2019년 발견된 외계 행성 목록

2019년에 발견된 외계 행성 목록은 ^[1]^[2]2019년에 처음 관측된 확인된 외계 행성 목록입니다.

반지름 속도로만 검출된 외계행성의 경우, 표시된 질량의 값은 하한값입니다.자세한 내용은 최소 질량을 참조하십시오.

이름.	질량()`M`_J	반지름()`R`_J	기간(일)	반장축(AU)	온도 (K)^[3]	디스커버리 방법	거리(ly)	항성질량()`M`_☉	호스트별 온도(K)	언급
7 큰개 c	0.87		996.00	2.153		레이디얼 벨	64.6	1.34	4826
베타 픽토리스 c	9		1200	2.7		레이디얼 벨	64.43	1.76
CI Tauri b	11.6^+2.9 _−2.7		8.9891±0.0202			레이디얼 벨	515.3±3.9	0.90±0.02
DS 투카나에 AB		0.509±0.015	8.140268±0.000011		850	통과하다	143.89±0.22	1.01±0.06	5428±80
엡실론 인디아브	3.25		16510	11.55	64.25	레이디얼 벨	11.87	0.75
글리제 49 b	0.0177^+0.0021 _−0.0021		13.8508^+0.0053 _−0.0051	0.0905±0.0011		레이디얼 벨	32.145±0.01	0.515±0.019	3805±51
글리제 143 b	0.09637^+0.00827 _−0.00840	0.2280839±0.0282262	35.589^+0.006 _−0.005	0.140±0.0002		통과하다	53.25±0.02	0.76^+0.03 _−0.02
글리제 357 b	0.00579	0.1086	3.93072	0.035	525	통과하다	30.80	0.342	3505
글리제 357 c	0.0107		9.1247	0.061	401.2	레이디얼 벨	30.80	0.342	3505
글리제 357 d	0.019		55.661	0.204	219.6	레이디얼 벨	30.80	0.342	3505	생명체가 살 수 있는 외계 행성
글리제 378 b	0.04097 ± 0.006		3.822±0.001	0.082±0.002		레이디얼 벨	48.79	0.56±0.01	3879±67
글리제 411 b	0.00941±0.00145		12.9532±0.0079		349.83±0.32	레이디얼 벨	8.284	0.386±0.039	3563±60
글리제 685 b	0.028^+0.0053 _−0.0057		24.160^+0.061 _−0.047	0.1344^+0.0052 _−0.0051		레이디얼 벨	46.7102	0.3816±0.069	0.55±0.06
글리제 686 b	0.022±0.003		15.53209^+0.00166 _−0.00167	0.091±0.004	379⁺²⁴ ₋₂₅	레이디얼 벨	26.612±0.008	0.42±0.05	3663±68
글리제 3512 b	0.463		203.59	0.3380		레이디얼 벨	30.95	0.123	3081	^[4]
글리제 4276 b	0.05213^+0.00296 _−0.00299		13.352±0.003	0.082±0.002		레이디얼 벨	69.6±0.1	0.41±0.03	3387±51
HAT-P-69b[id]	3.58	1.676	4.7869491	0.06555	1930	통과하다	1122	1.65	7394	^[5]
HAT-P-70b[id]	6.78 미만	1.87	2.74432452	0.04739	4000	통과하다	1073	1.89	8450	^[5]^[6]
HATS-54b	0.76	1.067	2.5441828	0.03763	1625	통과하다	2510	1.10	5702
HATS-55b	0.921	1.251	4.2042001	0.05412	1367	통과하다	2034	1.20	6214
HATS-56b	0.602	1.688	4.324799	0.06043	1902	통과하다	1882	1.57	6536
HATS-57b	3.147	1.139	2.3506210	0.03493	1413.4	통과하다	913	1.03	5587
HATS-58Ab	1.03	1.095	4.2180896	0.05798	1721	통과하다	1605	1.46	7175
HATS-70b	12.9^+1.8 _−1.6	1.384^+0.079 _−0.074	1.8882378±0.0000015	0.03632^+0.00074 _−0.00087	2730⁺¹⁴⁰ ₋₁₆₀	통과하다	4263⁺¹⁹⁶ ₋₂₀₂	0.81^+0.50 _−0.33	1.08^+0.16 _−0.14
HD 1397 b	0.415±0.020	1.026^+0.025 _−0.027	11.53533^+0.00079 _−0.00080	0.1097^+0.0011 _−0.0013	1228.3^+10.0 _−9.9	통과하다	260.121	1.324^+0.042 _−0.046	5521±60
HD 2685 b	1.17±0.12	1.44±0.05	4.18088^+0.00005 _−0.00004	0.0568±0.0006	2061±28	통과하다	645.72^+2.77 _−2.28	1.43^+0.05 _−0.04	6801±76
HD 8326 b	0.210±0.062		158.991±1.120	0.533±0.011		레이디얼 벨	100.2	0.80±0.05	4914⁺⁵¹ ₋₃₂
HD 13724 b	26.77^+4.40 _−2.20		14763.405^+4901.655 _−1599.795	12.40^+2.60 _−0.90		레이디얼 벨	141.9±0.17	0.76±0.71	5868±27
HD 15337 b	0.0236^+0.0034 _−0.0032	0.140±0.005	4.75615±0.00017	0.0522±0.0012	1001.0±11.5	통과하다	146.36±0.23	0.90±0.03	5125±50
HD 15337 c	0.0255^+0.0057 _−0.0053	0.213±0.011	17.1784±0.0016	0.1268±0.0038	642±10	통과하다	146.36±0.23	0.90±0.03	5125±50
HD 21411 b	0.207±0.081		84.288±0.198	0.362±0.007		레이디얼 벨	±95.11	0.89±0.05	5605⁺²⁴⁷ ₋₁₃₂
HD 21749 c	0.0116 미만	0.0796^+0.0057 _−0.0052	7.78993^+0.00051 _−0.00044	0.0695^+0.0021 _−0.0023	701⁺²⁵ ₋₂₃	통과하다	53.261±0.023	0.73±0.07	4640±100
HD 23472 b	0.05638^+0.00444 _−0.04405		17.667^+0.142 _−0.095	0.140±0.001		통과하다	127.46±0.13	0.75^+0.04 _−0.03
HD 23472 c	0.05405^+0.00337 _−0.04333		29.625^+0.224 _−0.171	0.170±0.001		통과하다	127.46±0.13	0.75^+0.04 _−0.03
HD 24085 b	0.0371±0.0098		2.0455±0.0002	0.034±0.001		레이디얼 벨	179.4	1.22±0.07	6034⁺³² ₋₅₃
HD 25015 b	4.48^+0.30 _−0.28		6019.320^+679.365 _−262.980	6.19^+0.45 _−0.23		레이디얼 벨	122.2±0.22	0.86±0.05	5160±63
HD 39855 b	0.027±0.005		3.2498±0.0004	0.041±0.001		레이디얼 벨	75.93	0.87±0.05	5576⁺⁵⁰ ₋₄₆
HD 64114 b	0.0560±0.0110		45.791±0.070	0.246±0.005		레이디얼 벨	102.9	0.95±0.05	5676⁺³² ₋₈₇
HD 65216c	1.295±0.062		577.6±1.328	1.140±0.020		레이디얼 벨	114.7±0.1	0.95±0.01	5718±8	2013년 허위^[7] 양성으로 2019년 재발견
HD 92788 c	3.67^+0.30 _−0.25		11611.2975^+5055.06 _−905.820	10.50^+2.90 _−0.55		레이디얼 벨	113.1385	1.15±0.07	5744±24
HD 92987 b	16.88^+0.69 _−0.65		10354.8375^+551.5275 _−270.2850	9.62^+0.36 _−0.26		레이디얼 벨	142.2±0.22	1.08±0.06	5770±36
HD 97048 b	2.5			130		이미징	603	2.4	10000	디스크 운동학 연구를 사용하여 검색됨
HD 102843 b	0.3584±0.0456		3090.942±295.049	4.074±0.199		레이디얼 벨	205.05	0.95±0.05	5436⁺¹⁴⁴ ₋₆₉
HD 103949 b	0.0352±0.0072		120.878±0.446	0.439±0.009		레이디얼 벨	86.50	0.77±0.04	4792⁺⁶⁶ ₋₅₄
HD 125390 b	22.16		1756.2	3.16		레이디얼 벨	503	1.36	4850
HD 180617 b	0.03839^+0.00315 _−0.0044		105.9^+0.09 _−0.1	0.3357^+0.0099 _−0.01		레이디얼 벨	19.28±0.07	0.45±0.04	3557±51
HD 181234 b	8.37^+0.34 _−0.36		7462.0575^+80.3550 _−76.7025	12.40^+2.60 _−0.90		레이디얼 벨	155.9±0.42	1.01±0.06	5386±60
HD 202772 Ab	1.017^+0.070 _−0.068	1.545^+0.052 _−0.060	3.308958±0.000083	0.05208^+0.00064 _−0.00068	2132⁺²⁸ ₋₃₀	통과하다	480.1^+8.2 _−7.8	1.72^+0.06 _−0.07	6272⁺⁷⁷ ₋₇₁
HD 206255 b	0.18±0.022		96.045±0.317	0.461±0.009		레이디얼 벨	245.9	1.42±0.08	5635⁺⁸² ₋₉₉
HD 210193 b	0.4817±0.0733		649.918±8.599	1.487±0.031		레이디얼 벨	137.8	1.04±0.06	5790⁺³⁸ ₋₅₀
HD 2170 b	0.0409±0.0079		25.201±0.025	0.140±0.003		레이디얼 벨	42.4	0.61±0.04	4127⁺¹⁴⁹ ₋₉₄
HD 213885 b	0.0278^+0.0021 _−0.0020	0.1557^+0.0045 _−0.0046	1.008035^+0.000021 _−0.000020	0.02012^+0.00015 _−0.00012		통과하다	156.45721±0.4566189	1.068^+0.020 _−0.018	5978±50	TES가 공개한 밝은(V=7.9) 별 주위에 지구와 유사한 조성을 가진 1일 주기 초지구
HD 213885 c	0.06277^+0.00434 _−0.00428		4.78503^+0.00056 _−0.000051	0.056798^+0.00044 _−0.00032	1265.4^+7.3 _−8.4	레이디얼 벨	156.45721±0.4566189	1.068^+0.020 _−0.018	5978±50
HD 219666 b	0.0522±0.0041	0.140±0.015	6.03607^+0.00064 _−0.00063	0.06356±0.00265	1073±20	통과하다	307.98	1.03±0.03	5527±65
HD 220197 b	0.20		1728	2.729		레이디얼 벨	210	0.91	5683
HD 221416 b	0.140±0.018	0.836^+0.031 _−0.028	14.2767±0.0037	0.1228^+0.00025 _−0.00026		통과하다	310.0931	1.212±0.074	5080±90	TES에 의해 확인된 뜨거운 토성형 행성
HD 221420 b	9.70^+1.10 _−1.00		22482⁺⁴²⁰⁰ ₋₄₁₀₀	18.5±2.3		레이디얼 벨	101.7±0.12	1.67±0.11	5830±44
HD 233832 b	1.78		2058	2.827		레이디얼 벨	192	0.71	4981
HIP 35173 b	0.0400±0.0085		41.516±0.077	0.217±0.004		레이디얼 벨	108.25	0.79±0.05	4881⁺⁵⁵ ₋₈₁
HIP 54373 b	0.02712±0.00579		7.760±0.003	0.063±0.001		레이디얼 벨	61.09	0.57±0.03	4021⁺²²⁶ ₋₁₄₆
HIP 54373 c	0.03914±0.00664		15.140±0.008	0.0990±0.0020		레이디얼 벨	61.09	0.57±0.03	4021⁺²²⁶ ₋₁₄₆
HIP 71135 b	0.0592±0.0129		87.140±0.381	0.335±0.007		레이디얼 벨	105.5	0.66±0.04	4146⁺¹⁰⁷ ₋₁₁₀
