25 Cep | | 25 | | 211833 | 110103 | $22^h$ $18^m$ $12.59^s$ | +62° 48′ 15.7″ | 5.75 | −0.88 | 689 | K3III | |
| HD 211029 | | | | 211029 | 109620 | $22^h$ $12^m$ $22.45^s$ | +63° 17′ 27.9″ | 5.76 | −1.36 | 865 | M3III | variable star, ΔV = $0.021^m,$ P = 1.86 d |
| HR 774 | | | | 16458 | 13055 | $02^h$ $47^m$ $47.63^s$ | +81° 26′ 55.2″ | 5.80 | −0.12 | 498 | G8p... | Prototypical Barium star |
| HD 214710 | | | | 214710 | 111660 | $22^h$ $37^m$ $12.86^s$ | +75° 22′ 18.5″ | 5.80 | −0.61 | 623 | M1III | |
| HD 192781 | | | | 192781 | 99663 | $20^h$ $13^m$ $27.57^s$ | +60° 38′ 25.6″ | 5.81 | −0.49 | 594 | K5III | |
| HD 200614 | | | | 200614 | 103810 | $21^h$ $02^m$ $09.00^s$ | +56° 40′ 10.6″ | 5.83 | −0.92 | 729 | B8III | |
| $ρ^1$ Cep | $ρ^1$ | 28 | | 213403 | 110787 | $22^h$ $26^m$ $42.45^s$ | +78° 47′ 09.4″ | 5.83 | 1.85 | 204 | A2m | |
| HD 22701 | | | | 22701 | 19454 | $04^h$ $10^m$ $00.22^s$ | +86° 37′ 34.9″ | 5.84 | 2.78 | 133 | F5IV | |
| HD 208682 | | | | 208682 | 108226 | $21^h$ $55^m$ $30.99^s$ | +65° 19′ 14.9″ | 5.84 | −2.00 | 1203 | B2.5Ve | suspected variable |
| HD 221861 | | | | 221861 | 116380 | $23^h$ $34^m$ $59.03^s$ | +71° 38′ 31.4″ | 5.86 | −3.86 | 2860 | K0Ib | |
| HD 201636 | | | | 201636 | 104171 | $21^h$ $06^m$ $23.39^s$ | +71° 25′ 55.5″ | 5.88 | 2.42 | 160 | F3IV | |
| HD 211554 | | | | 211554 | 109972 | $22^h$ $16^m$ $26.51^s$ | +57° 13′ 12.8″ | 5.88 | −0.86 | 728 | G8III | |
| HD 217157 | | | | 217157 | 112833 | $22^h$ $51^m$ $02.94^s$ | +85° 22′ 24.5″ | 5.89 | 0.16 | 457 | K5 | |
| HD 219485 | | | | 219485 | 114745 | $23^h$ $14^m$ $37.02^s$ | +74° 13′ 52.5″ | 5.89 | 0.16 | 455 | A0V | |
| V414 Cep | | | V414 | 197939 | 102358 | $20^h$ $44^m$ $22.04^s$ | +56° 29′ 18.3″ | 5.91 | −1.45 | 964 | M3III | semiregular variable |
| 77 Dra | | (77) | | 201908 | 104105 | $21^h$ $05^m$ $29.21^s$ | +78° 07′ 34.8″ | 5.91 | 0.40 | 412 | B8Vn | |
| HD 18778 | | | | 18778 | 14844 | $03^h$ $11^m$ $42.85^s$ | +81° 28′ 14.6″ | 5.92 | 1.96 | 202 | A7III-IV | suspected variable |
| HD 203399 | | | | 203399 | 104968 | $21^h$ $15^m$ $42.39^s$ | +77° 00′ 44.1″ | 5.92 | −1.12 | 836 | K5III | suspected variable |
| HD 207198 | | | | 207198 | 107374 | $21^h$ $44^m$ $53.28^s$ | +62° 27′ 38.1″ | 5.94 | −3.01 | 2012 | O9II | |
| HD 222386 | | | | 222386 | 116714 | $23^h$ $39^m$ $10.16^s$ | +75° 17′ 34.3″ | 5.95 | 1.42 | 263 | A3V | |
| HD 223128 | | | | 223128 | 117265 | $23^h$ $46^m$ $36.73^s$ | +66° 46′ 56.1″ | 5.95 | −2.68 | 1734 | B2IV | |
| HD 209112 | | | | 209112 | 108505 | $21^h$ $58^m$ $53.51^s$ | +62° 41′ 52.6″ | 5.96 | −2.02 | 1283 | M3III | variable star, ΔV = $0.020^m,$ P = 1.76 d |
