List of transiting exoplanets

Last updated December 17, 2024

This is a list of transiting extrasolar planets sorted by orbital periods. As of 2024, 4195 transiting exoplanets have been discovered.^[1] This list consist of all transiting exoplanets through 2012, and notable discoveries since. All the transiting planets have true masses, radii and most have known inclinations. Radius is determined by how much the star dims during the transit and inclination is determined^{[ clarification needed ]} from Rossiter–McLaughlin effect. True mass is determined by the minimum mass determined from radial velocity observations divided by the sine of inclination.

The first known planet to be discovered with the transit method was OGLE-TR-56b. The first planetary transit observed (by already known exoplanet) was caused by HD 209458 b. The most massive transiting exoplanet is KELT-1b which masses 27.23 M_J (making it a brown dwarf) while the least massive is Kepler-42d which masses less than 0.003 M_J or 0.9 M_E.^[2] The largest exoplanet known is HAT-P-32b which is 2.037 R_J. The smallest exoplanet known is also Kepler-42d which is 0.051 R_J or 0.57 R_🜨. The densest transiting exoplanet known is CoRoT-3b, which has density of 26.4 g/cm³; the diffusest transiting planet known is Kepler-12b, which has density of only 0.111 g/cm³. Previously, the longest period of any transiting planets was Kepler-1647b, which takes 1107 days to orbit its (double) stars.^[3]^[4] Only two years later, the longest period of a transiting planet was more than tripled by EPIC 248847494 b, which takes 3650 days to orbit its star. The shortest period is K2-137b, which takes just 0.18 days to orbit its star.

There are 60 members of multi-planet systems.