HIP 79098(AB)b	20.5±4.5			345±6	2450±150	이미징	477.2±8.2	3.75±1.25		갈색왜성
HR 858 b		0.120^+0.0061 _−0.0057	3.58599±0.00015	0.0480^+0.0010 _−0.0011	1572년⁺²² ₋₁₉	통과하다	104.35	1^+0.074 _−0.080. 1개	6201±50
HR 858 c		0.1730±0.0062	5.97293^+0.00060 _−0.00053	0.0674^+0.0014 _−0.0016	1326⁺¹⁸ ₋₁₆	통과하다	104.35	1^+0.074 _−0.080. 1개	6201±50
HR 858 d		0.120^+0.0077 _−0.0074	11.2300^+0.0011 _−0.0010	0.1027^+0.0022 _−0.0025	1075⁺¹⁵ ₋₁₃	통과하다	104.35	1^+0.074 _−0.080. 1개	6201±50
HR 5183 b	3.23		27000	18	171	레이디얼 벨	102.7	1.07	5794	2019년 현재 가장 타원궤도 중 하나로 발견된 외계 행성
K2-32e		0.0901^+0.0089 _−0.008	4.3482^+0.00069 _−0.00075	0.04951±0.00055		통과하다	516.6±4.2	0.856±0.028		반지름이 지구와 거의 동일하기 때문에 그것은 거의 확실히 지구형 행성이다.
K2-43c		0.216	2.198884		1093.7	통과하다	598	0.57	3841
K2-50c		0.089^+0.011 _−0.01	3.96151^+0.00046 _−0.00051			통과하다	845.82±10.63	0.61±0.06
K2-63c		0.35±0.11	25.4556±0.0047	0.140±0.011		통과하다	524.414±21	1.40±0.25	6771±표준
K2-133e[ru]		0.120^+0.012 _−0.012	26.5841^+0.0018 _−0.0017	0.1346±0.0011	296±10	통과하다	245.3±0.7	0.46±0.01	3655±80	^[8]주성: LP 358-499라고도 합니다.
K2-146c	0.02358	0.195	4.00498		1093.7	통과하다	259	0.33	3385
K2-166c		0.120^+0.019 _−0.015	3.80464^+0.00091 _−0.00105			통과하다	1568.81^+31.64 _−29.03	1.07±0.03
K2-168c		0.105^+0.012 _−0.009	8.0468^+0.0024 _−0.0025			통과하다	800.91±13.67	0.91±0.03
K2-198c		0.1270	3.3596055		1229.9	통과하다	362	0.80	5213
K2-198d		0.2175	7.4500177		943.2	통과하다	362	0.80	5213
K2-282c		0.120^+0.012 _−0.009	0.70531±0.00005			통과하다	1638.22±25.34	0.94±0.04	5499±표준	2020년^[9] 세 번째 행성 발견
K2-290b	0.0664	0.273±0.014	9.2165^+0.00033 _−0.00034	0.0923±0.0066	1230±38	통과하다	897±12	1.19^+0.07 _−0.08	6302±120	^[10] 역행^[11] 궤도에 있는 두 행성
K2-290c	0.774±0.047	1.006±0.050	48.36685^+0.00041 _−0.00040	0.0923±0.0066	676±16	통과하다	897±12	1.19^+0.07 _−0.08	6302±120	^[10] 역행^[11] 궤도에 있는 두 행성
K2-291b	0.0204±0.0036	0.1418^+0.0085 _−0.0064	2. 18177^+0.000066 _−0.000068	0.03261±0.00044		통과하다	295±2	0.93±0.04	5520±60
K2-292b	0.0771±0.0138	0.235^+0.010 _−0.009	16.9841±0.0008	0.13±0.01	795⁺³³ ₋₂₈	통과하다	372.76^+2.67 _−2.64	1.00±0.03	5725±65
K2-293b		0.219^+0.031 _−0.022	13.1225^+0.0011 _−0.0012		750⁺¹⁷⁰ ₋₅₀	통과하다	1290±22	0.96^+0.04 _−0.03	5532±78
K2-294b		0.120^+0.019 _−0.017	2.50387^+0.00022 _−0.00023		1425⁺⁷⁹ ₋₅₄	통과하다	1230±20	0.99^+0.03 _−0.03	5612±50
K2-295b	0.335±0.062	{0.897^+0.011 _−0.005}	4.024867±0.000015	0.0451^+0.0006 _−0.0014	852⁺¹⁴ ₋₆	통과하다	736.1±7.8	0.74±0.04	4444±70
K2-296b		0.120^+0.018 _−0.04	28.1656^+0.0027 _−0.0028			통과하다	521.78±4.57	0.41^+0.11 _−0.05
K2-297b		0.062^+0.005 _−0.004	2.13174±0.00022			통과하다	831.31±5.48	0.78^+0.09 _−0.17
K2-298b		0.098^+0.012 _−0.011	4.16959^+0.00051 _−0.00053			통과하다	1441.42±26.65	0.8^+0.08 _−0.16
K2-299b		0.120^+0.053 _−0.028	4.50756^+0.00062 _−0.0006			통과하다	1219.21±16.28	0.93^+0.08 _−0.1	5724±72	2020년^[9] 항성계 행성 2개 추가 발견
K2-300b		0.09^+0.021 _−0.012	2.87814^+0.00023 _−0.00026			통과하다	528.67±5.87	0.22^+0.04 _−0.06
K2-301b[ru]		0.120^+0.015 _−0.017	5.29711^+0.00074 _−0.0007			통과하다	1491.42±44.98	0.56±0.05	4114±99
K2-302b		0.08^+0.017 _−0.018	2.25372±0.00047			통과하다	359.49±3.52	0.41^+0.1 _−0.08		2020년 행성^[9] 2개 추가 발견
K2-303b		0.086^+0.01 _−0.013	1.58252^+0.00017 _−0.00018			통과하다	1034.57±9.59	0.71^+0.09 _−0.03
K2-304b		0.120^+0.007 _−0.008	2.28943±0.00019			통과하다	1380.78±23.94	0.83^+0.09 _−0.12
K2-305b		0.120^+0.06 _−0.037	18.0983^+0.006 _−0.0058			통과하다	2030.88±33.92	1.11^+0.14 _−0.12
K2-306b		0.120^+0.012 _−0.014	34.885^+0.011 _−0.01			통과하다	931.54±6.69	0.91^+0.04 _−0.16
K2-307b		0.1^+0.011 _−0.008	15.2841^+0.0037 _−0.0029			통과하다	1053.09±20.65	0.98^+0.04 _−0.03	6004⁺⁷⁷ ₋₇₈	2개의 행성이 더 있을 것으로 ^[12]추정되며^[13], 2021년 두 번째 행성이 확인되었습니다.
K2-308b		0.884±0.087	3.38628±0.00002			통과하다		1.09±0.09	6100±263
K2-310b		0.2307±0.0112	13.6030±0.0013	0.0980±0.0040	536±18	통과하다	1133.22	0.690±0.038	4684±79
K2-310c		0.2400±0.0130	65.5500±0.0089	0.280±0.006	316±10	통과하다	1133.22	0.690±0.038	4684±79
K2-311b	13 미만	1.11±0.07	3650⁺¹²⁸⁰ ₋₁₁₃₀	4.5±1.0	183⁺²⁵ ₋₁₈	통과하다	1826.48	0.90±0.09	4898±68
KELT-23Ab	0.938^+0.048 _−0.044	1.323±0.025	2.255251^+0.000011 _−0.000012	0.03302^+0.00068 _−0.00064	1561±20	통과하다	409.07±1.14	0.94^+0.06 _−0.05	5899±49
KELT-24b	5.18	1.272	5.5514926	0.06969	1459	통과하다	313.2	1.46	6509
케플러-47d	0.05984^+0.07501 _−0.03672	0.628^+0.059 _−0.044	187.366^+0.069 _−0.051	0.6992^+0.0031 _−0.0033		통과하다	4900	0.957^+0.013 _−0.015
케플러-65e	0.653^+0.056 _−0.055		258.8^+1.5 _−1.3	0.362±0.007		레이디얼 벨	999.3±8.8	1.25±0.06	6211±66
케플러-82f	0.0658±0.0031		75.732±0.012	0.3395±0.0041		타이밍.	3026.64	0.91±0.03	5401±108
케플러-88d	3.15±0.15		1409⁺¹⁴ ₋₁₃	2.45±0.02		레이디얼 벨	1243±7	1.022^+0.023 _−0.026	5513±67	^[14]
케플러-411e	0.0340±0.0035		31.509728±0.000085	0.140±0.003	503±9	타이밍.	500.94±1.57	0.87±0.04		^[15]
케플러-448c	22		2500	4.2		타이밍.	1318	1.5
케플러-1659b	0.028±0.001	0.17±0.02	13.608±0.00006	0.11229		통과하다	3812.7570	1.02
케플러-1659c	0.0014±0.001	0.17±0.03	20.4415±0.0013	0.1472		통과하다	3812.7570	1.02
케플러-1660b	7.693±0.054			237.68977±0.08237		타이밍.	4013.68±73.27	1.21		이 발견은 케플러에 의해 관측된 2,000개 이상의 일식 쌍성들 사이의 일식 시기 변화를 찾아낸 결과입니다.
KMT-2016-BLG-0212Lb	18			2.2		마이크로렌즈	21000	0.48
KMT-2016-BLG-1107Lb	3.283^+3.468 _−1.835			0.342^+0.070 _−0.085		마이크로렌즈	21700⁺³⁰⁹⁰ ₋₄₄₀₀	0.087^+0.092 _−0.049
KMT-2017-BLG-0165Lb	0.11^+0.05 _−0.04			3.45^+0.98 _−0.95		마이크로렌즈	14774.88	0.760^+0.340 _−0.270		^[16]^[17]
KMT-2017-BLG-1038Lb	2.0^+2.0 _−1.1			1.8^+0.6 _−0.5		마이크로렌즈	19569.3826	0.37^+0.36 _−0.20
KMT-2017-BLG-1146Lb	0.710^+0.800 _−0.420			1.6±0.6		마이크로렌즈	21200.16	0.33^+0.36 _−0.20
KMT-2018-BLG-1990Lb	0.348			0.763		마이크로렌즈	3150	0.09
LHS 3844 b		0.1162±0.0020	0.46292913±0.00000190	0.00622±0.00017	805±20	통과하다	48.60±0.03	0.15±0.01	3036±77
LP 791-18 b		0.0999	0.9480050	0.009690	650	통과하다	86.41	0.14	2960
LP 791-18 c		0.206	4.989963	0.029392	370	통과하다	86.41	0.14	2960
루이텐 98-59 b	0.00157^+0.00094 _−0.00063	0.071±0.004	2.25314±0.00002	0.0233±0.0017		통과하다	34.64	0.31±0.01	3367±150
루이텐 98-59 c	0.00755^+0.00566 _−0.00252	0.12^+0.007 _−0.006	3.690621^+0.000013 _−0.000014	0.0324±0.0023-0.0024		통과하다	34.64	0.31±0.01	3367±150
루이텐 98-59 d	0.0107^+0.0085 _−0.0044	0.14±0.012	7.45086^+0.00004 _−0.00005	0.052±0.004		통과하다	34.64	0.31±0.01	3367±150
LSPM J216+0234 b	0.04185^+0.00315 _−0.00346		14.4399^+0.0078 _−0.0087	0.0876^+0.0022 _−0.0021		레이디얼 벨	57.53±0.07	0.43±0.03	3475±51
