عرض مصدر قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2017

فيما يلي قائمة الكواكب الخارجية المكتشفة عام 2017.

تضم الكواكب الخارجية التي كُشف النقاب عنها بطريقة السرعة الشعاعية فقط، قيمة الكتلة هي في الواقع حدٌ أدنى (لمزيد من المعلومات طالع [[أدنى كتلة]])
{|class="wikitable plainrowheaders sortable" style="width:100%; style="font-size: 83%;"
 !الاسم
 !data-sort-type="number"|الكتلة ({{كتلة المشتري}})
 !data-sort-type="number"|نصف القطر ({{نصف قطر المشتري}})
 !data-sort-type="number"|[[دور مداري]] (بالأيام)
 !data-sort-type="number"|[[نصف المحور الأكبر والأصغر|نصف المحور الرئيسي]] (AU)
 !data-sort-type="number"|[[درجة حرارة التوازن الكوكبي]] ([[كلفن]])<ref>{{استشهاد ويب
|مسار = http://exoplanet.eu/catalog/
|عنوان = موسوعة الكواكب خارج المجموعة الشمسية
|تاريخ الوصول = 2015-11-09| مسار أرشيف = https://web.archive.org/web/20190522181154/http://exoplanet.eu/catalog/ | تاريخ أرشيف = 22 مايو 2019 }}</ref>
 !طريقة الاكتشاف
 !data-sort-type="number"|سنة الاكتشاف
 !data-sort-type="number"|المسافة (ly)
 !data-sort-type="number"|كتلة النجم المستضيف ({{Solar mass|link=yes}})
 !data-sort-type="number"|[[درجة الحرارة الفعالة]] (كلفن)
 !ملاحظات
<onlyinclude>|-
|[[BD+03 2562 b]]
|6.4
|
|481.9
|1.3
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|8540
|1.14
|4095
|
|-
|[[CoRoT 223977153 b]]
|0.15
|0.57
|6.71837
|0.071
|938
|style="background:#FFFF00"|transit
|2017
|
|1.08
|5970
|
|-
|[[لويتن b]]
|0.00909
|
|18.6498
|0.091101
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.29
|3382
|
|-
|[[Gliese 273 c]]
|0.00371
|
|4.7234
|0.036467
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.29
|3382
|
|-
|[[Gliese 625 b]]
|0.00887
|
|14.628
|0.078361
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|21
|0.30
|3499
|
|-
|[[Gliese 1148 c]]
|0.2141
|
|532.58
|0.912
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|35.98
|
|
|
|-
|[[Gliese 3138 b]]
|0.0056
|
|1.22003
|0.0197
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|92.9
|0.68
|3717
|
|-
|[[Gliese 3138 c]]
|0.01315
|
|5.974
|0.057
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|92.9
|0.68
|3717
|
|-
|[[Gliese 3138 d]]
|0.03304
|
|257.8
|0.698
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|92.9
|0.68
|3717
|
|-
|[[Gliese 3293 d]]
|0.02391
|
|48.1345
|0.19394
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|51.4
|0.42
|3466
|
|-
|[[Gliese 3293 e]]
|0.01032
|
|13.2543
|0.08208
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|51.4
|0.42
|3466
|
|-
|[[Gliese 3323 b]]
|0.00636
|
|5.3636
|0.03282
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|17.4
|0.16
|3159
|
|-
|[[Gliese 3323 c]]
|0.00727
|
|40.54
|0.1264
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|17.4
|0.16
|3159
|
|-
|[[Gliese 3942 b]]
|0.0225
|
|6.905
|0.0608
|590
|style="background:#00FF00"|سرعة شعاعية.