Yellow rows denote members of a multi-planet system

Planet ^[1]	Mass (M_J)	Radius (R_J)	Density (g/cm³)	Temperature (K)	Period (d)	Semi-major axis (AU)	Eccentricity	Inclination (°)	Year of discovery
TOI-6883 b	4.34	1.087		805.5	16.25	0.129			2024
SPECULOOS-3 b		0.08716		553	0.719	0.00733			2024
IRAS 04125+2902 b	0.3	0.955			8.83				2024
HD 63433 d		0.09573		1040	4.21	0.0503			2024
WASP-193b	0.139	1.464		1254	6.2463345	0.0676			2023
TOI-5678 b	0.063	0.438		513	47.73022	0.249			2023
TOI-4603 b	12.89	1.042		1677	7.24599	0.0888			2023
TOI-4127 b	2.30	1.096		605.1	56.39879	0.3081			2023
TOI-3235 b	0.665	1.017		604	2.59261842	0.02709			2023
TOI-715 b		0.1383		234	19.288004	0.0830			2023
TOI-700 e	0.0025730809	0.08502		350	27.80978	0.134			2023
TOI-672 b	0.0760	0.470		676.15	3.633575				2023
LHS 475 b	0.002876	0.0883		586	2.029088	0.0206			2023
K2-415b	0.0094	0.091		412	4.0179694	0.0270			2023
TOI-2180 b	2.755	1.010		348	260.79	0.828			2022
TOI-1452 b	0.0152	0.149		326	11.06201	0.061			2022
Kepler-1708b	<4.6	0.8886			737.11310	1.64			2022
TOI-2257 b		0.196		256	35.189346	0.145			2021
TOI-1601 b	0.99	1.239		1619	5.331751	0.06864			2021
TOI-1478 b	0.847	1.061		918	10.180249	0.0903			2021
TOI-1431 b	3.14	1.51		2370	2.65022	0.047			2021
TOI-1227 b		0.854			27.36397	0.0886			2021
TOI-640 b	0.88	1.771		1749	5.0037775	0.06608			2021
TOI-628 b	6.33	1.060		1586	3.4095675	0.04860			2021
TOI-178c	0.015	0.149		873	3.238450	0.0370			2021
TOI-4138 b	0.67	1.49		1762	3.660028	0.051			2021
NGTS-14Ab	0.092	0.444		1143	3.5357173	0.0403			2021
NGTS-13b	4.84	1.142		1605	4.12	0.0549			2021
Kepler-1704b	4.15	1.065		253.8	988.88113	2.026			2021
Gliese 367 b	0.0017	0.064		1745	0.321962	0.0071			2021
TOI-849 b	0.128	0.308		1800	0.7655240	0.01598			2020
TOI-813 b		0.599		610	83.8911	0.423			2020
TOI-700 d	0.00711	0.1062		295	37.426	0.163			2020
TOI-561 b	0.0050	0.127			0.446578	0.01055			2020
K2-315b		0.085		460	3.1443189	0.0234			2020
K2-137b	<0.5	0.057		1471	0.179719	0.0058	0	93.10	2017
Kepler-42c	<0.006	0.065		720	0.45328509	0.006	0		2012
55 Cancri e	0.027	0.194	4.905		0.7365449	0.0156	0.057	81	2004
Kepler-32f		0.073			0.74296	0.01652	0.0126		2012
WASP-19b	1.152	1.310	0.593	2009	0.788840	0.0164	0.0234	99.206	2009
WASP-43b	1.782	0.930	2.938		0.813475	0.0142	0.0076	82.657	2011
Kepler-10b	0.014	0.127	8.849	1833	0.837495	0.0168	0.0003	95.567	2011
CoRoT-7b	0.0151	0.15	5.275	1656	0.853585	0.0172	0	80.1	2009
WASP-18b	10.425	1.165	7.724		0.941452	0.0204	0.0088	85.962	2009
WTS-1b	0.504	0.916	0.759		1.083904	0.0185	0.0082	81.251	2012
WASP-12b	1.389	1.834	0.260	2525	1.091423	0.0229	0.0490	96.927	2008