LTT 1445 Ab	0.0069	0.123	5.35882	0.03807	433	통과하다	22.4	0.26	3337	^[18]
MOA-bin-29b	0.600			0.48		마이크로렌즈	23200	0.03		^[19]
NGTS-5b[ja]	0.229±0.037	1.140±0.023	3.3569866±0.0000026	0.0382±0.0013	952±24	통과하다	309.5±8.5	0.66^+0.07 _−0.06	4987±41	^[20]
NGTS-6b[ja]	1.339	1.326	0.8820590	0.01677		통과하다	1010	0.77	4730	^[21]
NGTS-8b	0.93	1.09	2.49970	0.035	1345	통과하다	1420	0.89	5241
NGTS-9b	2.90	1.07	4.43527	0.058	1448	통과하다	1420	1.34	6330
NSVS 14256825 b	14.15±0.16		3225±22	3.12±0.07		타이밍.	2734.2±137.31	0.42±0.07	40000
NY 버진리스 c	5.54		8799			타이밍.	1800
OGLE-2015-BLG-1649L	2.54			2.07		마이크로렌즈	1380	0.34
OGLE-2015-BLG-1670Lb	0.0563^+0.0302 _−0.0277			2.62^+0.58 _−0.60		마이크로렌즈	22000⁺³³⁰⁰ ₋₄₂₀₀	0.55±0.28
OGLE-2016-BLG-1067Lb	0.43			1.70		마이크로렌즈	3730	0.30
OGLE-2018-BLG-0532Lb	0.02062^+0.00285 _−0.00254			1^+0.118 _−0.107. 1개		마이크로렌즈				^[22]
OGLE-2018-BLG-0596Lb	0.04383±0.00491			0.97±0.13		마이크로렌즈	18400±2400	0.23±0.03
OGLE-2018-BLG-0740Lb	4.8		5480	6.1		마이크로렌즈	10400	1.0	5912
OGLE-2018-BLG-1011Lb	1.8			6.1		마이크로렌즈	23000	0.18
OGLE-2018-BLG-1011Lc	2.8			0.80		마이크로렌즈	23000	0.18
PDS 70b	8.0±6.0	1.3 이상	43500	22		이미징	369.96±1.70	0.76±0.02	3972±36
PDS 70c	8.0±4.0			34.5±2		이미징	369.96±1.7	0.76±0.02	3972±36
카타르-6b	0.668	1.062	3.506195	0.0423		통과하다	330	0.822	5052
카타르-7b	1.88±0.25	1.70±0.03	{2.0320460±0.0000097	0.0352±0.0002		통과하다	2364.6337	1.409±0.026	6387±38
카타르-8b	0.371±0.062	1.285±0.022	3.71495±0.00100	0.0474±0.0008	1457±14	통과하다	902.5±11	1.03±0.05	5738±51
카타르-9b	1.19±0.16	1.009±0.014	1.540731±0.000038	0.0234±0.0003	1134±9	통과하다	689.5±5.2	0.72±0.02	4309±31
카타르-10b	0.736±0.090	1.543±0.040	1.645321±0.000010	0.0286±0.0006	1955±25	통과하다	1760±33	1.16±0.07	6124±46
SDSS J1228+1040 b		0.0009^+0.0045 _−0.000758	0.0857±0.00021	0.0034±0.000009	1800	타이밍.	413.337977±0.4892346	0.705±0.05		발견된 외계 행성 중 가장 작다.
티가든 b	0.00330^+0.00041 _−0.00038		4.9100±0.0014	0.0252^+0.0008 _−0.0009		레이디얼 벨	12.50±0.013	0.09±0.01	2904±51
티가든 C	0.00349^+0.00050 _−0.00047		11.409±0.009	0.0443^+0.0014 _−0.0015	226	레이디얼 벨	12.50±0.013	0.09±0.01	2904±51	생명체가 살 수 있는 외계 행성
TOI-125 b	0.0299±0.00277	0.2432±0.00669	4.65382±0.00033	0.05186^+0.00086 _−0.00077	1037±11	통과하다	363.3382±1.435088	0.859^+0.044 _−0.038	5320±39	^[23]^[24]
TOI-125 c	0.02086±0.00311	0.24614±0.009	9.15059^+0.0007 _−0.00082	0.814±0.0013	827.8±8.6	통과하다	363.3382±1.435088	0.859^+0.044 _−0.038	5320±39	^[25]^[24]
TOI-125 d	0.0428±0.0038	0.2614±0.0152	19.98^+0.005 _−0.0056	0.05186^+0.00086 _−0.00077	638.1±6.6	통과하다	363.3382±1.435088	0.859^+0.044 _−0.038	5320±39	^[26]^[24]
TOI-150b	1.75^+0.14 _−0.17	1.38±0.04	5.857342^+0.000065 _−0.000066	0.0583^+0.0013 _−0.0018	1493⁺²⁹ ₋₃₂	통과하다	1095.89±6.52	1.25^+0.07 _−0.12	6003⁺¹⁰⁴ ₋₉₈
TOI-163b	1.22	1.489	4.231306	0.0580	1669	통과하다	1359	1.44	6495
TOI-172b	5.42^+0.22 _−0.20	0.965^+0.032 _−0.029	9.47725^+0.00064 _−0.00079	0.0914±0.0017		통과하다	1097.418	1.128^+0.065 _−0.061	5645±50
TOI-216 b	0.059±0.002	0.714^+0.268 _−0.179	17.1607	0.1293^+0.0067 _−0.0051	628⁺¹³ ₋₁₁	통과하다	583±3	0.77	5026±125	반장축은 몇 년의^[27]^[28]^[29] 시간 척도의 행성-행성 상호작용으로 인해 매우 가변적입니다.
TOI-216 c	0.56±0.02	0.902±0.018	34.525528	0.2069^+0.0107 _−0.0082	497⁺¹⁰ ₋₈	통과하다	583±3	0.77	5026±125	반장축은 몇 년의^[27]^[28]^[29] 시간 척도의 행성-행성 상호작용으로 인해 매우 가변적입니다.
TOI-270b[ja]	0.0050	0.1112	3.360080	0.0306	528	통과하다	73.23	0.40	3386	^[30]^[31]
TOI-270c[ja]	0.0193	0.216	5.660172	0.0472	424	통과하다	73.23	0.40	3386	^[30]^[31]
TOI-270d[ja]	0.0150	0.190	11.38014	0.0733	340	통과하다	73.23	0.40	3386	^[30]^[31]
TOI-564b	1.463^+0.10 _−0.096	1.02^+0.71 _−0.29	1.651144±0.000018	0.02734^+0.00061 _−0.00053	1714년⁺²⁰ ₋₂₁	통과하다	643.8±5.9	0.998^+0.068 _−0.057	5640⁺³⁴ ₋₃₇	^[32]
TOI-905b	0.667^+0.042 _−0.041	1.171^+0.052 _−0.051	3.739494±0.000038	0.04666^+0.00096 _−0.0011	1192⁺³⁹ ₋₃₆	통과하다	489.9^+23.5 _−22.5	0.968^+0.061 _−0.068	5570⁺¹⁵⁰ ₋₁₄₀	^[32]
V1298 Tauri b		0.120^+0.049 _−0.053	24.13861^+0.00102 _−0.00090	0.1687^+0.0025 _−0.0026	668±22	통과하다	353.9±2.3	1.10±0.05	4970±120	^[33]
V1298 Tauri c		0.499	8.24958	0.0825	845±27	통과하다	353.9	1.10	4970	^[34]
V1298 Tauri d		0.572	12.4032	0.1083	677±22	통과하다	353.9	1.10	4970	^[34]
V1298 Taurie		0.780	60	0.308	492⁺⁶⁶ ₋₁₀₄	통과하다	353.9	1.10	4970	^[34]
WASP-18Ac	0.140±0.039		2.1558	0.035		타이밍.	404	1.22	6400
WASP-126c	0.140±0.077		7.63±0.17			타이밍.	763.165±48.9235	1.12	5800
WASP-169b	0.561	1.304	5.6114118	0.0681	1604	통과하다	2080	1.34	6110
WASP-171b	1.084	0.980	3.8186244	0.05040	1642	통과하다	2530	1.17	5965
WASP-175b	0.990	1.208	3.0652907	0.04403	1571	통과하다	2080	1.21	6229
WASP-177b	0.508±0.038	1.58^+0.66 _−0.83	3.071722±0.000001	0.03957±0.00058	1142±32	통과하다	580.5583	0.876±0.038	5017±70
WASP-178b	1.66	1.81	3.3448285	0.0558	2470	통과하다	1360	2.07	9360	^[35]
WASP-180Ab	0.9	1.24	3.409264	0.048		통과하다	830	1.3	6600
WASP-181b	0.140±0.034	1.184^+0.071 _−0.059	4.159±0.0000034	0.00542±0.00069	1186⁺³² ₋₂₆	통과하다	1444.872	1.04±0.04	5839±70
WASP-182b	0.148	0.850	3.3769848	0.0451	1479	통과하다	1080	1.08	5638
WASP-183b	0.502±0.047	1.47^+0.94 _−0.33	4.1177±0.0000051	0.0463±0.00075	1111±30	통과하다	1069.79292	1.00±0.03	0.784±0.038
WASP-184b	0.57	1.33	5.18170	0.0627	1480	통과하다	2090	1.23	6000	^[35]
WASP-185b	0.980	1.25	9.38755	0.0904	1160	통과하다	897	1.12	5900	^[35]
WASP-190b	1.0±0.1	1.15±0.09	5.367753±0.000004	0.0663±0.0008	1500±50	통과하다	1796.323	1.35±0.05	6400±100
WASP-192b	2.30	1.23	2.8786765	0.0408	1620	통과하다	1610	1.09	5910	^[35]
KMT-2016-BLG-1836L b	2.2^+1.9 _−1.1			3.5^+1.1 _−0.9		마이크로렌즈	23157.1^+2609.25 _−7827.753	0.49^+0.38 _−0.25		^[36]
HD 85628 A b	3.1±0.9	1.53^+0.07 _−0.04	2.82406±0.00003	0.047±0.004	2100±100	통과하다	559.47±3.05	1.75±0.05	7800±200	마스카라-4b: A3V 거성과 역행 ^[37]궤도에 있는 행성.
OGLE-2016-BLG-127 b	0.79^+1.3 _−0.39			3.4^+2.1 ₋₁		마이크로렌즈		0.1^+0.17 _−0.05		^[38]
OGLE-2013-BLG-0911L b	9.51^+2.72 _−1.69					마이크로렌즈	10500⁺¹⁵⁰⁰ ₋₁₁₀₀	0.29^+0.07 _−0.05		^[39]
L 1159-16 b	0.088^+0.060 _−0.035		241.59^+4.6 _−4.0	0.403^+0.039 _−0.047		레이디얼 벨	14.584±0.007	0.15	3158	^[40]^[41] 2022년 반박^[42]
L 1159-16 c	0.23±0.02		772.05^+2.41 _−1.84	0.88±0.02		레이디얼 벨	14.578±0.005	0.15±0.01	3154±54	^[40]^[41]2022년 L 1159-16b로^[42] 확정
TOI-175b	0.00126^+0.00050 _−0.00048	0.0642^+0.0046 _−0.0035	2.2531136^+0.0000012 _−0.0000015	0.02191^+0.00080 _−0.00084	627⁺³³ ₋₃₆	통과하다	34.636±0.010	0.273±0.030	3415±135	^[43] 현재까지 반지름 속도 ^[44]기법을 사용하여 확인되거나 측정된 행성 중 가장 낮은 질량을 가진 행성이다.L 98-59로도 ^[45]알려진 호스트 별.