|2017
|55.3
|0.63
|3867
|
|-
|[[HAT-P-67b]]
|0.34
|2.085
|4.81010250
|0.06505
|
|style="background:#FFFF00"|transit
|2017
|1000
|1.642
|6406
|
|-
|[[HATS-22b]]
|2.74
|0.953
|4.7228124
|0.05025
|858
|style="background:#FFFF00"|transit
|2017
|678
|0.76
|4803
|
|-
|[[HATS-23b]]
|1.47
|1.86
|2.1605156
|0.03397
|1654
|style="background:#FFFF00"|transit
|2017
|2440
|1.12
|5780
|
|-
|[[HATS-24b]]
|2.44
|1.487
|1.3484954
|0.02547
|2067
|style="background:#FFFF00"|transit
|2017
|1700
|1.21
|6346
|
|-
|[[HD 3167 d]]
|0.0217
|
|8.509
|0.07757
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|149
|0.86
|5261
|
|-
|[[HD 17674 b]]
|0.87
|
|623.8
|1.42
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|145
|0.98
|5904
|
|-
|[[HD 20794 e]]
|0.0150
|
|147.02
|0.509
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|19.8
|0.7
|5401
|
|-
|[[HD 27894 c]]
|0.162
|
|36.07
|0.198
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|138.2
|0.8
|4875
|
|-
|[[HD 27894 d]]
|5.415
|
|5174
|5.448
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|138.2
|0.8
|4875
|
|-
|[[HD 29021 b]]
|2.4
|
|1362.3
|2.28
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|100
|0.85
|5560
|
|-
|[[HD 34445 c]]
|0.168
|
|214.67
|0.7181
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|146.8
|1.07
|5836
|
|-
|[[HD 34445 d]]
|0.0970
|
|117.87
|0.4817
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|146.8
|1.07
|5836
|
|-
|[[HD 34445 e]]
|0.0529
|
|49.175
|0.2687
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|146.8
|1.07
|5836
|
|-
|[[HD 34445 f]]
|0.119
|
|676.8
|1.543
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|146.8
|1.07
|5836
|
|-
|[[HD 34445 g]]
|0.38
|
|5700
|6.36
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|146.8
|1.07
|5836
|
|-
|[[HD 40956 b]]
|2.7
|
|578.6
|1.4
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|385
|2.00
|4869
|
|-
|[[HD 42012 b]]
|1.6
|
|857.5
|1.67
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|121
|0.83
|5405
|
|-
|[[HD 76920 b]]
|3.93
|
|415.4
|1.149
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|602.7
|1.17
|4698
|مدار منحرف للغاية يدور حول نجم [[عملاق أحمر]] متطور
|-
|[[HD 106315 b]]
|
|0.199
|9.5521
|0.09012
|1149
|style="background:#FFFF00"|transit
|2017
|350
|1.07
|6290
|
|-
|[[HD 106315 c]]
|
|0.352
|21.0576
|0.1526
|1143
|style="background:#FFFF00"|transit
|2017
|350
|1.07
|6290
|
|-
|[[HD 111591 b]]
|4.4
|
|1056.4
|2.5
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|352
|1.94
|4884
|
|-
|[[HD 113996 b]]
|6.3
|
|610.2
|1.6
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|331.4
|1.49
|4181
|
|-
|[[HD 176986 b]]
|0.0181
|
|6.48980
|0.06296
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|86.1
|0.79
|4931
|
|-
|[[HD 176986 c]]
|0.02888
|
|16.8191
|0.11878
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|86.1
|0.79
|4931
|
|-
|[[HD 177565 b]]
|0.04751
|
|44.505
|0.246
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|56
|1.0
|
|
|-
|[[HD 208897 b]]
|1.40
|
|352.7
|1.05
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|211
|1.25
|4860
|
|-
|[[HIP 65426 b]]
|9.0
|
|
|92
|1450
|style="background:#FF6CDA"|imaging
|2017
|363
|1.96
|8840
|
|-
|[[HIP 67537 b]]
|11.1
|
|2556.5
|4.91
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|
|2.41
|4985
|
|-
|[[K2-18c]]
|0.0236
| 
|8.962
|0.060
|363
|style="background:#00FF00"|سرعة شعاعية.
