قائمة الكواكب خارج المجموعة الشمسية المكتشفة سنة 2017

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
!data-sort-type="number"|نصف القطر
!data-sort-type="number"|دور مداري (بالأيام)
!data-sort-type="number"|نصف المحور الرئيسي (AU)
!data-sort-type="number"|درجة حرارة التوازن الكوكبي (كلفن)
!طريقة الاكتشاف
!data-sort-type="number"|سنة الاكتشاف
!data-sort-type="number"|المسافة (ly)
!data-sort-type="number"|كتلة النجم المستضيف
!data-sort-type="number"|درجة الحرارة الفعالة (كلفن)
!ملاحظات
|-
|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 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
|
|-
|
|
|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
|-
|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
||}
قوائم الكواكب الخارجية
قائمة الكواكب خارج المجموعة الشمسية (القائمة الكاملة)
قائمة كواكب خارج المجموعة الشمسية مكتشفة قبل عام 2000
قائمة الكواكب الخارجية المكتشفة بين عامي 2000-2009
قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2010
قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2011
قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2012
قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2013
قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2014
قائمة كواكب خارج المجموعة الشمسية مكتشفة عام 2016
المراجع
قوائم الكواكب خارج المجموعة الشمسية
قوائم متعلقة 2017
كواكب خارج المجموعة الشمسية اكتشفت في 2017