Knowledge (XXG)

Kepler-89e

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548: 585: 614: 272: 578: 27: 619: 571: 49: 609: 70: 488:"False Positive Probabilities for Allkeplerobjects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives" 426:
Weiss, Lauren M; et al. (2013). "The Mass of KOI-94d and a Relation for Planet Radius, Mass, and Incident Flux".
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0.3046 ± 0.0040 AU (45,570,000 ± 600,000 km)
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Kepler-89e orbits the star Kepler-89. Kepler-89 has a mass of 1.18
440: 295: 373: 291: 279: 219: 174: 365: 319: 101: 559: 282:, and giving it the appearance of a larger version of 380:
of 6,210 K, making it appear bright yellowish-white.
228: 200: 173: 153: 148: 138: 117: 107: 90: 80: 68: 61: 47: 39: 26: 21: 364:. It is 3.3 billion years old, younger than the 579: 8: 554:This extrasolar-planet-related article is a 16: 310:6.56 times that of the Earth. It orbits an 586: 572: 521: 503: 439: 486:Morton, Timothy D.; et al. (2016). 481: 479: 477: 475: 421: 419: 417: 415: 413: 322:, making its orbit smaller than that of 411: 409: 407: 405: 403: 401: 399: 397: 395: 393: 389: 15: 234:584 K (311 °C; 592 °F) 7: 544: 542: 558:. You can help Knowledge (XXG) by 14: 546: 318:(au), with a period of 54.32031 1: 615:Exoplanets discovered in 2013 636: 541: 523:10.3847/0004-637X/822/2/86 458:10.1088/0004-637X/768/1/14 345: 278:, making it cloudless and 492:The Astrophysical Journal 428:The Astrophysical Journal 312:F-type main-sequence star 306:, 0.60 g/cm, giving it a 238: 93:Orbital period (sidereal) 294:around 35 times that of 255:in the constellation of 149:Physical characteristics 314:at a distance of 0.305 63:Orbital characteristics 620:Cygnus (constellation) 376:old (3 Gyr). It has a 326:'s. It has a very low 610:Transiting exoplanets 372:about 3,000,000,000 514:2016ApJ...822...86M 450:2013ApJ...768...14W 330:of 0.019. It has a 298:. It has a similar 271:It is classed as a 267:Physical properties 40:Discovery date 18: 316:astronomical units 99:54.32031 ± 0.00012 28:Discovered by 567: 566: 242: 241: 627: 588: 581: 574: 550: 543: 536: 535: 525: 507: 483: 470: 469: 443: 423: 247:, also known as 218: 217: 216: 188: 187: 186: 134: 133: 132: 122: 100: 50:Detection method 32:Lauren M. Weiss 19: 635: 634: 630: 629: 628: 626: 625: 624: 605:Exoplanet stubs 595: 594: 593: 592: 540: 539: 485: 484: 473: 425: 424: 391: 386: 350: 344: 269: 214: 212: 211: 209: 206: 195: 192: 184: 182: 181: 179: 168: 165: 158: 130: 128: 127: 125: 118: 98: 95: 73: 71:Semi-major axis 52: 12: 11: 5: 633: 631: 623: 622: 617: 612: 607: 597: 596: 591: 590: 583: 576: 568: 565: 564: 551: 538: 537: 471: 388: 387: 385: 382: 346:Main article: 343: 340: 268: 265: 240: 239: 236: 235: 232: 226: 225: 207: 201: 198: 197: 193: 190: 177: 171: 170: 166: 163: 159: 154: 151: 150: 146: 145: 140: 136: 135: 123: 120:Semi-amplitude 115: 114: 111: 105: 104: 96: 91: 88: 87: 84: 78: 77: 74: 69: 66: 65: 59: 58: 56:Transit method 53: 48: 45: 44: 41: 37: 36: 30: 24: 23: 13: 10: 9: 6: 4: 3: 2: 632: 621: 618: 616: 613: 611: 608: 606: 603: 602: 600: 589: 584: 582: 577: 575: 570: 569: 563: 561: 557: 552: 549: 545: 533: 529: 524: 519: 515: 511: 506: 501: 497: 493: 489: 482: 480: 478: 476: 472: 467: 463: 459: 455: 451: 447: 442: 437: 433: 429: 422: 420: 418: 416: 414: 412: 410: 408: 406: 404: 402: 400: 398: 396: 394: 390: 383: 381: 379: 375: 371: 368:, making its 367: 363: 359: 355: 349: 341: 339: 337: 333: 329: 325: 321: 317: 313: 309: 305: 301: 297: 293: 289: 285: 281: 277: 274: 266: 264: 262: 258: 254: 250: 246: 237: 233: 231: 227: 224: 221: 208: 205: 199: 196: 178: 176: 172: 169: 160: 157: 152: 147: 144: 141: 137: 124: 121: 116: 112: 110: 106: 103: 97: 94: 89: 85: 83: 79: 75: 72: 67: 64: 60: 57: 54: 51: 46: 42: 38: 35: 31: 29: 25: 20: 560:expanding it 553: 495: 491: 431: 427: 354:solar masses 351: 328:eccentricity 270: 259:. It orbits 248: 244: 243: 161:6.56 ± 0.62 113:89.76 ± 0.15 86:0.019 ± 0.23 82:Eccentricity 43:9 March 2013 33: 378:temperature 362:solar radii 332:temperature 290:. It has a 230:Temperature 156:Mean radius 109:Inclination 599:Categories 505:1605.02825 384:References 245:Kepler-89e 17:Kepler-89e 498:(2): 86. 441:1303.2150 434:(1): 14. 348:Kepler-89 342:Host star 261:Kepler-89 253:exoplanet 143:Kepler-89 22:Discovery 532:20832201 466:14261965 360:of 1.32 356:, and a 273:type III 251:, is an 510:Bibcode 446:Bibcode 370:planets 334:of 584 324:Mercury 300:density 288:Neptune 249:KOI-94e 204:density 530:  464:  358:radius 308:radius 304:Saturn 284:Uranus 276:planet 257:Cygnus 34:et al. 528:S2CID 500:arXiv 462:S2CID 436:arXiv 374:years 296:Earth 215:−0.56 213:+0.26 202:Mean 556:stub 320:days 292:mass 286:and 280:blue 210:0.60 175:Mass 139:Star 131:−3.5 129:+2.3 518:doi 496:822 454:doi 432:768 366:Sun 302:to 185:−28 183:+18 126:4.5 601:: 526:. 516:. 508:. 494:. 490:. 474:^ 460:. 452:. 444:. 430:. 392:^ 338:. 263:. 223:cm 180:35 167:🜨 587:e 580:t 573:v 562:. 534:. 520:: 512:: 502:: 468:. 456:: 448:: 438:: 336:K 220:g 194:E 191:M 164:R 102:d

Index

Discovered by
Detection method
Transit method
Orbital characteristics
Semi-major axis
Eccentricity
Orbital period (sidereal)
d
Inclination
Semi-amplitude
Kepler-89
Mean radius
R🜨
Mass
ME
density
g
cm
Temperature
exoplanet
Cygnus
Kepler-89
type III
planet
blue
Uranus
Neptune
mass
Earth
density

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