| HD 205072 | | | | 205072 | 105727 | $21^h$ $24^m$ $49.40^s$ | +80° 31′ 29.5″ | 5.97 | 0.78 | 355 | G6III: | |
| HD 222387 | | | | 222387 | 116728 | $23^h$ $39^m$ $21.17^s$ | +74° 00′ 09.4″ | 5.98 | 0.43 | 419 | G8III | |
| HD 200039 | | | | 200039 | 103219 | $20^h$ $54^m$ $44.28^s$ | +75° 55′ 31.7″ | 5.99 | 0.37 | 434 | G5III | |
| HD 202987 | | | | 202987 | 105080 | $21^h$ $17^m$ $14.23^s$ | +55° 47′ 52.7″ | 6.00 | −2.28 | 1475 | K3III | |
| HD 431 | | | | 431 | 760 | $00^h$ $09^m$ $19.83^s$ | +79° 42′ 52.7″ | 6.01 | 0.67 | 381 | A7IV | |
| HD 213973 | | | | 213973 | 111314 | $22^h$ $33^m$ $02.70^s$ | +69° 54′ 48.1″ | 6.01 | 1.60 | 249 | A9III | |
| HD 216595 | | | | 216595 | 112998 | $22^h$ $53^m$ $03.77^s$ | +60° 06′ 03.7″ | 6.01 | −1.99 | 1299 | K2V: | |
| HD 197373 | | | | 197373 | 102011 | $20^h$ $40^m$ $17.88^s$ | +60° 30′ 17.3″ | 6.02 | 3.41 | 108 | F6IV | |
| HD 12005 | | | | 12005 | 9568 | $02^h$ $02^m$ $57.04^s$ | +77° 54′ 58.6″ | 6.04 | −1.55 | 1076 | K0 | |
| HD 212495 | | | | 212495 | 110498 | $22^h$ $23^m$ $00.50^s$ | +62° 25′ 09.6″ | 6.04 | −0.66 | 712 | A1V | |
| HD 12467 | | | | 12467 | 10054 | $02^h$ $09^m$ $25.44^s$ | +81° 17′ 45.3″ | 6.05 | 1.87 | 223 | A1V | |
| HD 8065 | | | | 8065 | 6522 | $01^h$ $23^m$ $46.82^s$ | +78° 43′ 33.8″ | 6.07 | −8.93 | 32600 | A0Iab | suspected variable |
| HD 216102 | | | | 216102 | 112635 | $22^h$ $48^m$ $44.24^s$ | +62° 56′ 18.7″ | 6.07 | −0.39 | 639 | K0 | |
| HD 206842 | | | | 206842 | 107197 | $21^h$ $42^m$ $45.37^s$ | +59° 16′ 15.0″ | 6.10 | −3.26 | 2433 | K1III | |
| HD 203574 | | | | 203574 | 105370 | $21^h$ $20^m$ $33.50^s$ | +60° 45′ 23.2″ | 6.11 | 0.51 | 429 | G5III | |
| V426 Cep | | | V426 | 204599 | 105949 | $21^h$ $27^m$ $25.30^s$ | +59° 45′ 00.4″ | 6.11 | −1.28 | 982 | M3II-III... | slow irregular variable |
| HD 211300 | | | | 211300 | 109659 | $22^h$ $12^m$ $52.72^s$ | +73° 18′ 25.7″ | 6.11 | −1.05 | 881 | A3V+... | suspected variable |
| HD 203501 | | | | 203501 | 104756 | $21^h$ $13^m$ $21.60^s$ | +81° 13′ 51.5″ | 6.12 | 0.14 | 512 | A3IV | |
| HD 211242 | | | | 211242 | 109746 | $22^h$ $13^m$ $49.71^s$ | +63° 09′ 44.5″ | 6.13 | −1.23 | 967 | B8Vn | |
| HD 204754 | | | | 204754 | 106052 | $21^h$ $28^m$ $52.72^s$ | +55° 25′ 07.2″ | 6.14 | −1.13 | 929 | B8III | |
| HD 36905 | | | | 36905 | 28532 | $06^h$ $01^m$ $20.17^s$ | +85° 10′ 55.6″ | 6.17 | −1.89 | 1336 | M0III | |
| HD 197734 | | | | 197734 | 102216 | $20^h$ $42^m$ $39.69^s$ | +60° 36′ 04.9″ | 6.17 | −0.56 | 724 | A2IV | |
| HD 208606 | | | | 208606 | 108209 | $21^h$ $55^m$ $20.60^s$ | +61° 32′ 30.5″ | 6.17 | −6.05 | 9056 | G8Ib... | |
| HD 207780 | | | | 207780 | 107723 | $21^h$ $49^m$ $19.01^s$ | +61° 16′ 22.1″ | 6.18 | −0.96 | 872 | M1II-III | suspected variable |