특정 외계 행성 목록

레퍼런스

^ "NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. California Institute of Technology. Retrieved 27 March 2018.
^ "Extrasolar Planet's Catalogue (sic)". Kyoto University. Retrieved 20 December 2019.
^ "The Extrasolar Planets Encyclopaedia". Retrieved 20 January 2018.
^ Morales, J. C.; et al. (2019). "A giant exoplanet orbiting a very-low-mass star challenges planet formation models". Science. 365 (6460): 1441–1445. arXiv:1909.12174. Bibcode:2019Sci...365.1441M. doi:10.1126/science.aax3198. ISSN 0036-8075. PMID 31604272. S2CID 202888425.
^ ^a ^b Zhou, G.; et al. (2019), "Two New HATNet Hot Jupiters around a Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS", The Astronomical Journal, 158 (4): 141, arXiv:1906.00462, Bibcode:2019AJ....158..141Z, doi:10.3847/1538-3881/ab36b5, S2CID 173990300
^ Bello-Arufe, Aaron; Cabot, Samuel H. C.; Mendonça, João M.; Buchhave, Lars A.; Rathcke, Alexander D. (2021), Mining the Ultra-Hot Skies of HAT-P-70b: Detection of a Profusion of Neutral and Ionized Species, arXiv:2112.03292
^ Wittenmyer, Robert A.; et al. (2019). "Truly eccentric – I. Revisiting eight single-eccentric planetary systems". Monthly Notices of the Royal Astronomical Society. 484 (4): 5859–5867. arXiv:1901.08471. Bibcode:2019MNRAS.484.5859W. doi:10.1093/mnras/stz290.
^ Validation of a Temperate Fourth Planet in the K2-133 Multi-planet System, 2019, arXiv:1905.05206
^ ^a ^b ^c Adams, Elisabeth R.; Jackson, Brian; Johnson, Samantha; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Furlan, Elise; Howell, Steve B.; Jayanthi, Prasanna; MacQueen, Phillip J.; Matson, Rachel A.; Partyka-Worley, Ciera; Schlieder, Joshua; Scott, Nicholas J.; Stanton, Sevio M.; Ziegler, Carl (2020), ULTRA SHORT PERIOD PLANETS IN K2 III: NEIGHBORS ARE COMMON WITH 12 NEW MULTI-PLANET SYSTEMS AND 26 NEWLY VALIDATED PLANETS IN CAMPAIGNS 0-8, 10, arXiv:2011.11698
^ ^a ^b Hjorth, M.; Justesen, A. B.; Hirano, T.; Albrecht, S.; Gandolfi, D.; Dai, F.; Alonso, R.; Barragán, O.; Esposito, M.; Kuzuhara, M.; Lam, K. W. F.; Livingston, J. H.; Montanes-Rodriguez, P.; Narita, N.; Nowak, G.; Prieto-Arranz, J.; Redfield, S.; Rodler, F.; Van Eylen, V.; Winn, J. N.; Antoniciello, G.; Cabrera, J.; Cochran, W. D.; Csizmadia, Sz; De Leon, J.; Deeg, H.; Eigmüller, Ph; Endl, M.; Erikson, A.; et al. (2019), "K2-290: a warm Jupiter and a mini-Neptune in a triple-star system", Monthly Notices of the Royal Astronomical Society, 484 (3): 3522, arXiv:1901.03716, Bibcode:2019MNRAS.484.3522H, doi:10.1093/mnras/stz139
^ ^a ^b Hjorth, Maria; Albrecht, Simon; Hirano, Teruyuki; Winn, Joshua N.; Dawson, Rebekah I.; Zanazzi, J. J.; Knudstrup, Emil; Sato, Bun'ei (2021), "A backward-spinning star with two coplanar planets", Proceedings of the National Academy of Sciences of the United States of America, 118 (8): e2017418118, arXiv:2102.07677, Bibcode:2021PNAS..11820174H, doi:10.1073/pnas.2017418118, PMC 7923373, PMID 33593909
^ Kovacs, Geza (2020), "More planetary candidates from K2 Campaign 5 using TRAN_K2", Astronomy & Astrophysics, 643: A169, arXiv:2008.10075, Bibcode:2020A&A...643A.169K, doi:10.1051/0004-6361/202038726, S2CID 221266076
^ De Leon, J. P.; Livingston, J.; Endl, M.; Cochran, W. D.; Hirano, T.; García, R. A.; Mathur, S.; Lam, K W F.; Korth, J.; Trani, A. A.; Dai, F.; Díez Alonso, E.; Castro-González, A.; Fridlund, M.; Fukui, A.; Gandolfi, D.; Kabath, P.; Kuzuhara, M.; Luque, R.; Savel, A. B.; Gill, H.; Dressing, C.; Giacalone, S.; Narita, N.; Palle, E.; Van Eylen, V.; Tamura, M. (2021), "37 new validated planets in overlapping K2 campaigns", Monthly Notices of the Royal Astronomical Society, 508: 195–218, arXiv:2108.05621, doi:10.1093/mnras/stab2305
^ Weiss, Lauren M.; Fabrycky, Daniel C.; Agol, Eric; Mills, Sean M.; Howard, Andrew W.; Isaacson, Howard; Petigura, Erik A.; Fulton, Benjamin; Hirsch, Lea; Sinukoff, Evan (2020-04-29). "The Discovery of the Long-Period, Eccentric Planet Kepler-88 d and System Characterization with Radial Velocities and Photodynamical Analysis" (PDF). The Astronomical Journal. 159 (5): 242. arXiv:1909.02427. Bibcode:2020AJ....159..242W. doi:10.3847/1538-3881/ab88ca. ISSN 1538-3881. S2CID 202539420.
^ Sun, L.; Ioannidis, P.; Gu, S.; Schmitt, J. H. M. M.; Wang, X.; Kouwenhoven, M. B. N. (2019), "Kepler-411: a four-planet system with an active host star", Astronomy & Astrophysics, 624: A15, arXiv:1902.09719, Bibcode:2019A&A...624A..15S, doi:10.1051/0004-6361/201834275, S2CID 102481339
^ Jung, Youn Kil; Gould, Andrew; Zang, Weicheng; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Han, Cheongho; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Shin, In-Gu; Shvartzvald, Yossi; Zhu, Wei; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; KMTNet Collaboration; Penny, Matthew T.; Mao, Shude; Fouqué, Pascal; Wang, Tianshu; CFHT Collaboration (2018), "KMT-2017-BLG-0165Lb: A Super-Neptune mass planet Orbiting a Sun-like Host Star", The Astronomical Journal, 157 (2): 72, arXiv:1809.01288, Bibcode:2019AJ....157...72J, doi:10.3847/1538-3881/aaf87f, S2CID 119096973
^ Ryu, Yoon-Hyun; Mróz, Przemek; Gould, Andrew; Hwang, Kyu-Ha; Kim, Hyoun-Woo; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Jung, Youn Kil; Shin, In-Gu; Shvartzvald, Yossi; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Han, Cheongho; Pogge, Richard W.; Udalski, Andrzej; Poleski, Radek; Skowron, Jan; Szymański, Michał K.; Soszyński, Igor; Pietrukowicz, Paweł; Kozłowski, Szymon; Ulaczyk, Krzysztof; et al. (2021), "KMT-2017-BLG-2820 and the Nature of the Free-Floating Planet Population", The Astronomical Journal, 161 (3): 126, arXiv:2010.07527, Bibcode:2021AJ....161..126R, doi:10.3847/1538-3881/abd55f, S2CID 222378863
^ Winters, Jennifer G.; et al. (2019), "Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M-dwarf System at 6.9 pc", The Astronomical Journal, 158 (4): 152, arXiv:1906.10147, Bibcode:2019AJ....158..152W, doi:10.3847/1538-3881/ab364d, S2CID 195584444
^ Kondo, Iona; et al. (2019), "MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star", The Astronomical Journal, 158 (6): 224, arXiv:1905.01239, Bibcode:2019AJ....158..224K, doi:10.3847/1538-3881/ab4e9e, S2CID 145052576
^ Eigmüller, Philipp; et al. (2019), "NGTS-5b: A highly inflated planet offering insights into the sub-Jovian desert", Astronomy & Astrophysics, 625: A142, arXiv:1905.02593, Bibcode:2019A&A...625A.142E, doi:10.1051/0004-6361/201935206, S2CID 146809360
^ Vines, Jose I.; et al. (2019), "NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf", Monthly Notices of the Royal Astronomical Society, 489 (3): 4125–4134, arXiv:1904.07997, doi:10.1093/mnras/stz2349