|2017
|110
|0.36
|3547
|
|-
|[[K2-105b]]
|0.09439
|0.369
|8.266902
|0.081
|
|style="background:#FFFF00"|transit
|2017
|760
|1.01
|5434
|
|-
|[[K2-107b]]
|0.84
|1.44
|3.31392
|0.048
|
|style="background:#FFFF00"|transit
|2017
|
|1.3
|6030
|
|-
|[[K2-108b]]
|0.18689
|0.471
|4.73401
|0.0573
|1446
|style="background:#FFFF00"|transit
|2017
|
|1.12
|5474
|
|-
|[[K2-110b]]
|0.0525
|0.2312
|13.86375
|0.1021
|640
|style="background:#FFFF00"|transit
|2017
|385
|0.74
|5010
|
|-
|[[K2-111b]]
|0.0271
|0.17
|5.35117
|0.0621
|1309
|style="background:#FFFF00"|transit
|2017
|680
|0.88
|5730
|
|-
|[[K2-113b]]
|1.29
|0.930
|5.817608
|0.0558
|1178
|style="background:#FFFF00"|transit
|2017
|1800
|1.01
|5627
|
|-
|[[K2-114b]]
|1.85
|0.942
|11.39109
|0.09309
|719
|style="background:#FFFF00"|transit
|2017
|1570
|0.83
|5027
|
|-
|[[K2-115b]]
|0.84
|1.115
|20.273034
|0.1367
|682
|style="background:#FFFF00"|transit
|2017
|1360
|0.83
|5560
|
|-
|[[K2-116b]]
|
|0.062
|4.655411
|0.048
|
|style="background:#FFFF00"|transit
|2017
|183.1
|0.69
|4348
|
|-
|[[K2-117b]]
|
|0.175
|1.291505
|0.019
|
|style="background:#FFFF00"|transit
|2017
|
|0.58
|3842
|
|-
|[[K2-117c]]
|
|0.181
|5.444820
|0.051
|
|style="background:#FFFF00"|transit
|2017
|
|0.58
|3842
|
|-
|[[K2-118b]]
|
|0.227
|50.92092
|0.245
|
|style="background:#FFFF00"|transit
|2017
|
|0.76
|4726
|
|-
|[[K2-119b]]
|
|0.204
|7.728578
|0.070
|
|style="background:#FFFF00"|transit
|2017
|
|0.76
|4753
|
|-
|[[K2-120b]]
|
|0.179
|9.562742
|0.078
|
|style="background:#FFFF00"|transit
|2017
|
|0.69
|4350
|
|-
|[[K2-121b]]
|
|0.814
|5.185754
|0.052
|
|style="background:#FFFF00"|transit
|2017
|
|0.71
|4471
|
|-
|[[K2-122b]]
|
|0.114
|2.219405
|0.029
|
|style="background:#FFFF00"|transit
|2017
|
|0.63
|3993
|
|-
|[[K2-123b]]
|
|0.236
|30.956763
|0.167
|
|style="background:#FFFF00"|transit
|2017
|
|0.65
|4076
|
|-
|[[K2-124b]]
|
|0.236
|6.413539
|0.051
|
|style="background:#FFFF00"|transit
|2017
|
|0.44
|3561
|
|-
|[[K2-125b]]
|
|0.194
|21.750264
|0.121
|
|style="background:#FFFF00"|transit
|2017
|
|0.49
|3654
|
|-
|[[K2-126b]]
|
|0.164
|7.387073
|0.066
|
|style="background:#FFFF00"|transit
|2017
|
|0.70
|4368
|
|-
|[[K2-127b]]
|
|0.773
|3.588165
|0.041
|
|style="background:#FFFF00"|transit
|2017
|
|0.70
|4388
|
|-
|[[K2-128b]]
|
|0.127
|5.675819
|0.056
|
|style="background:#FFFF00"|transit
|2017
|
|0.71
|4470
|
|-
|[[K2-129b]]
|
|0.0928
|8.239493
|0.057
|
|style="background:#FFFF00"|transit
|2017
|
|0.36
|3459
|
|-
|[[K2-130b]]
|
|0.112
|2.494120
|0.032
|
|style="background:#FFFF00"|transit
|2017
|
|0.70
|4356
|
|-
|[[K2-131b]]
|
|0.161
|0.3693038
|
|
|style="background:#FFFF00"|transit