| HD 212454 | | | | 212454 | 110497 | $22^h$ $23^m$ $00.17^s$ | +57° 17′ 04.6″ | 6.18 | −0.90 | 851 | B8III-IV | |
| HD 216172 | | | | 216172 | 112670 | $22^h$ $49^m$ $00.68^s$ | +68° 34′ 12.2″ | 6.19 | 2.21 | 204 | F5 | |
| HD 6319 | | | | 6319 | 5928 | $01^h$ $16^m$ $12.60^s$ | +87° 08′ 44.0″ | 6.20 | 1.20 | 326 | K2III: | |
| HD 218560 | | | | 218560 | 114227 | $23^h$ $07^m$ $57.20^s$ | +64° 13′ 21.2″ | 6.21 | −1.36 | 1065 | K0 | |
| HD 199661 | | | | 199661 | 103346 | $20^h$ $56^m$ $17.01^s$ | +56° 53′ 15.0″ | 6.23 | −0.71 | 795 | B2.5IV | suspected variable |
| HD 6473 | | | | 6473 | 5412 | $01^h$ $09^m$ $12.29^s$ | +80° 00′ 42.0″ | 6.24 | 0.46 | 468 | K0 | |
| HD 218537 | | | | 218537 | 114212 | $23^h$ $07^m$ $47.74^s$ | +63° 38′ 00.5″ | 6.25 | −1.62 | 1221 | B3V | suspected variable |
| HD 214019 | | | | 214019 | 111325 | $22^h$ $33^m$ $16.76^s$ | +70° 22′ 25.3″ | 6.26 | 0.82 | 400 | A0V | |
| HD 7238 | | | | 7238 | 5947 | $01^h$ $16^m$ $31.04^s$ | +79° 54′ 35.5″ | 6.27 | 1.98 | 236 | F5Vs | |
| HD 210905 | | | | 210905 | 109585 | $22^h$ $11^m$ $56.74^s$ | +59° 05′ 03.8″ | 6.29 | 1.16 | 345 | K0III | |
| HD 213232 | | | | 213242 | 110919 | $22^h$ $28^m$ $19.48^s$ | +64° 05′ 06.8″ | 6.30 | 0.99 | 377 | K0 | |
| V398 Cep | | | V398 | 225136 | 302 | $00^h$ $03^m$ $51.63^s$ | +66° 42′ 43.9″ | 6.31 | −1.09 | 985 | M4 | semiregular variable |
| δ Cep C | δ | 27 | | 213307 | 110988 | $22^h$ $29^m$ $09.23^s$ | +58° 24′ 14.7″ | 6.30 | | 887 | B7IV | Component of the δ Cep system; spectroscopic binary; suspected variable |
| HD 209258 | | | | 209258 | 108420 | $21^h$ $57^m$ $51.07^s$ | +74° 59′ 48.3″ | 6.32 | −1.35 | 1113 | K5 | suspected variable |
| V379 Cep | | | V379 | 197770 | 102258 | $20^h$ $43^m$ $13.69^s$ | +57° 06′ 50.4″ | 6.32 | −5.10 | 6269 | B2III | Algol variable, ΔV = $0.047^m,$ P = 99.76 d |
| HD 215907 | | | | 215907 | 112508 | $22^h$ $47^m$ $23.23^s$ | +58° 28′ 58.8″ | 6.33 | −1.01 | 956 | B9.5IV | |
| ξ Cep B | ξ | 17 | | 209791 | | $22^h$ $03^m$ $46.22^s$ | +64° 37′ 41.5″ | 6.34 | | 96 | F8V | component of the ξ Cep system; spectroscopic binary |
| HD 210220 | | | | 210220 | 109190 | $22^h$ $07^m$ $09.65^s$ | +58° 50′ 26.8″ | 6.34 | 0.16 | 560 | G6III | |
| HD 1141 | | | | 1141 | 1296 | $00^h$ $16^m$ $13.88^s$ | +76° 57′ 02.7″ | 6.35 | −0.04 | 617 | B9Vn | |
| HD 219841 | | | | 219841 | 114984 | $23^h$ $17^m$ $18.86^s$ | +75° 17′ 56.5″ | 6.35 | −0.07 | 628 | A2Vs | |
| 80 Dra | | (80) | | 210873 | 109434 | $22^h$ $10^m$ $15.32^s$ | +72° 06′ 40.7″ | 6.36 | 0.38 | 511 | B9MNp... | |
| HR 9038 | | | | 223778 | 117712 | $23^h$ $52^m$ $24.52^s$ | +75° 32′ 40.2″ | 6.36 | 6.19 | 35 | K3V | |