^ OGLE-2018-BLG-0532Lb: Cold Neptune With Possible Jovian Sibling, 2020, arXiv:1905.08148
^ "The Extrasolar Planet Encyclopaedia — TOI-813 b". exoplanet.eu.
^ ^a ^b ^c Nielsen, L. D.; Gandolfi, D.; Armstrong, D. J.; Jenkins, J. S.; Fridlund, M.; Santos, N. C.; Dai, F.; Adibekyan, V.; Luque, R.; Steffen, J. H.; Esposito, M.; Meru, F.; Sabotta, S.; Bolmont, E.; Kossakowski, D.; Otegi, J. F.; Murgas, F.; Stalport, M.; Rodler, F.; Díaz, M. R.; Kurtovic, N. T.; Ricker, G.; Vanderspek, R.; Latham, D. W.; Seager, S.; Winn, J. N.; Jenkins, J. M.; Allart, R.; Almenara, J. M.; et al. (2020), "Mass determinations of the three mini-Neptunes transiting TOI-125", Monthly Notices of the Royal Astronomical Society, 492 (4): 5399, arXiv:2001.08834, Bibcode:2020MNRAS.492.5399N, doi:10.1093/mnras/staa197
^ "exoplanet.eu toi-125_c".
^ "exoplanet.eu toi-125_d".
^ ^a ^b Teachey, Alex; Jansen, Tiffany; Bakos, Gaspar; Torres, Guillermo; Hartman, Joel; Nesvorný, David; Kipping, David (2019). "A resonant pair of warm giant planets revealed by TESS". Monthly Notices of the Royal Astronomical Society. 486 (4): 4980–4986. arXiv:1902.03900. doi:10.1093/mnras/stz1141.
^ ^a ^b Dawson, Rebekah I.; et al. (2019). "TOI-216b and TOI-216 c: Two Warm, Large Exoplanets in or Slightly Wide of the 2:1 Orbital Resonance". The Astronomical Journal. 158 (2): 65. arXiv:1904.11852. Bibcode:2019AJ....158...65D. doi:10.3847/1538-3881/ab24ba. S2CID 135466349.
^ ^a ^b Dawson, Rebekah I.; Huang, Chelsea X.; Brahm, Rafael; Collins, Karen A.; Hobson, Melissa J.; Jordán, Andrés; Dong, Jiayin; Korth, Judith; Trifonov, Trifon; Abe, Lyu; Agabi, Abdelkrim; Bruni, Ivan; Butler, R. Paul; Barbieri, Mauro; Collins, Kevin I.; Conti, Dennis M.; Crane, Jeffrey D.; Crouzet, Nicolas; Dransfield, Georgina; Evans, Phil; Espinoza, Néstor; Gan, Tianjun; Guillot, Tristan; Henning, Thomas; Lissauer, Jack J.; Jensen, Eric L. N.; Sainte, Wenceslas Marie; Mékarnia, Djamel; Myers, Gordon; et al. (2021), "Precise transit and radial-velocity characterization of a resonant pair: a warm Jupiter TOI-216c and eccentric warm Neptune TOI-216b", The Astronomical Journal, 161 (4): 161, arXiv:2102.06754, Bibcode:2021AJ....161..161D, doi:10.3847/1538-3881/abd8d0, S2CID 231924886
^ ^a ^b ^c "太陽系外惑星「TOI 270 b、c、d」を発見。地球外生命体の存在は？". sorae. 2019-07-30. Retrieved 2021-01-08.
^ ^a ^b ^c Van Eylen, Vincent; Astudillo-Defru, Nicola; Bonfils, Xavier; Livingston, J.; Hirano, T.; Luque, Rafael; Lam, K. W. F.; Justesen, A. B.; Winn, J. N.; Gandolfi, D.; Nowak, G.; Palle, E.; Albrecht, S.; Dai, F.; Campos Estrada, B.; Owen, J. E.; Foreman-Mackey, D.; Fridlund, M.; Korth, J.; Mathur, S.; Forveille, Thierry; Mikal-Evans, T.; Osborne, H. L. M.; Ho, C. S. K.; Almenara, José M.; Artigau, Étienne; Barragán, O.; Bouchy, François; Cabrera, J.; et al. (2021), "Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley", Monthly Notices of the Royal Astronomical Society, arXiv:2101.01593, doi:10.1093/mnras/stab2143
^ ^a ^b Davis, Allen B.; Wang, Songhu; et al. (2020). "TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS". Astronomical Journal. 160 (5): 229. arXiv:1912.10186. Bibcode:2020AJ....160..229D. doi:10.3847/1538-3881/aba49d. hdl:1721.1/134083. S2CID 209444463.
^ David, Trevor J.; Cody, Ann Marie; Hedges, Christina L.; Mamajek, Eric E.; Hillenbrand, Lynne A.; Ciardi, David R.; Beichman, Charles A.; Petigura, Erik A.; Fulton, Benjamin J.; Isaacson, Howard T.; Howard, Andrew W.; Gagné, Jonathan; Saunders, Nicholas K.; Rebull, Luisa M.; Stauffer, John R.; Vasisht, Gautam; Hinkley, Sasha (2019), "A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau", The Astronomical Journal, 158 (2): 79, arXiv:1902.09670, Bibcode:2019AJ....158...79D, doi:10.3847/1538-3881/ab290f, S2CID 119003936
^ ^a ^b ^c David, Trevor J.; Petigura, Erik A.; Luger, Rodrigo; Foreman-Mackey, Daniel; Livingston, John H.; Mamajek, Eric E.; Hillenbrand, Lynne A. (2019), "Four newborn planets transiting the young solar analog V1298 Tau", The Astrophysical Journal, 885 (1): L12, arXiv:1910.04563, Bibcode:2019ApJ...885L..12D, doi:10.3847/2041-8213/ab4c99, S2CID 204008446
^ ^a ^b ^c ^d Hellier, Coel; Anderson, D. R.; Barkaoui, K.; Benkhaldoun, Z.; Bouchy, F.; Burdanov, A.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Nielsen, L. D.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ségransan, D.; Smalley, B.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2019), "WASP-South hot Jupiters: WASP-178b, WASP-184b, WASP-185b & WASP-192b", Monthly Notices of the Royal Astronomical Society, 490 (1): 1479, arXiv:1907.11667, Bibcode:2019MNRAS.490.1479H, doi:10.1093/mnras/stz2713
^ Yang, Hongjing; et al. (2020). "KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field". The Astronomical Journal. 159 (3): 98. arXiv:1908.10011. Bibcode:2020AJ....159...98Y. doi:10.3847/1538-3881/ab660e. S2CID 201646063.
^ "MASCARA-4 b/bRing-1b - A retrograde hot Jupiter around the bright A3V star HD 85628". GroundAI.
^ "The Extrasolar Planet Encyclopaedia — OGLE-2016-BLG-1227 b". exoplanet.eu.
^ "The Extrasolar Planet Encyclopaedia — OGLE-2013-BLG-0911L b". exoplanet.eu.
^ ^a ^b Barnes, J. R.; et al. (2019-06-11), Frequency of planets orbiting M dwarfs in the Solar neighbourhood, arXiv:1906.04644v1, Bibcode:2019arXiv190604644T.
^ ^a ^b Feng, Fabo; Shectman, Stephen A.; Clement, Matthew S.; Vogt, Steven S.; Tuomi, Mikko; Teske, Johanna K.; Burt, Jennifer; Crane, Jeffrey D.; Holden, Bradford; Sharon Xuesong Wang; Thompson, Ian B.; Diaz, Matias R.; Paul Butler, R. (2020), Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs, arXiv:2008.07998, doi:10.3847/1538-4365/abb139, S2CID 221150644
^ ^a ^b The CARMENES search for exoplanets around M dwarfs Two Saturn-mass planets orbiting active stars, 2022, arXiv:2203.16504
^ Kostov, Veselin B.; Schlieder, Joshua E.; et al. (2019). "The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf". The Astronomical Journal. 158 (1): 32. arXiv:1903.08017. Bibcode:2019AJ....158...32K. doi:10.3847/1538-3881/ab2459. hdl:1721.1/124742. ISSN 1538-3881. S2CID 118855908.
^ Demangeon, O. D. S.; Zapatero Osorio, M. R.; Alibert, Y.; Barros, S. C. C.; Adibekyan, V.; Tabernero, H. M.; Antoniadis-Karnavas, A.; Camacho, J. D.; al, et (2021). "Warm terrestrial planet with half the mass of Venus transiting a nearby star" (PDF). Astronomy & Astrophysics. 653: A41. arXiv:2108.03323. Bibcode:2021A&A...653A..41D. doi:10.1051/0004-6361/202140728. S2CID 236957385.
^ "Planet L 98-59 b". exoplanet.eu. Retrieved 6 August 2021.