|2017
|568
|0.84
|5200
|
|-
|[[K2-132b]]
|
|1.30
|9.1751
|
|
|style="background:#FFFF00"|transit
|2017
|568
|1.08
|4840
|
|-
|[[K2-133b]]
|
|0.117
|3.0712
|0.033
|
|style="background:#FFFF00"|transit
|2017
|250
|0.51
|3655
|
|-
|[[K2-133c]]
|
|0.132
|4.8682
|0.045
|
|style="background:#FFFF00"|transit
|2017
|250
|0.51
|3655
|
|-
|[[K2-133d]]
|
|0.180
|11.0234
|0.077
|
|style="background:#FFFF00"|transit
|2017
|250
|0.51
|3655
|
|-
|[[K2-135b]]
|
|0.156
|1.208957
|0.020
|1043.5
|style="background:#FFFF00"|transit
|2017
|98.8
|0.66
|4255
|
|-
|[[K2-135c]]
|
|0.121
|3.64802
|0.042
|721.9
|style="background:#FFFF00"|transit
|2017
|98.8
|0.66
|4255
|
|-
|[[K2-135d]]
|
|0.187
|6.20141
|0.060
|604.9
|style="background:#FFFF00"|transit
|2017
|98.8
|0.66
|4255
|
|-
|[[K2-136b]]
|
|0.0883
|7.975292
|
|553
|style="background:#FFFF00"|transit
|2017
|
|0.74
|4499
|
|-
|[[K2-136c]]
|
|0.260
|17.307137
|0.11728
|425
|style="background:#FFFF00"|transit
|2017
|
|0.74
|4499
|
|-
|[[K2-136d]]
|
|0.129
|25.575065
|
|373
|style="background:#FFFF00"|transit
|2017
|
|0.74
|4499
|
|-
|[[K2-137b]]
|<0.5
|0.079
|0.179715
|0.0058
|1471
|style="background:#FFFF00"|transit
|2017
|
|0.46
|3492
|
|-
|[[K2-139b]]
|0.387
|0.808
|28.38236
|0.179
|565
|style="background:#FFFF00"|transit
|2017
|496
|1.8
|5340
|
|-
|[[كيلت-9b]]
|2.88
|1.891
|1.4811235
|0.03462
|4050
|style="background:#FFFF00"|transit
|2017
|615.5
|2.52
|10170
|الكوكب الخارجي الأكثر سخونة المعروف على الإطلاق
|-
|[[KELT-11b]]
|0.195
|1.37
|4.736529
|0.06229
|1712
|style="background:#FFFF00"|transit
|2017
|320
|1.44
|5370
|
|-
|[[KELT-12b]]
|0.950
|1.78
|5.031623
|0.06708
|1800
|style="background:#FFFF00"|transit
|2017
|
|1.59
|6279
|
|-
|[[KELT-16b]]
|2.75
|1.415
|0.9689951
|0.02044
|
|style="background:#FFFF00"|transit
|2017
|1289.2
|1.21
|6236
|
|-
|[[KELT-18b]]
|1.18
|1.570
|2.8717518
|0.04550
|2085
|style="background:#FFFF00"|transit
|2017
|
|1.52
|6670
|
|-
|[[KELT-20b]]
|
|1.741
|3.4741085
|0.0542
|2262
|style="background:#FFFF00"|transit
|2017
|455.6
|1.76
|8720
|
|-
|[[Kepler-19d]]
|0.0708
|
|62.95
|
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|6910
|0.94
|5541
|
|-
|[[كيبلر 80]]
|
|0.101
|14.64558
|
|418
|style="background:#FFFF00"|transit
|2017
|1160
|0.73
|4540
|
|-
|[[كيبلر-90i|كيبلر 90 آي]]
|
|0.118
|14.44912
|
|709
|style="background:#FFFF00"|transit
|2017
|2540
|1.2
|6080
|
|-
|[[Kepler-150f]]
|
|0.325
|637.2093
|1.24
|
|style="background:#FFFF00"|transit
|2017
|
|
|5560
|
|-
|[[Kepler-1649b]]
|
|0.0964
|8.689090
|0.0514
|
|style="background:#FFFF00"|transit
|2017
|
|0.22
|3240
|
|-
|[[Kepler-1650b]]
|
|0.0856
|1.53818001
|
|
|style="background:#FFFF00"|transit