| HD 208132 | | | | 208132 | 107893 | $21^h$ $51^m$ $37.25^s$ | +65° 45′ 09.9″ | 6.37 | 1.86 | 260 | Am+... | |
| HD 3440 | | | | 3440 | 3132 | $00^h$ $39^m$ $47.75^s$ | +82° 29′ 36.9″ | 6.38 | 3.83 | 105 | F6V: | |
| HD 202582 | | | | 202582 | 104788 | $21^h$ $13^m$ $42.46^s$ | +64° 24′ 15.1″ | 6.38 | 3.30 | 135 | G2IV+... | suspected variable |
| V444 Cep | | | V444 | 210071 | 109124 | $22^h$ $06^m$ $13.55^s$ | +56° 20′ 36.2″ | 6.38 | 0.14 | 576 | A0III | rotating ellipsoidal variable |
| HD 25904 | | | | 25904 | 20039 | $04^h$ $17^m$ $51.85^s$ | +80° 32′ 08.7″ | 6.39 | −0.92 | 945 | K0 | |
| HD 208947 | | | | 208947 | 108364 | $21^h$ $57^m$ $11.09^s$ | +66° 09′ 22.2″ | 6.41 | −2.06 | 1614 | B2V | |
| V421 Cep | | | V421 | 203025 | 105091 | $21^h$ $17^m$ $18.79^s$ | +58° 36′ 41.4″ | 6.42 | −3.03 | 2527 | B2III | Be star |
| V422 Cep | | | V422 | 203265 | 105193 | $21^h$ $18^m$ $32.43^s$ | +61° 11′ 03.8″ | 6.43 | −2.03 | 1606 | M3 | slow irregular variable |
| V438 Cep | | | V438 | 209111 | 108133 | $21^h$ $54^m$ $26.54^s$ | +80° 18′ 30.9″ | 6.43 | −0.59 | 825 | M3 | semiregular variable |
| RW Cep | | | RW | 212466 | 110504 | $22^h$ $23^m$ $07.02^s$ | +55° 57′ 47.6″ | 6.44 | −3.18 | 2739 | G8Ia | semiregular variable, $V_{max}$ = $6.0^m,$ $V_{min}$ = $7.3^m,$ P = 346 d; one of the largest stars known |
| HD 12918 | | | | 12918 | 10623 | $02^h$ $16^m$ $45.27^s$ | +83° 33′ 41.5″ | 6.45 | 0.86 | 428 | K0 | |
| HD 198781 | | | | 198781 | 102771 | $20^h$ $49^m$ $17.39^s$ | +64° 02′ 32.2″ | 6.45 | −3.03 | 2567 | B0.5V | suspected variable |
| HD 207636 | | | | 207636 | 107555 | $21^h$ $47^m$ $00.87^s$ | +70° 09′ 03.4″ | 6.45 | 0.55 | 492 | A0V | |
| HD 215588 | | | | 215588 | 112324 | $22^h$ $45^m$ $03.70^s$ | +58° 08′ 50.6″ | 6.45 | 3.68 | 117 | F5 | |
| HD 12927 | | | | 12927 | 10309 | $02^h$ $12^m$ $49.98^s$ | +79° 41′ 29.3″ | 6.46 | 0.96 | 410 | A3 | suspected variable |
| HD 212136 | | | | 212136 | 110314 | $22^h$ $20^m$ $38.77^s$ | +58° 24′ 35.5″ | 6.46 | 0.15 | 597 | G8III | |
| HD 217348 | | | | 217348 | 113498 | $22^h$ $59^m$ $09.00^s$ | +59° 48′ 52.8″ | 6.46 | −1.29 | 1156 | B9III | |
| V431 Cep | | | V431 | 205938 | 106604 | $21^h$ $35^m$ $25.91^s$ | +68° 13′ 09.3″ | 6.47 | 0.08 | 617 | Ap Si | α² CVn variable |
| HD 207826 | | | | 207826 | 107710 | $21^h$ $49^m$ $08.12^s$ | +66° 47′ 31.9″ | 6.49 | 1.57 | 314 | F3IV | |
| HD 224890 | | | | 224890 | 128 | $00^h$ $01^m$ $39.30^s$ | +73° 36′ 42.8″ | 6.50 | 2.41 | 214 | Am... | |
| HD 32196 | | | | 32196 | 25911 | $05^h$ $31^m$ $48.00^s$ | +85° 56′ 19.4″ | 6.50 | 1.51 | 324 | A5m | |
| HD 198236 | | | | 198236 | 102370 | $20^h$ $44^m$ $33.08^s$ | +69° 45′ 06.8″ | 6.50 | 0.89 | 431 | G8III | |