[1] "NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. California Institute of Technology. Retrieved 27 March 2018.

[2] "Extrasolar Planet's Catalogue (sic)". Kyoto University. Retrieved 20 December 2019.

[3] "The Extrasolar Planets Encyclopaedia". Retrieved 20 January 2018.

[4] Morales, J. C.; et al. (2019). "A giant exoplanet orbiting a very-low-mass star challenges planet formation models". Science. 365 (6460): 1441–1445. arXiv:1909.12174. Bibcode:2019Sci...365.1441M. doi:10.1126/science.aax3198. ISSN 0036-8075. PMID 31604272. S2CID 202888425.

[Zhou2019-5] Zhou, G.; et al. (2019), "Two New HATNet Hot Jupiters around a Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS", The Astronomical Journal, 158 (4): 141, arXiv:1906.00462, Bibcode:2019AJ....158..141Z, doi:10.3847/1538-3881/ab36b5, S2CID 173990300

[6] Bello-Arufe, Aaron; Cabot, Samuel H. C.; Mendonça, João M.; Buchhave, Lars A.; Rathcke, Alexander D. (2021), Mining the Ultra-Hot Skies of HAT-P-70b: Detection of a Profusion of Neutral and Ionized Species, arXiv:2112.03292

[Wittenmyer2019-7] Wittenmyer, Robert A.; et al. (2019). "Truly eccentric – I. Revisiting eight single-eccentric planetary systems". Monthly Notices of the Royal Astronomical Society. 484 (4): 5859–5867. arXiv:1901.08471. Bibcode:2019MNRAS.484.5859W. doi:10.1093/mnras/stz290.