|2017
|393
|0.33
|3410
|
|-
|[[Kepler-1651b]]
|
|0.164
|9.87863917
|
|
|style="background:#FFFF00"|transit
|2017
|226
|0.52
|3713
|
|-
|{{Ill-WD2|كليبر 1652 بي|id=Q43449547}}
|
|0.143
|38.09722
|0.1654
|268
|style="background:#FFFF00"|transit
|2017
|822
|0.40
|3638
|
|-
|[[Kepler-1653b]]
|
|0.194
|140.2524
|0.4706
|284
|style="background:#FFFF00"|transit
|2017
|2460
|0.72
|4807
|
|-
|[[إل إتش إس 1140 بي]]
|0.0209
|0.128
|24.73712
|0.0875
|230
|style="background:#FFFF00"|transit
|2017
|40.7
|0.15
|3131
|
|-
|[[MASCARA-1b]]
|3.7
|1.5
|2.148780
|0.043
|2570
|style="background:#FFFF00"|transit
|2017
|615.5
|1.72
|7554
|
|-
|[[MOA-2012-BLG-006Lb]]
|8.40
|
|
|10.2
|
|style="background:#0099FF"|microlensing
|2017
|17000
|0.49
|
|
|-
|[[MOA-2012-BLG-505Lb]]
|0.02108
|
|
|0.900
|
|style="background:#0099FF"|microlensing
|2017
|23500
|0.10
|
|
|-
|[[MOA-2016-BLG-227Lb]]
|2.8
|
|
|1.67
|
|style="background:#0099FF"|microlensing
|2017
|21000
|0.29
|
|
|-
|[[MXB 1658-298 b]]
|23.7
|
|760
|1.613
|
|style="background:#FF7519"|timing
|2017
|
|1.98
|
|
|-
|[[NGTS-1b]]
|0.812
|1.33
|2.647298
|0.0326
|790
|style="background:#FFFF00"|transit
|2017
|731
|0.617
|3916
|
|-
|[[OGLE-2013-BLG-0132Lb]]
|0.29
|
|
|3.6
|
|style="background:#0099FF"|microlensing
|2017
|13000
|0.54
|
|
|-
|[[OGLE-2013-BLG-1721Lb]]
|0.64
|
|
|2.6
|
|style="background:#0099FF"|microlensing
|2017
|21000
|0.46
|
|
|-
|[[OGLE-2016-BLG-0263Lb]]
|4.10
|
|
|5.4
|
|style="background:#0099FF"|microlensing
|2017
|21000
|0.13
|
|
|-
|[[OGLE-2016-BLG-0613(AB)b]]
|4.18
|
|
|6.40
|
|style="background:#0099FF"|microlensing
|2017
|11100
|0.72
|
|
|-
|[[OGLE-2016-BLG-1190Lb]]
|13.38
|
|1224
|2.17
|
|style="background:#0099FF"|microlensing
|2017
|22100
|0.88
|
|ضخم للغاية؛ احتمال أن يكون [[قزم بني]]<ref name="ARX-20171027">{{استشهاد بأرخايف|author=Ryu, Y.-H. et al. |title=OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf Boundary |date=27 October 2017|eprint=1710.09974 |class=astro-ph.EP }}</ref>
|-
|[[OGLE-2016-BLG-1195Lb]]
|0.00450
|
|
|1.16
|
|style="background:#0099FF"|microlensing
|2017
|13000
|0.08
|
|
|-
|[[PSR J2322-2650 b]]
|0.7949
|
|0.322963997
|0.0102
|
|style="background:#FF7519"|timing
|2017
|750
|1.4
|
|
|-
|[[Qatar-3b]]
|4.31
|1.096
|2.5079204
|0.03783
|1681
|style="background:#FFFF00"|transit
|2017
|
|1.15
|6007
|
|-
|[[Qatar-4b]]
|6.10
|1.135
|1.8053564
|0.02803
|1385
|style="background:#FFFF00"|transit
|2017
|
|0.90
|5215
|
|-
|[[Qatar-5b]]
|4.32
|1.107
|2.8792319
|0.04127
|1415
|style="background:#FFFF00"|transit
|2017
|
|1.13
|5747
|
|-
|[[روس 128 b]]
|0.00440
|
|9.8658
|0.0496
|301
|style="background:#00FF00"|سرعة شعاعية.