| V Cep | | | V | 224309 | 118027 | $23^h$ $56^m$ $27.56^s$ | +83° 11′ 28.0″ | 6.57 | 1.75 | 301 | A3V | not variable |
| V419 Cep | | | V419 | 202380 | 104719 | $21^h$ $12^m$ $47.25^s$ | +60° 05′ 52.8″ | 6.62 | | 5200 | M2Ib | slow irregular variable |
| 79 Dra | | (79) | | 208509 | 107995 | $21^h$ $52^m$ $46.94^s$ | +73° 42′ 08.2″ | 6.65 | 2.21 | 276 | A2V | |
| 15 Cep | | 15 | | 209744 | 108925 | $22^h$ $03^m$ $53.86^s$ | +59° 48′ 52.5″ | 6.69 | −1.43 | 1370 | B1V | multiple star |
| AH Cep | | | AH | 216014 | 112562 | $22^h$ $47^m$ $52.94^s$ | +65° 03′ 43.8″ | 6.88 | | 3330 | B0.5V+... | β Lyr variable, $V_{max}$ = $6.78^m,$ $V_{min}$ = $7.07^m,$ P = 1.77 d |
| U Cep | | | U | 5679 | 4843 | $01^h$ $02^m$ $18.34^s$ | +81° 52′ 32.1″ | 6.90 | 0.32 | 674 | G8III | Algol variable, $V_{max}$ = $6.75^m,$ $V_{min}$ = $9.24^m,$ P = 2.49 d |
| HD 12648 | | | | 12648 | 10800 | $02^h$ $19^m$ $00.0^s$ | +85° 44′ 10″ | 6.98 | | 517 | G5 | has a planet (b) |
| HD 202432 | | | | 202432 | 104632 | $21^h$ $11^m$ $40.4^s$ | +70° 26′ 28″ | 7.00 | | 525 | K2 D | has a planet (b) |
| EM Cep | | | EM | 208392 | 108073 | $21^h$ $53^m$ $48.10^s$ | +62° 36′ 51.9″ | 7.03 | | 1610 | B1Vn | W UMa variable, $V_{max}$ = $7.02^m,$ $V_{min}$ = $7.17^m,$ P = 0.81 d |
| SS Cep | | | SS | 22689 | 17881 | $03^h$ $49^m$ $30.01^s$ | +80° 19′ 20.9″ | 7.16 | | 847 | M5III | semiregular variable, $V_{max}$ = $6.5^m,$ $V_{min}$ = $7.7^m,$ P = 90 d |
| DQ Cep | | | DQ | 199908 | 103471 | $20^h$ $57^m$ $48.61^s$ | +55° 29′ 15.6″ | 7.26 | | 579 | F1IV | δ Sct variable, $V_{max}$ = $7.22^m,$ $V_{min}$ = $7.32^m,$ P = 0.079 d |
| HD 204521 | | | | 204521 | 105766 | $21^h$ $25^m$ $16.80^s$ | +70° 28′ 39.1″ | 7.29 | | 86 | G0V_Fe-08 | Will pass near the Sun in the future |
| HD 207538 | | | | 207538 | 107598 | $21^h$ $47^m$ $39.79^s$ | +59° 12′ 01.3″ | 7.30 | | | O9.7IV | peculiar metal abundances |
| T Cep | | | T | 202012 | 104451 | $21^h$ $09^m$ $32.00^s$ | +68° 29′ 25.0″ | 7.33 | | 612 | M6-9e | Mira variable, $V_{max}$ = $5.2^m,$ $V_{min}$ = $11.3^m,$ P = 388.14 d |
| V380 Cep | | | V380 | 200775 | 103763 | $21^h$ $01^m$ $36.92^s$ | +68° 09′ 47.8″ | 7.36 | | 1720 | B2Ve | in NGC 7023; Orion variable, $V_{max}$ = $7.24^m,$ $V_{min}$ = $7.42^m$ |
| VW Cep | | | VW | 197433 | 101750 | $20^h$ $37^m$ $21.54^s$ | +75° 36′ 01.5″ | 7.38 | | 90 | G8V+K0V | W UMa variable, $V_{max}$ = $7.23^m,$ $V_{min}$ = $7.68^m,$ P = 0.28 d |
| S Cep | | | S | 206362 | 106583 | $21^h$ $25^m$ $12.83^s$ | +78° 37′ 28.2″ | 7.40 | | 1330 | C7,4e | Mira variable, $V_{max}$ = $7.4^m,$ $V_{min}$ = $12.9^m,$ P = 486.84 d |
| HD 1 | | | | 1 | 422 | $00^h$ $05^m$ $08.84^s$ | +67° 50′ 23.97″ | 7.42 | -0.01 | 1,190 | G9-K0IIIa | spectroscopic binary |