OGLE-TR-56b	1.316	1.300	0.700	1973	1.211909	0.0235	0.0012	101.205	2003
HAT-P-23b	2.087	1.368	0.952		1.212884	0.0232	0.1059	85.059	2010
Kepler-42b	<0.009	0.07		519	1.2137672	0.0116	0		2012
Kelt-1b	27.23	1.11			1.217514	0.02466			2012
WASP-33b	3.841	1.497	1.325		1.219867	0.0255	0.0374	87.670	2010
TrES-3b	1.924	1.295	1.036		1.306190	0.0226	0.0166	98.275	2007
HAT-P-36b	1.832	1.264			1.327347	0.0238	0.063	86	2012
Qatar-2b	2.487	1.144			1.3371182	0.02149	0	88.3	2011
WASP-4b	1.122	1.363	0.587	1653	1.338228	0.0231	0.0025	88.751	2007
WASP-77Ab	1.667	1.23		1715	1.36002854	0.02335	00.0074		2012
Qatar-1b	1.090	1.164	0.803		1.420033	0.0234	0.0028	96.535	2010
WASP-46b	2.101	1.310	1.238		1.430370	0.0245	0.0007	82.629	2011
OGLE-TR-113b	1.317	1.090	1.205		1.432476	0.0229	0.0064	90.574	2004
TrES-5b	1.778	1.209			1.4822446	0.02446	0	84.529	2011
Kepler-17b	2.45	1.31	1.35	1570	1.4857108	0.02591	<0.011	87.2	2011
CoRoT-1b	1.03	1.49	0.413	1898	1.5089557	0.0254	0	85.1	2007
CoRoT-14b	7.6	1.09	6.886		1.51214	0.027	0	79.6	2010
WASP-36b	2.447	1.373	1.160		1.547288	0.0277	0.0384	88.785	2010
WASP-64b	1.271	1.271		1689	1.5732918	0.02648	0		2012
GJ 1214 b	0.021	0.245	1.745	516	1.580393	0.0142	0.0982	88.619	2009
Kepler-9d	0.022	0.147	9.460		1.592851	0.0267	0.0109	87.666	2010
WASP-64b	1.2	0.7			1.6				2011
WASP-5b	1.637	1.171	1.206	1732	1.628425	0.0273	0.0032	85.779	2007
OGLE-TR-132b	1.144	1.175	0.834		1.689868	0.0300	0.0032	95.209	2004
WASP-52b	0.5	1.3			1.7				2011
CoRoT-2b	3.673	1.545	1.321	1537	1.742996	0.0294	0.0083	92.157	2007
KOI-13b	8.3	1.83			1.7637				2011
SWEEPS-11 b	9.665	1.135	8.047		1.795546	0.0289	0.0124	86.045	2006
WASP-3b	2.060	1.454	0.797	1983	1.846837	0.0317	0.0020	85.064	2007
Kepler-41b	0.49	0.841	1.02	1930	1.855558	0.029	0	88.3	2011
Kepler-42d	<0.003	0.051		450	1.856169	0.0154	0		2012
CoRoT-18b	3.47	1.31	2.05		1.9000693	0.0295	<0.08	86.5	2011
WASP-50b	1.468	1.153			1.9550959	0.02945	0.009	44	2011
WASP-48b	0.977	1.671	0.277		2.143634	0.0344	0.0177	80.088	2011
HAT-P-32b	0.941	2.037			2.150009	0.0344	0.163	52	2011
WASP-2b	0.847	1.079	0.801	1300	2.152225	0.0308	0.0089	95.197	2006
HAT-P-7b	1.802	1.421	0.755	2729	2.204730	0.0377	0.0524	95.891	2008
HD 189733 b	1.127	1.138	0.901	1117	2.218573	0.0309	0.0059	85.756	2005
WASP-14b	7.725	1.259	4.759	2779	2.243770	0.0368	0.0903	95.205	2008
WASP-65b	1.6	1.3			2.3				2011
WASP-24b	1.032	1.104	0.897		2.341208	0.0359	0.0378	83.644	2010
WASP-44b	0.889	1.144	0.787		2.423804	0.0347	0.0009	86.022	2011
KOI-254b	0.505	0.96	0.8	1000	2.455239	0.030	0.11	87.0	2012
TrES-2b	1.199	1.272	0.687		2.470627	0.0356	0.0277	96.375	2006