[8] Validation of a Temperate Fourth Planet in the K2-133 Multi-planet System, 2019, arXiv:1905.05206

[Adams2020-9] Adams, Elisabeth R.; Jackson, Brian; Johnson, Samantha; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Furlan, Elise; Howell, Steve B.; Jayanthi, Prasanna; MacQueen, Phillip J.; Matson, Rachel A.; Partyka-Worley, Ciera; Schlieder, Joshua; Scott, Nicholas J.; Stanton, Sevio M.; Ziegler, Carl (2020), ULTRA SHORT PERIOD PLANETS IN K2 III: NEIGHBORS ARE COMMON WITH 12 NEW MULTI-PLANET SYSTEMS AND 26 NEWLY VALIDATED PLANETS IN CAMPAIGNS 0-8, 10, arXiv:2011.11698

[Njorth2019-10] Hjorth, M.; Justesen, A. B.; Hirano, T.; Albrecht, S.; Gandolfi, D.; Dai, F.; Alonso, R.; Barragán, O.; Esposito, M.; Kuzuhara, M.; Lam, K. W. F.; Livingston, J. H.; Montanes-Rodriguez, P.; Narita, N.; Nowak, G.; Prieto-Arranz, J.; Redfield, S.; Rodler, F.; Van Eylen, V.; Winn, J. N.; Antoniciello, G.; Cabrera, J.; Cochran, W. D.; Csizmadia, Sz; De Leon, J.; Deeg, H.; Eigmüller, Ph; Endl, M.; Erikson, A.; et al. (2019), "K2-290: a warm Jupiter and a mini-Neptune in a triple-star system", Monthly Notices of the Royal Astronomical Society, 484 (3): 3522, arXiv:1901.03716, Bibcode:2019MNRAS.484.3522H, doi:10.1093/mnras/stz139

[Njorth2021-11] Hjorth, Maria; Albrecht, Simon; Hirano, Teruyuki; Winn, Joshua N.; Dawson, Rebekah I.; Zanazzi, J. J.; Knudstrup, Emil; Sato, Bun'ei (2021), "A backward-spinning star with two coplanar planets", Proceedings of the National Academy of Sciences of the United States of America, 118 (8): e2017418118, arXiv:2102.07677, Bibcode:2021PNAS..11820174H, doi:10.1073/pnas.2017418118, PMC 7923373, PMID 33593909

[Kovaks2020-12] Kovacs, Geza (2020), "More planetary candidates from K2 Campaign 5 using TRAN_K2", Astronomy & Astrophysics, 643: A169, arXiv:2008.10075, Bibcode:2020A&A...643A.169K, doi:10.1051/0004-6361/202038726, S2CID 221266076

[Leon2021-13] De Leon, J. P.; Livingston, J.; Endl, M.; Cochran, W. D.; Hirano, T.; García, R. A.; Mathur, S.; Lam, K W F.; Korth, J.; Trani, A. A.; Dai, F.; Díez Alonso, E.; Castro-González, A.; Fridlund, M.; Fukui, A.; Gandolfi, D.; Kabath, P.; Kuzuhara, M.; Luque, R.; Savel, A. B.; Gill, H.; Dressing, C.; Giacalone, S.; Narita, N.; Palle, E.; Van Eylen, V.; Tamura, M. (2021), "37 new validated planets in overlapping K2 campaigns", Monthly Notices of the Royal Astronomical Society, 508: 195–218, arXiv:2108.05621, doi:10.1093/mnras/stab2305

[Weiss2019-14] Weiss, Lauren M.; Fabrycky, Daniel C.; Agol, Eric; Mills, Sean M.; Howard, Andrew W.; Isaacson, Howard; Petigura, Erik A.; Fulton, Benjamin; Hirsch, Lea; Sinukoff, Evan (2020-04-29). "The Discovery of the Long-Period, Eccentric Planet Kepler-88 d and System Characterization with Radial Velocities and Photodynamical Analysis" (PDF). The Astronomical Journal. 159 (5): 242. arXiv:1909.02427. Bibcode:2020AJ....159..242W. doi:10.3847/1538-3881/ab88ca. ISSN 1538-3881. S2CID 202539420.

[Sun2019-15] Sun, L.; Ioannidis, P.; Gu, S.; Schmitt, J. H. M. M.; Wang, X.; Kouwenhoven, M. B. N. (2019), "Kepler-411: a four-planet system with an active host star", Astronomy & Astrophysics, 624: A15, arXiv:1902.09719, Bibcode:2019A&A...624A..15S, doi:10.1051/0004-6361/201834275, S2CID 102481339

[16] Jung, Youn Kil; Gould, Andrew; Zang, Weicheng; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Han, Cheongho; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Shin, In-Gu; Shvartzvald, Yossi; Zhu, Wei; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; KMTNet Collaboration; Penny, Matthew T.; Mao, Shude; Fouqué, Pascal; Wang, Tianshu; CFHT Collaboration (2018), "KMT-2017-BLG-0165Lb: A Super-Neptune mass planet Orbiting a Sun-like Host Star", The Astronomical Journal, 157 (2): 72, arXiv:1809.01288, Bibcode:2019AJ....157...72J, doi:10.3847/1538-3881/aaf87f, S2CID 119096973

[17] Ryu, Yoon-Hyun; Mróz, Przemek; Gould, Andrew; Hwang, Kyu-Ha; Kim, Hyoun-Woo; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Jung, Youn Kil; Shin, In-Gu; Shvartzvald, Yossi; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Han, Cheongho; Pogge, Richard W.; Udalski, Andrzej; Poleski, Radek; Skowron, Jan; Szymański, Michał K.; Soszyński, Igor; Pietrukowicz, Paweł; Kozłowski, Szymon; Ulaczyk, Krzysztof; et al. (2021), "KMT-2017-BLG-2820 and the Nature of the Free-Floating Planet Population", The Astronomical Journal, 161 (3): 126, arXiv:2010.07527, Bibcode:2021AJ....161..126R, doi:10.3847/1538-3881/abd55f, S2CID 222378863

[18] Winters, Jennifer G.; et al. (2019), "Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M-dwarf System at 6.9 pc", The Astronomical Journal, 158 (4): 152, arXiv:1906.10147, Bibcode:2019AJ....158..152W, doi:10.3847/1538-3881/ab364d, S2CID 195584444

[19] Kondo, Iona; et al. (2019), "MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star", The Astronomical Journal, 158 (6): 224, arXiv:1905.01239, Bibcode:2019AJ....158..224K, doi:10.3847/1538-3881/ab4e9e, S2CID 145052576

[20] Eigmüller, Philipp; et al. (2019), "NGTS-5b: A highly inflated planet offering insights into the sub-Jovian desert", Astronomy & Astrophysics, 625: A142, arXiv:1905.02593, Bibcode:2019A&A...625A.142E, doi:10.1051/0004-6361/201935206, S2CID 146809360

[21] Vines, Jose I.; et al. (2019), "NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf", Monthly Notices of the Royal Astronomical Society, 489 (3): 4125–4134, arXiv:1904.07997, doi:10.1093/mnras/stz2349

[22] OGLE-2018-BLG-0532Lb: Cold Neptune With Possible Jovian Sibling, 2020, arXiv:1905.08148

[23] "The Extrasolar Planet Encyclopaedia — TOI-813 b". exoplanet.eu.

[Nielsen2019-24] Nielsen, L. D.; Gandolfi, D.; Armstrong, D. J.; Jenkins, J. S.; Fridlund, M.; Santos, N. C.; Dai, F.; Adibekyan, V.; Luque, R.; Steffen, J. H.; Esposito, M.; Meru, F.; Sabotta, S.; Bolmont, E.; Kossakowski, D.; Otegi, J. F.; Murgas, F.; Stalport, M.; Rodler, F.; Díaz, M. R.; Kurtovic, N. T.; Ricker, G.; Vanderspek, R.; Latham, D. W.; Seager, S.; Winn, J. N.; Jenkins, J. M.; Allart, R.; Almenara, J. M.; et al. (2020), "Mass determinations of the three mini-Neptunes transiting TOI-125", Monthly Notices of the Royal Astronomical Society, 492 (4): 5399, arXiv:2001.08834, Bibcode:2020MNRAS.492.5399N, doi:10.1093/mnras/staa197

[25] "exoplanet.eu toi-125_c".

[26] "exoplanet.eu toi-125_d".

[Kipping2019-27] Teachey, Alex; Jansen, Tiffany; Bakos, Gaspar; Torres, Guillermo; Hartman, Joel; Nesvorný, David; Kipping, David (2019). "A resonant pair of warm giant planets revealed by TESS". Monthly Notices of the Royal Astronomical Society. 486 (4): 4980–4986. arXiv:1902.03900. doi:10.1093/mnras/stz1141.

[Dawson2019-28] Dawson, Rebekah I.; et al. (2019). "TOI-216b and TOI-216 c: Two Warm, Large Exoplanets in or Slightly Wide of the 2:1 Orbital Resonance". The Astronomical Journal. 158 (2): 65. arXiv:1904.11852. Bibcode:2019AJ....158...65D. doi:10.3847/1538-3881/ab24ba. S2CID 135466349.