| NY Cep | | | NY | 217312 | 113461 | $22^h$ $58^m$ $39.80^s$ | +63° 04′ 37.7″ | 7.44 | | | B0IV | Algol variable, $V_{max}$ = $7.4^m,$ $V_{min}$ = $7.55^m,$ P = 15.28 d |
| V368 Cep | | | V368 | 220140 | 115147 | $23^h$ $19^m$ $26.63^s$ | +79° 00′ 12.7″ | 7.54 | | 63 | G9V | RS CVn variable |
| W Cep | | | W | 214369 | 111592 | $22^h$ $36^m$ $27.56^s$ | +58° 25′ 33.9″ | 7.59 | | | K0Iapev... | semiregular variable, $V_{max}$ = $7.02^m,$ $V_{min}$ = $8.5^m,$ P = 350 d |
| EI Cep | | | EI | 205234 | 106024 | $21^h$ $28^m$ $28.21^s$ | +76° 24′ 12.6″ | 7.61 | | 657 | F3V+F1m | Algol variable, $V_{max}$ = $7.54^m,$ $V_{min}$ = $8.06^m,$ P = 8.44 d |
| CW Cep | | | CW | 218066 | 113907 | $23^h$ $04^m$ $02.22^s$ | +63° 23′ 48.8″ | 7.67 | | 2080 | B0.5V+B1V | in Cepheus OB3; Algol variable, $V_{max}$ = $7.6^m,$ $V_{min}$ = $8.04^m,$ P = 2.73 d |
| IR Cep | | | IR | 208960 | 108426 | $21^h$ $57^m$ $51.93^s$ | +61° 01′ 07.9″ | 7.86 | | 2200 | G0 | classical Cepheid, $V_{max}$ = $7.58^m,$ $V_{min}$ = $7.98^m,$ P = 2.11 d |
| EK Cep | | | EK | 206821 | 107083 | $21^h$ $41^m$ $21.50^s$ | +69° 41′ 34.1″ | 7.89 | | 528 | A0V | Algol variable |
| HD 204827 | | | | 204827 | 106059 | $21^h$ $28^m$ $57.76^s$ | +58° 44′ 23.2″ | 7.94 | | | O9V+B0.5III | in Trumpler 37; spectroscopic binary |
| XZ Cep | | | XZ | | 111257 | $22^h$ $32^m$ $25.08^s$ | +67° 09′ 02.5″ | 8.51 | | 1730 | O9.5V | β Lyr variable, $V_{max}$ = $8^m,$ $V_{min}$ = $8.83^m,$ P = 5.10 d |
| HD 211810 | | | | 211810 | 110094 | $22^h$ $18^m$ $07.0^s$ | +61° 08′ 04″ | 8.59 | | 199 | G5 | has a planet (b) |
| ZZ Cep | | | ZZ | 215661 | 112317 | $22^h$ $45^m$ $02.61^s$ | +68° 07′ 58.4″ | 8.60 | | 430 | B7v+... | Algol variable, $V_{max}$ = $8.6^m,$ $V_{min}$ = $9.55^m,$ P = 2.14 d |
| DH Cep | | | DH | 215835 | 112470 | $22^h$ $46^m$ $54.11^s$ | +58° 05′ 03.5″ | 8.61 | | 5000 | O5.5V+O6V | in NGC 7380; rotating ellipsoidal variable, $V_{max}$ = $8.58^m,$ $V_{min}$ = $8.62^m,$ P = 2.11 d |
| CQ Cep | | | CQ | 214419 | 111633 | $22^h$ $36^m$ $53.95^s$ | +56° 54′ 21.0″ | 8.80 | | | WN6+O9II-Ib | β Lyr variable, $V_{max}$ = $8.63^m,$ $V_{min}$ = $9.12^m,$ P = 1.64 d |
| WX Cep | | | WX | 213631 | 111166 | $22^h$ $31^m$ $15.79^s$ | +63° 31′ 23.6″ | 9.00 | | 1520 | A5V+A2V | Algol variable, $V_{max}$ = $8.7^m,$ $V_{min}$ = $9.29^m,$ P = 3.38 d |
| HD 211853 | | | GP | 211853 | 100154 | $22^h$ $18^m$ $45.61^s$ | +56° 07′ 33.9″ | 9.00 | | 1450 | WN6o+O6I | eclipsing binary, $V_{max}$ = $8.96^m,$ $V_{min}$ = $9.07^m,$ P = 6.69 d |
| XX Cep | | | XX | 222217 | 116648 | $23^h$ $38^m$ $20.29^s$ | +64° 20′ 02.7″ | 9.18 | | 799 | A7V | Algol variable, $V_{max}$ = $9.20^m,$ $V_{min}$ = $10.32^m,$ P = 2.34 d |