OGLE2-TR-L9b	4.336	1.614	1.253		2.485534	0.0413	0.0178	97.526	2008
WASP-1b	0.859	1.484	0.310	1833	2.519945	0.0389	0.0067	96.077	2006
XO-2b	0.573	0.973	0.742		2.615838	0.0369	0.0325	91.208	2007
Gliese 436 b	0.0737	0.365	2.01		2.6438986	0.02887	0.12	85.8	2004
WASP-32b	3.601	1.183	2.653		2.718650	0.0394	0.0179	94.663	2010
CoRoT-21b	2.26	1.3	1.36		2.72474	0.0417	0	86.8	2011
WASP-26b	1.027	1.316	0.536		2.756601	0.0399	0.0019	82.513	2010
HAT-P-16b	4.193	1.289	2.316		2.775962	0.0413	0.0358	93.411	2010
Kepler-21b	<0.033	0.1459	<12.9	1956	2.785755	0.0425	0	82.58	2011
HAT-P-5b	1.06	1.274	0.390		2.788491	0.0407	0.0141	86.753	2007
HAT-P-37b	1.169	1.169			2.797436	0.0379	0.058	86.9	2012
WASP-49b	0.4	1.3			2.8				2011
WASP-57b	0.8	1.1			2.8				2011
HAT-P-31b/WASP-51b	0.711	1.34			2.810595	0.0419	0.0089	83.6	2011
CoRoT-12b	0.917	1.44	0.407		2.828042	0.04016	0.07	85.48	2010
HAT-P-20b	7.246	0.867	13.809		2.875317	0.0361	0.0272	86.467	2010
HD 149026 b	0.360	0.813	0.811	2359	2.875889	0.0437	0.0073	83.345	2005
HAT-P-3b	0.591	0.827	1.386		2.899703	0.0387	0.0021	87.074	2007
HAT-P-13b	0.851	1.284	0.484		2.916293	0.0427	0.0142	96.726	2009
WASP-23b	0.875	0.963	1.146		2.937160	0.0379	0.0003	84.436	2010
CoRoT-11b	2.33	1.43	1.057		2.99433	0.0436	0	83.17	2010
KOI-135b	3.23	1.2	2.33	1637	3.024095	0.0449	< 0.025		2011
TrES-1b	0.613	1.081	0.573	1063	3.030065	0.0392	0.0570	88.410	2004
HAT-P-27b/WASP-40b	0.617	1.055	0.797		3.039572	0.0399	0.0007	84.983	2011
WASP-41b	0.923	1.211	0.611		3.052394	0.0405	0.0002	92.664	2010
HAT-P-4b	0.599	0.890	1.027		3.056536	0.0445	0.0165	89.923	2007
HAT-P-8b	1.341	1.497	0.530		3.076337	0.0449	0.0201	92.227	2008
WASP-10b	3.058	1.078	2.962		3.092762	0.0371	0.0568	86.838	2008
OGLE-TR-10b	0.626	1.263	0.369		3.101286	0.0439	0.0026	95.495	2002
WASP-16b	0.855	1.008	1.013		3.118601	0.0421	0.0023	94.782	2009
WASP-45b	1.007	1.157	0.863		3.126088	0.0405	0.0008	84.470	2011
WASP-35b	0.722	1.324	0.412		3.161575	0.0432	0.0027	87.960	2011
XO-3b	11.791	1.217	8.600		3.191524	0.0452	0.2576	84.215	2007
HAT-P-22b	2.147	1.081	2.078		3.212220	0.0415	0.0274	91.267	2010
HAT-P-12b	0.211	0.959	0.281		3.213060	0.0385	0.0516	88.946	2009
Kepler-4b	0.077	0.357	2.050	1647	3.213457	0.0456	0.0038	89.757	2010
Kepler-6b	0.669	1.323	0.354	1661	3.234230	0.0456	0.0186	86.813	2010
HAT-P-24b	0.685	1.242	0.422		3.355240	0.0465	0.0671	88.628	2010
WASP-6b	0.504	1.224	0.327	1293	3.361006	0.0418	0.0540	88.466	2008
WASP-31b	0.478	1.537	0.155		3.405909	0.0465	0.0013	84.542	2010
WASP-28b	0.910	1.117	0.785		3.408821	0.0455	0.0463	89.100	2010
HAT-P-33b	0.763	1.827			3.474474	0.0503	0.148	86.7	2011
Kepler-18b	0.0217	0.179	4.9	1179	3.504725	0.0447	0	84.92	2011