[Dawson2021-29] Dawson, Rebekah I.; Huang, Chelsea X.; Brahm, Rafael; Collins, Karen A.; Hobson, Melissa J.; Jordán, Andrés; Dong, Jiayin; Korth, Judith; Trifonov, Trifon; Abe, Lyu; Agabi, Abdelkrim; Bruni, Ivan; Butler, R. Paul; Barbieri, Mauro; Collins, Kevin I.; Conti, Dennis M.; Crane, Jeffrey D.; Crouzet, Nicolas; Dransfield, Georgina; Evans, Phil; Espinoza, Néstor; Gan, Tianjun; Guillot, Tristan; Henning, Thomas; Lissauer, Jack J.; Jensen, Eric L. N.; Sainte, Wenceslas Marie; Mékarnia, Djamel; Myers, Gordon; et al. (2021), "Precise transit and radial-velocity characterization of a resonant pair: a warm Jupiter TOI-216c and eccentric warm Neptune TOI-216b", The Astronomical Journal, 161 (4): 161, arXiv:2102.06754, Bibcode:2021AJ....161..161D, doi:10.3847/1538-3881/abd8d0, S2CID 231924886

[sorae-30] "太陽系外惑星「TOI 270 b、c、d」を発見。地球外生命体の存在は？". sorae. 2019-07-30. Retrieved 2021-01-08.

[Eylen2021-31] Van Eylen, Vincent; Astudillo-Defru, Nicola; Bonfils, Xavier; Livingston, J.; Hirano, T.; Luque, Rafael; Lam, K. W. F.; Justesen, A. B.; Winn, J. N.; Gandolfi, D.; Nowak, G.; Palle, E.; Albrecht, S.; Dai, F.; Campos Estrada, B.; Owen, J. E.; Foreman-Mackey, D.; Fridlund, M.; Korth, J.; Mathur, S.; Forveille, Thierry; Mikal-Evans, T.; Osborne, H. L. M.; Ho, C. S. K.; Almenara, José M.; Artigau, Étienne; Barragán, O.; Bouchy, François; Cabrera, J.; et al. (2021), "Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley", Monthly Notices of the Royal Astronomical Society, arXiv:2101.01593, doi:10.1093/mnras/stab2143

[:0-32] Davis, Allen B.; Wang, Songhu; et al. (2020). "TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS". Astronomical Journal. 160 (5): 229. arXiv:1912.10186. Bibcode:2020AJ....160..229D. doi:10.3847/1538-3881/aba49d. hdl:1721.1/134083. S2CID 209444463.

[33] David, Trevor J.; Cody, Ann Marie; Hedges, Christina L.; Mamajek, Eric E.; Hillenbrand, Lynne A.; Ciardi, David R.; Beichman, Charles A.; Petigura, Erik A.; Fulton, Benjamin J.; Isaacson, Howard T.; Howard, Andrew W.; Gagné, Jonathan; Saunders, Nicholas K.; Rebull, Luisa M.; Stauffer, John R.; Vasisht, Gautam; Hinkley, Sasha (2019), "A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau", The Astronomical Journal, 158 (2): 79, arXiv:1902.09670, Bibcode:2019AJ....158...79D, doi:10.3847/1538-3881/ab290f, S2CID 119003936

[David2019-34] David, Trevor J.; Petigura, Erik A.; Luger, Rodrigo; Foreman-Mackey, Daniel; Livingston, John H.; Mamajek, Eric E.; Hillenbrand, Lynne A. (2019), "Four newborn planets transiting the young solar analog V1298 Tau", The Astrophysical Journal, 885 (1): L12, arXiv:1910.04563, Bibcode:2019ApJ...885L..12D, doi:10.3847/2041-8213/ab4c99, S2CID 204008446

[Hellier2019-35] Hellier, Coel; Anderson, D. R.; Barkaoui, K.; Benkhaldoun, Z.; Bouchy, F.; Burdanov, A.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Nielsen, L. D.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ségransan, D.; Smalley, B.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2019), "WASP-South hot Jupiters: WASP-178b, WASP-184b, WASP-185b & WASP-192b", Monthly Notices of the Royal Astronomical Society, 490 (1): 1479, arXiv:1907.11667, Bibcode:2019MNRAS.490.1479H, doi:10.1093/mnras/stz2713

[36] Yang, Hongjing; et al. (2020). "KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field". The Astronomical Journal. 159 (3): 98. arXiv:1908.10011. Bibcode:2020AJ....159...98Y. doi:10.3847/1538-3881/ab660e. S2CID 201646063.

[37] "MASCARA-4 b/bRing-1b - A retrograde hot Jupiter around the bright A3V star HD 85628". GroundAI.

[38] "The Extrasolar Planet Encyclopaedia — OGLE-2016-BLG-1227 b". exoplanet.eu.

[39] "The Extrasolar Planet Encyclopaedia — OGLE-2013-BLG-0911L b". exoplanet.eu.

[barnes2019-40] Barnes, J. R.; et al. (2019-06-11), Frequency of planets orbiting M dwarfs in the Solar neighbourhood, arXiv:1906.04644v1, Bibcode:2019arXiv190604644T.

[Feng2020-41] Feng, Fabo; Shectman, Stephen A.; Clement, Matthew S.; Vogt, Steven S.; Tuomi, Mikko; Teske, Johanna K.; Burt, Jennifer; Crane, Jeffrey D.; Holden, Bradford; Sharon Xuesong Wang; Thompson, Ian B.; Diaz, Matias R.; Paul Butler, R. (2020), Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs, arXiv:2008.07998, doi:10.3847/1538-4365/abb139, S2CID 221150644

[Quirrenbach2022-42] The CARMENES search for exoplanets around M dwarfs Two Saturn-mass planets orbiting active stars, 2022, arXiv:2203.16504

[KostovSchlieder2019-43] Kostov, Veselin B.; Schlieder, Joshua E.; et al. (2019). "The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf". The Astronomical Journal. 158 (1): 32. arXiv:1903.08017. Bibcode:2019AJ....158...32K. doi:10.3847/1538-3881/ab2459. hdl:1721.1/124742. ISSN 1538-3881. S2CID 118855908.

[DemangeonZapatero_Osorio2021-44] Demangeon, O. D. S.; Zapatero Osorio, M. R.; Alibert, Y.; Barros, S. C. C.; Adibekyan, V.; Tabernero, H. M.; Antoniadis-Karnavas, A.; Camacho, J. D.; al, et (2021). "Warm terrestrial planet with half the mass of Venus transiting a nearby star" (PDF). Astronomy & Astrophysics. 653: A41. arXiv:2108.03323. Bibcode:2021A&A...653A..41D. doi:10.1051/0004-6361/202140728. S2CID 236957385.

[45] "Planet L 98-59 b". exoplanet.eu. Retrieved 6 August 2021.

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]

[9]

[10]

[11]

[12]

[13]

[14]

[15]

[16]

[17]

[18]

[19]

[20]

[21]

[22]

[23]

[24]

[25]

[26]

[27]

[28]

[29]

[30]

[31]

[32]

[33]

[34]

[35]

[36]

[37]

[38]

[39]

[40]

[41]

[42]

[43]

[44]

[45]

v t 2019년 우주여행
§ 2018년 2020년 »
우주 탐사선 기동하다	베레시트 (달 착륙선; 2019년 2월) LightSail 2 (솔라 세일 시연, 2019년 6월) 찬드라얀-2 / 비크람 / 프라얀 (달 궤도선, 착륙선, 탐사선; 2019년 7월)
영향 이벤트	캄차카 운석(발표) 2019 MO
선택된 NEO	소행성 근접 접근 2018 XB4 2019 AS5 2016년 AZ8 66391 모슈업 2019년 OK 1620 지리 2006년 QV89 2100 라샬롬 2019년 SU3 2019년 TA7 2019년 UN13
외계 행성	AD 레오니스 b 베타 픽토리스 c DS 투카나에 b 글리제 251 c 글리제 357 d 글리제 588 b c 글리제 687 c 글리제 555 b 글리제 754 b 글리제 784 b HR 5183 b 케플러-47d 확인 K2-288Bb L 1159-16 b c d LP 816-60 b LTT 1445 Ab 루이텐의 별 d e PDS 70c 센타우루스자리 프록시마 c 스트루베 2398 Bb Bc Tau Cetii i(저체화) 티가든의 별 b c V1298 타우리 b c d e 울프 359 b c
검출	2019년 AQ3 ASASSN-19bt AT2019qiz GRB 190114c EPIC 204376071 GW190412 GW190521g(bh-bh 합병으로 인한 사상 최초의 빛) GW190814(최초 '매스갭' 충돌) K2-18b 수증기 M87*이미지 PSR J0030+0451 매핑 PSR J0740+6620 S5-HVS1 2I/보리소프 토성의 20개 위성 WD 0145+234 엑소스테로이드 교란 검출 WD J0914+1914
혜성	289P/블랑페인 78P/게렐 168P/Hergenrother 163P/NEAT 138P/슈메이커-부담금 171P/Spahr
우주 탐사	뉴호라이즌스 (486958 Arrokoth와 비교; 2018년 12월 / 2019년 1월) 창어4 / 유투-2 (달 뒷면 착륙, 2019년 1월) 오퍼튜니티 (미션 종료; 2018년 8월 / 2019년 2월) 하야부사2 (162173류구에서 출발, 2019년 12월)
우주 포털 카테고리:2018 in space — 카테고리:2019 in space — 카테고리:2020 in space

Search

2019년 발견된 외계 행성 목록

특정 외계 행성 목록

레퍼런스