| RZ Cep | | | RZ | | 111839 | $22^h$ $39^m$ $13.18^s$ | +64° 51′ 30.6″ | 9.19 | | | A0-F2 | RR Lyr variable, $V_{max}$ = $9.15^m,$ $V_{min}$ = $9.72^m,$ P = 0.31 d |
| IL Cep | | | IL | | 113017 | $22^h$ $53^m$ $15.60^s$ | +62° 08′ 45.0″ | 9.31 | | 2790 | B3IVe+A3 | UX Ori star, $V_{max}$ = $9.24^m,$ $V_{min}$ = $9.61^m$ |
| EG Cep | | | EG | 194089 | | $20^h$ $15^m$ $56.83^s$ | +76° 48′ 35.7″ | 9.49 | | | A7V | β Lyr variable, $V_{max}$ = $9.31^m,$ $V_{min}$ = $10.21^m,$ P = 0.54 d |
| Kruger 60 A | | | | 239960 | 110893 | $22^h$ $27^m$ $59.47^s$ | +57° 41′ 45.2″ | 9.59 | 11.58 | 13.1 | M2.0V | one of the nearest known stars; member of the Kruger 60 system |
| HIP 109384 | | | | | 109384 | $22^h$ $08^m$ $32.0^s$ | +71° 18′ 52″ | 9.63 | | 183 | G5 | has a planet (b) |
| CR Cep | | | CR | 240059 | 112430 | $22^h$ $46^m$ $24.77^s$ | +59° 26′ 31.9″ | 9.64 | | 1760 | G0 | classical Cepheid, $V_{max}$ = $9.43^m,$ $V_{min}$ = $9.83^m,$ P = 6.23 d |
| PQ Cep | | | PQ | | | $21^h$ $44^m$ $28.78^s$ | +73° 38′ 04.9″ | 9.82 | | | C6-,3e | Mira variable |
| HD 219460 | | | V458 | 219460 | 114791 | $23^h$ $15^m$ $12.39^s$ | +60° 27′ 01.8″ | 9.89 | | | WN5+B1III | Wolf–Rayet star |
| 4U 2206+54 | | | | | | $23^h$ $07^m$ $56.24^s$ | +54° 31′ 06.4″ | 9.90 | | | O9.5Vep | high-mass X-ray binary, $V_{max}$ = $9.7^m,$ $V_{min}$ = $9.9^m$ |
| SV Cep | | | SV | | | $22^h$ $21^m$ $33.20^s$ | +73° 40′ 27.1″ | 10.35 | | | A2IVe | UX Ori star, $V_{max}$ = $10.35^m,$ $V_{min}$ = $12.15^m$ |
| V354 Cephei | | | V354 | | | $22^h$ $33^m$ $35^s$ | +58° 53′ 45″ | 10.90 | | 9000 | M2.5 Iab | One of the largest known stars; slow irregular variable, $V_{max}$ = $10.82^m,$ $V_{min}$ = $11.35^m$ |
| DO Cep | | | DO | 239960 | | $22^h$ $27^m$ $59.57^s$ | +57° 41′ 45.3″ | 10.30 | | 13.1 | M4.0V | member of the Kruger 60 system; flare star, $V_{max}$ = $10.3^m,$ $V_{min}$ = $11.4^m$ |
| CP Cep | | | CP | | 108427 | $21^h$ $57^m$ $52.69^s$ | +56° 09′ 50.1″ | 10.58 | | 1360 | F5Ib | classical Cepheid, $V_{max}$ = $10.06^m,$ $V_{min}$ = $10.96^m,$ P = 17.86 d |
| AK Cep | | | AK | | 110964 | $22^h$ $28^m$ $50.09^s$ | +58° 12′ 39.4″ | 10.86 | | 713 | F8 | classical Cepheid, $V_{max}$ = $10.86^m,$ $V_{min}$ = $11.52^m,$ P = 7.23 d |
| EE Cep | | | EE | | | $23^h$ $09^m$ $22.76^s$ | +55° 45′ 24.2″ | 10.9 | | | B5:nev | Algol variable, $V_{max}$ = $10.72^m,$ $V_{min}$ = $12.15^m,$ P = 2049.53 d |
| BH Cep | | | BH | | | $22^h$ $01^m$ $42.87^s$ | +69° 44′ 36.5″ | 11.01 | | | F5IIIe | UX Ori star, $V_{max}$ = $10.79^m,$ $V_{min}$ = $12.7^m$ |
| GW Cep | | | GW | | | $01^h$ $45^m$ $58.58^s$ | +80° 04′ 55.3″ | 11.21 | | | G3 | W UMa variable |