Kepler-8b	0.603	1.419	0.259	1764	3.522540	0.0483	0.0892	95.932	2010
HD 209458 b	0.685	1.325	0.369	1129	3.524749	0.0454	0.0709	86.677	1999
WASP-22b	0.565	1.122	0.471		3.532687	0.0467	0.0229	89.245	2010
Kepler-5b	2.114	1.431	0.882	1928	3.548465	0.0506	0.0071	86.282	2010
TrES-4b	0.919	1.799	0.193	1782	3.553945	0.0487	0.0136	82.857	2006
WASP-37b	1.696	1.136	1.369		3.577471	0.0434	0.0043	88.779	2010
CoRoT-23b	2.8	1.05	3.21		3.6314	0.0477	0.16	85.7	2011
HAT-P-35b	1.054	1.332			3.646706	0.0498	0.025	87.3	2012
HAT-P-25b	0.567	1.190	0.397		3.652836	0.0466	0.0322	87.561	2010
OGLE-TR-211b	0.918	1.329	0.481		3.677240	0.0509	0.0689	92.831	2007
Kepler-20b	0.027	0.170	6.5	1024	3.6961219	0.04537	<0.32	86.50	2011
WASP-54b	0.6	1.4			3.7				2011
WASP-70b	0.6	0.8			3.7				2011
WASP-11b/HAT-P-10b	0.462	1.035	0.500	1030	3.722469	0.0440	0.1710	88.509	2008
WASP-17b	0.491	1.736	0.114		3.735442	0.0500	0.1286	92.246	2009
WASP-15b	0.542	1.428	0.229	1496	3.752066	0.0500	0.0236	94.526	2008
WASP-25b	0.578	1.258	0.343		3.764831	0.0473	0.0216	87.704	2010
CoRoT-17b	2.449	1.023	3.037		3.768125	0.0475	0.0004	91.660	2010
WASP-61b	1.7	1.4			3.8				2011
HAT-P-6b	1.055	1.264	0.650		3.852985	0.0523	0.0024	85.505	2007
CoRoT-19b	1.11	1.45	0.48		3.89713	0.0518	0.047	87.61	2011
WASP-69b	0.3	1			3.9				2011
Lupus-TR-3b	0.712	0.932	1.090		3.914049	0.0463	0.2178	91.736	2007
WASP-29b	0.244	0.792	0.584		3.922727	0.0456	0.0273	91.237	2010
HAT-P-9b	0.671	1.398	0.555		3.922814	0.0528	0.0012	86.467	2008
XO-1b	0.937	1.184	0.678		3.941534	0.0489	0.0110	90.690	2006
OGLE-TR-182b	1.008	1.132	0.844		3.979100	0.0519	0.0114	94.280	2007
WASP-20b	0.3	0.9			4				2011
HAT-P-19b	0.292	1.133	0.232		4.008778	0.0466	0.0674	88.235	2010
OGLE-TR-111b	0.529	1.022	0.603		4.014448	0.0463	0.0049	91.900	2004
CoRoT-13b	1.308	0.885	2.503		4.03519	0.051	0	88.02	2010
CoRoT-5b	0.856	1.211	0.577		4.037896	0.0496	0.0935	85.833	2008
WASP-39b	0.277	1.267	0.181	1116	4.05526	0.0486	0.0057	87.833	2011
WASP-47b	1.1	1.2			4.1				2011
WASP-66b	1.9	1.5			4.1				2011
HAT-P-21b	4.063	1.024	4.588		4.124461	0.0495	0.0477	87.484	2010
XO-4b	1.721	1.338	0.893		4.125020	0.0552	0.0025	88.680	2008
XO-5b	1.151	1.154	0.937		4.187754	0.0487	0.0029	93.164	2008
SWEEPS-04 b	3.653	0.814	8.672		4.201572	0.0547	0.0219	92.090	2006
HAT-P-26b	0.059	0.565	0.431		4.234516	0.0479	0.1244	88.582	2010
CoRoT-3b	21.66	1.01	26.4		4.2568	0.057	0	85.9	2008
WASP-60b	0.5	0.9			4.3				2011
WASP-34b	0.591	1.218	0.378		4.317678	0.0521	0.0382	85.201	2010
WASP-21b	0.301	1.067	0.296		4.322482	0.0520	0.0029	91.250	2010
WASP-13b	0.457	1.209	0.313	1403	4.352977	0.0546	0.0147	93.073	2008