|2017
|11.03
|0.17
|3192
|
|-
|[[SAND978 b]]
|2.18
|
|511.21
|
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|2051.3
|1.37
|4200
|
|-
|[[TAP 26 b]]
|1.66
|
|10.79
|0.0968
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|480
|1.04
|4620
|
|-
|[[تاو قيطس]]
|0.0124
|
|162.87
|0.538
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.78
|
|
|-
|[[تاو قيطس]]
|0.0124
|
|636.13
|1.334
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.78
|
|
|-
|[[تاو قيطس]]
|0.00551
|
|20.00
|0.133
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.78
|
|
|-
|[[تاو قيطس]]
|0.00576
|
|49.41
|0.243
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.78
|
|
|-
|[[ترابيست-1e]]
|0.00195
|0.082
|6.099615
|0.02817
|251
|style="background:#FFFF00"|transit
|2017
|39
|0.08
|2559
|كوكب خارجي محتمل أن يكون صالحاً للعيش
|-
|[[ترابيست-1f]]
|0.00214
|0.093
|9.20669
|0.0371
|219
|style="background:#FFFF00"|transit
|2017
|39
|0.08
|2559
|كوكب خارجي محتمل أن يكون صالحاً للعيش
|-
|[[ترابيست-1g]]
|0.00422
|0.101
|12.35294
|0.0451
|199
|style="background:#FFFF00"|transit
|2017
|39
|0.08
|2559
|كوكب خارجي محتمل أن يكون صالحاً للعيش
|-
|[[ترابيست-1h]]
|
|0.067
|20
|0.063
|168
|style="background:#FFFF00"|transit
|2017
|39
|0.08
|2559
|
|-
|[[TYC 4282-605-1 b]]
|10.78
|
|101.54
|0.422
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|2300
|0.97
|4300
|
|-
|[[WASP-53b]]
|2.132
|1.074
|3.3098443
|0.04101
|
|style="background:#FFFF00"|transit
|2017
|
|0.84
|4953
|
|-
|[[WASP-53c]]
|16.35
|
|2840
|3.73
|
|style="background:#FFFF00"|transit
|2017
|
|0.84
|4953
|
|-
|[[WASP-81b]]
|0.729
|1.429
|2.7164762
|0.03908
|
|style="background:#FFFF00"|transit
|2017
|
|1.08
|5870
|
|-
|[[WASP-91b]]
|1.34
|1.03
|2.798581
|0.037
|1160
|style="background:#FFFF00"|transit
|2017
|490
|0.84
|4920
|
|-
|[[WASP-105b]]
|1.8
|0.96
|7.87288
|0.075
|900
|style="background:#FFFF00"|transit
|2017
|
|0.89
|5070
|
|-
|[[WASP-107b]]
|0.12
|0.94
|5.721490
|0.055
|770
|style="background:#FFFF00"|transit
|2017
|
|0.69
|4430
|
|-
|[[WASP-151b]]
|0.31
|1.13
|4.533471
|0.055
|1290
|style="background:#FFFF00"|transit
|2017
|1570
|1.01
|5871
|
|-
|[[WASP-153b]]
|0.39
|1.55
|3.332609
|0.048
|1700
|style="background:#FFFF00"|transit
|2017
|1400
|1.34
|5914
|
|-
|[[WASP-156b]]
|0.128
|0.51
|3.836169
|0.0453
|970
|style="background:#FFFF00"|transit
|2017
|460
|0.84
|4910
|
|-
|[[WASP-167b]]
|
|1.58
|2.0219596
|0.0365
|2329
|style="background:#FFFF00"|transit
|2017
|1240
|1.59
|7000
|
|-
|[[YZ قيطس]]
|0.0024
|
|1.96876
|0.01557
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.13
|3056
|
|-
|[[YZ قيطس]]
|0.00308
|
|3.06008
|0.02090
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.13
|3056
|
|-
|[[YZ قيطس]]
|0.00359
|
|4.65627
|0.02764
|
|style="background:#00FF00"|سرعة شعاعية.
|2017
|12
|0.13
|3056
|
</onlyinclude>|}

==قوائم الكواكب الخارجية==
* [[قائمة الكواكب خارج المجموعة الشمسية]] ( [[قائمة الكواكب خارج المجموعة الشمسية (الكاملة)|القائمة الكاملة]])
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة قبل سنة 2000|قائمة كواكب خارج المجموعة الشمسية مكتشفة قبل عام 2000]]
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة بين عامي 2000-2009|قائمة الكواكب الخارجية المكتشفة  بين عامي 2000-2009]]
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2010|قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2010]] 
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2011|قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2011]] 
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2012|قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2012]] 
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2013|قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2013]] 
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2014|قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2014]] 
* [[قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2016|قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2016]]

==المراجع==
{{مراجع}}

{{علم الكواكب خارج النظام الشمسي}}
{{شريط بوابات|علم الفلك|علم الكواكب خارج المجموعة الشمسية}}

{{بذرة علم الفلك}}

[[تصنيف:قوائم الكواكب خارج المجموعة الشمسية]]
[[تصنيف:قوائم متعلقة 2017]]
[[تصنيف:كواكب خارج المجموعة الشمسية اكتشفت في 2017]]