| WZ Cep | | | WZ | | | $23^h$ $22^m$ $24.22^s$ | +72° 54′ 56.7″ | 11.23 | | | F5 | W UMa variable |
| BO Cep | | | BO | | | $22^h$ $16^m$ $54.06^s$ | +70° 03′ 45.0″ | 11.55 | | | F5Ve | UX Ori star, $V_{max}$ = $11.5^m,$ $V_{min}$ = $12.4^m$ |
| WR 152 | | | | 211564 | | $22^h$ $16^m$ $24.04^s$ | +55° 37′ 36.7″ | 11.61 | | | WN3 | Wolf–Rayet star |
| DI Cep | | | DI | | 113269 | $22^h$ $56^m$ $11.53^s$ | +58° 40′ 01.8″ | 11.95 | | 797 | G8IVe | T Tauri star |
| CX Cep | | | CX | | | $22^h$ $09^m$ $33.44^s$ | +57° 44′ 30.5″ | 12.12 | | | WN4+O5V | β Lyr variable, $V_{max}$ = $12.09^m,$ $V_{min}$ = $12.24^m,$ P = 2.13 d |
| Wolf 1106 | | | | | | $21^h$ $07^m$ $55.40^s$ | +59° 43′ 19.3″ | 13.23 | | 79 | sdM1.5 | One of first three subdwarfs discovered |
| Cepheus X-4 | | | V490 | | | $21^h$ $39^m$ $30.68^s$ | +56° 59′ 10.5″ | | | | B1.5Ve | in IC 1396; high-mass X-ray binary |
| V350 Cep | | | V350 | | | $20^h$ $43^m$ $00.01^s$ | +66° 11′ 28.0″ | 16.20 | | M2... | WN4+O5V | in NGC 7129; T Tauri star |
| PV Cep | | | PV | | | $20^h$ $45^m$ $53.94^s$ | +67° 57′ 38.7″ | 17.46 | | | A5 | in nebula GM 1-29; EXor |
| IV Cep | | | IV | | | $22^h$ $04^m$ $36.92^s$ | +53° 30′ 23.7″ | | | | | nova |
| Cepheus A HW 2 | | | | | | $22^h$ $56^m$ $17.9^s$ | +62° 01′ 49″ | | | | B0.5 | in Cepheus A; massive protostar |
| S140 IRS 1 | | | | | | $22^h$ $19^m$ $18.28^s$ | +63° 18′ 45.8″ | | | | | in S140; protostar |
| IRAS 21391+5802 | | | | | | $21^h$ $40^m$ $42.36^s$ | +58° 16′ 09.7″ | | | | | in IC 1396N; protostar |
| NGC 7538 IRS 1 | | | | | | $23^h$ $13^m$ $45.32^s$ | +61° 28′ 11.7″ | | | | O | in NGC 7538; massive protostar |
| NGC 7538 IRS 9 | | | | | | $23^h$ $14^m$ $01.63^s$ | +61° 27′ 20.2″ | | | | | in NGC 7538; massive protostar |
| OH 104.9+2.4 | | | | | | $22^h$ $19^m$ $27.48^s$ | +59° 51′ 21.7″ | | | | | OH/IR star |
| PSR B2224+65 | | | | | | $22^h$ $25^m$ $52.36^s$ | +65° 35′ 33.8″ | | | | | pulsar |
| PSR J2229+6114 | | | | | | $22^h$ $29^m$ $04.97^s$ | +61° 14′ 12.9″ | | | | | pulsar |
| Table legend:  • Name = Proper name  • B = Bayer designation  • F or/and G. = Flamsteed designation or Gould designation  • Var = Variable star designation  • HD = Henry Draper Catalogue designation number  • HIP = Hipparcos Catalogue designation number  • RA = Right ascension for the Epoch/Equinox J2000.0  • Dec = Declination for the Epoch/Equinox J2000.0  • vis. mag. = visual magnitude (m or $m_v),$ also known as apparent magnitude  • abs. mag. = absolute magnitude $(M_v)$  • Dist. (ly) = Distance in light-years from Earth  • Sp. class = Spectral class of the star in the stellar classification system  • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] |||||||||||||