WASP-62b	0.5	1.5			4.4				2011
WASP-63b	0.3	1			4.4				2011
Kepler-12b	0.431	1.695	0.111	1361	4.4379637	0.0556	<0.01	88.76	2011
HAT-P-1b	0.590	1.355	0.292		4.465293	0.0552	0.0904	85.896	2006
WASP-55b	0.6	1.4			4.5				2011
WASP-56b	0.6	1.2			4.5				2011
WASP-67b	0.4	1.7			4.5				2011
HAT-P-14b	2.232	1.199	1.647		4.627657	0.0606	0.0948	97.152	2010
HAT-P-38b	0.267	0.825			4.640382	0.0523	0.067	88.3	2012
Kepler-93b	0.013	0.132	6.88	1037	4.726740	0.05343	0	89.18	2014
Kepler-7b	0.433	1.478	0.160	1541	4.885525	0.0622	0.3764	86.529	2010
HAT-P-11b	0.081	0.452	1.076	878	4.887816	0.0525	0.1980	91.496	2009
Kepler-15b	0.66	0.96	0.93	1111	4.942782	0.05714	0.06	87.44	2011
WASP-7b	0.960	0.915	1.515	1997	4.954658	0.0617	0.0323	90.370	2008
WASP-42b	0.6	1			5				2011
WASP-58b	1.1	1.3			5				2011
HAT-P-31b	2.171	1.07			5.005425	0.055	0.245	87.1	2011
WASP-68b	0.8	0.9			5.1				2011
CoRoT-16b	0.497	0.813	1.118		5.353421	0.0578	0.0292	94.178	2010
HAT-P-34b	3.328	1.107			5.452654	0.0677	0.441	87.1	2012
HAT-P-18b	0.197	0.995	0.232		5.508023	0.0560	0.0842	91.201	2010
HAT-P-2b	9.090	1.157	7.522	1187	5.633473	0.0676	0.5171	86.722	2007
Kepler-33b		0.16			5.66793	0.0677		86.39	2012
HAT-P-29b	0.778	1.107			5.72318	0.0667	0.095	87.1	2011
Kepler-32b	4.1	0.37		542	5.90124	0.05			2012
Kepler-28b	<1.51	0.32			5.9123	0.062			2012
Kepler-20e	<0.005	0.077		1040	6.098493	0.0507	<0.28	87.50	2011
COROT-8b	0.222	0.572	1.436		6.212295	0.0634	0.0043	88.435	2010
Kepler-25b	<12.7	0.23			6.2385	0.068			2012
Kepler-14b	8.40	1.136	7.1		6.7901230		0.035	90.0	2011
WASP-38b	2.712	1.079	2.746	1292	6.871815	0.0755	0.0321	88.692	2010
Kepler-40b	2.217	1.175	1.824	1618	6.873495	0.0807	0.0039	89.716	2010
Kepler-23b	<0.8	0.17			7.1073	0.075			2012
Kepler-223e		0.18			7.3831	0.076			2011
Kepler-18c	0.054	0.489	0.59	909	7.64159	0.0752	0	87.68	2011
WASP-59b	0.7	0.9			7.9				2011
Kepler-24b	<1.6	0.21			8.1453				2012
WASP-8b	2.233	1.172	1.749		8.158716	0.0742	0.3082	88.516	2008
Kepler-32c	0.5	0.33		475	8.7522	0.09			2012
CoRoT-6b	2.959	1.166	2.319		8.886903	0.0855	0.0278	94.581	2009
Kepler-28c	<1.36	0.3			8.9858	0.081			2012
CoRoT-20b	4.24	0.84	9.49		9.20	0.0902	0.562	88.21	2011
CoRoT-4b	0.728	1.168	0.561	1074	9.202047	0.0887	0.0019	89.779	2008
Kepler-19b	<0.06	0.2	<7.76	714	9.2869944	0.0853	0	89.94	2011
HD 97658 b	0.02	0.262			9.4957	0.0797	0.13		2010
KOI-730c		0.23			9.8499		0.092		2011
KIC 10905746 b		0.237			9.8844		88.42		2011
Kepler-11b	0.014	0.176	3.280		10.303751	0.0912	0.0025	88.505	2011
Kepler-29b	0.4	0.32		815	10.3376	0.09			2012
HAT-P-17b	0.526	1.011	0.636	814	10.338520	0.0882	0.3455	89.182	2010
Kepler-23c	<2.7	0.29			10.7421	0.099			2012
Kepler-20c	0.051	0.273	2.91	713	10.854092	0.0930	<0.40	88.39	2011
HAT-P-15b	1.946	1.072	1.936		10.863502	0.0964	0.1898	89.054	2010
Kepler-26b	<0.38	0.32			12.2829	0.085			2012
Kepler-24c	<1.6	0.25			12.3335	0.106			2012
Kepler-25c	<4.16	0.4			12.7204	0.11			2012
Kepler-11c	0.043	0.282	2.519		13.025021	0.1064	0.0076	88.986	2011
Kepler-33c		0.29			13.17562	0.1189		89.46	2012
CoRoT-10b	2.75	0.97	3.997		13.2406	0.1055	0.53	88.55	2010
Kepler-29c	0.3	0.26		749	13.2907	0.11			2012
KOI-730b		0.31			14.7903	0.12			2011
Kepler-18d	0.051	0.62	0.27	728	14.85888	0.1172	0	88.07	2011
Kepler-27b	<9.11	0.36			15.3348	0.118			2012
Kepler-9b	0.252	0.842	0.536		19.243158	0.1405	0.0297	88.553	2010
Kepler-20f	<0.010	0.092		705	19.57706	0.1104	<0.32	88.68	2011
Kepler-223d		0.25			19.7216	0.145			2011
Kepler-31b	<6.8	0.38		776	20.8613				2012
Mulchatna	3.125	1.095	3.065		21.214398	0.1626	0.6696	86.486	2007
Kepler-33d		0.48			21.77596	0.1662		88.71	2012
Kepler-11d	0.019	0.307	0.882		22.687189	0.1586	0.0044	90.713	2011
Kepler-30b	0.2	0.33		548	29.329	0.18			2012
Kepler-27c	<13.8	0.44			31.3309	0.191			2012
Kepler-33e		0.36			31.7844	0.2138		89.576	2012
Kepler-11e	0.026	0.404	0.531		31.995899	0.1935	0.0065	88.788	2011
Kepler-9c	0.171	0.823	0.393		38.908610	0.2246	0.0337	88.124	2010
Kepler-33f		0.4			41.02902	0.2535		89.772	2012
Kepler-31c	4.7	0.38		612	42.6318	0.26			2012
Kepler-10c	<0.063	0.199	<10	485	45.29485	0.2407		89.65	2011
Kepler-11f	0.007	0.234	0.754		46.688756	0.2501	0.0018	90.614	2011
Kepler-943b		0.72			49.76971	0.2672		89.2	2011
Kepler-30c	9.1	1.29		431	60.3251	0.30			2012
Kepler-20d	<0.063	0.245	<4.07	369	77.61184	0.3453	<0.60	89.570	2011
Kepler-991b		0.227			82.5342519				2016
CoRoT-9b	0.838	1.045	0.945	377	95.273774	0.4070	0.1127	37.383	2010
HD 80606 b	3.945	1.029	4.741	347	111.436366	0.4309	0.9337	89.285	2001
Kepler-11g	0.019	0.327	0.725		118.377738	0.4617	0.0097	89.754	2011
Kepler-35b	0.127	0.728	0.410		131.458	0.60347	0.042	90.76	2012
PH1b	0.531	.551		481	138.317	0.652	0.0702	90.050	2012
Kepler-30d	17	0.96		323	143.213	0.5			2012
Kepler-16b	0.333	0.7538	0.964	170-200	228.776	0.7048	0.0069	90.0322	2011
Kepler-34b	0.22	0.764	0.410		288.822	1.0896	0.182	90.355	2012
Kepler-22b	<0.11	0.212	<14.7	262	289.8623	0.849	0	89.764	2011
Kepler-1647b ^[3]^[4]	1.06	1.52			1107	2.7205	0.0581	90.1	2016
EPIC 248847494 b	<13	1.11		183	3650	4.5	0	89.87	2018
Kepler-560b		0.153							2016
Kepler-1649b									2017
Kepler-1649c									2020
Kepler-1662b									2020
Kepler-1652b									2017
Kepler-1514b									2016
Kepler-1514c									2020
Kepler-1544b		0.159							2016

External links and references

"Transiting planets". Extrasolar Planets Encyclopaedia . 1995. Retrieved 2012-04-01.
"Exoplanets Data Explorer" . Retrieved 2011-01-20.

1 2 "NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 2024-03-19.
↑ NASA.gov
1 2 Astronomers Discover Circumbinary Planet 3,700 Light-Years Away
1 2 New planet is largest discovered that orbits two suns

Related Research Articles

This page describes exoplanet orbital and physical parameters.

Kepler-7b is one of the first five exoplanets to be confirmed by NASA's Kepler spacecraft, and was confirmed during the first 34 days of Kepler's science operations. It orbits a star slightly hotter and significantly larger than the Sun that is expected to soon reach the end of the main sequence. Kepler-7b is a hot Jupiter that is about half the mass of Jupiter, but is nearly 1.5 times its size; at the time of its discovery, Kepler-7b was the second most diffuse planet known, surpassed only by WASP-17b. It orbits its host star every five days at a distance of approximately 0.06 AU. Kepler-7b was announced at a meeting of the American Astronomical Society on January 4, 2010. It is the first extrasolar planet to have a crude map of cloud coverage.

Kepler-5b is one of the first five planets discovered by NASA's Kepler spacecraft. It is a hot Jupiter that orbits a subgiant star that is more massive, larger, and more diffuse than the Sun is. Kepler-5 was first flagged as the location of a possibly transiting planet, and was reclassified as a Kepler Object of Interest until follow-up observations confirmed the planet's existence and many of its characteristics. The planet's discovery was announced at a meeting of the American Astronomical Society on January 4, 2010. The planet has approximately twice the mass of Jupiter, and is about 1.5 times larger. It is also fifteen times hotter than Jupiter. Kepler-5b orbits Kepler-5 every 3.5 days at a distance of approximately 0.051 AU.

Kepler-8 is a star located in the constellation Lyra in the field of view of the Kepler Mission, a NASA-led operation tasked with discovering terrestrial planets. The star, which is slightly hotter, larger, and more massive than the Sun, has one gas giant in its orbit, Kepler-8b. This gas giant is larger than Jupiter, but is less massive, and thus more diffuse. The planet's discovery was announced to the public on January 4, 2010 along with four other planets. As the fifth confirmed planetary system verified by Kepler, it helped demonstrate the capabilities of the Kepler spacecraft.

Kepler-9c is one of the first seven extrasolar planets, exoplanets, discovered by NASA's Kepler Mission, and one of at least two planets orbiting the star Kepler-9. Kepler-9c and Kepler-9b were the first exoplanets confirmed to be transiting their star. The planet's discovery was announced by the Kepler Mission team on August 26, 2010 after its initial discovery by Kepler. At the time, it was one of 700 planetary candidates noted by Kepler.

<span class="mw-page-title-main">Discoveries of exoplanets</span> Detecting planets located outside the Solar System

An exoplanet is a planet located outside the Solar System. The first evidence of an exoplanet was noted as early as 1917, but was not recognized as such until 2016; no planet discovery has yet come from that evidence. What turned out to be the first detection of an exoplanet was published among a list of possible candidates in 1988, though not confirmed until 2003. The first confirmed detection came in 1992, with the discovery of terrestrial-mass planets orbiting the pulsar PSR B1257+12. The first confirmation of an exoplanet orbiting a main-sequence star was made in 1995, when a giant planet was found in a four-day orbit around the nearby star 51 Pegasi. Some exoplanets have been imaged directly by telescopes, but the vast majority have been detected through indirect methods, such as the transit method and the radial-velocity method. As of 24 July 2024, there are 7,026 confirmed exoplanets in 4,949 planetary systems, with 1007 systems having more than one planet. This is a list of the most notable discoveries.

Kepler-10, formerly known as KOI-72, is a Sun-like star in the constellation of Draco that lies 607 light-years from Earth. Kepler-10 was targeted by NASA's Kepler space telescope, as it was seen as the first star identified by the Kepler mission that could be a possible host to a small, transiting exoplanet. The star is slightly less massive, slightly larger, and slightly cooler than the Sun; at an estimated 11.9 billion years in age, Kepler-10 is 2.3 times the age of the Sun.

Kepler-10c is an exoplanet orbiting the G-type star Kepler-10, located around 608 light-years away in Draco. Its discovery was announced by the Kepler space telescope team in May 2011, although it had been seen as a planetary candidate since January 2011, when Kepler-10b was discovered. The team confirmed the observation using data from NASA's Spitzer Space Telescope and a technique called BLENDER that ruled out most false positives. Kepler-10c was the third transiting planet to be confirmed statistically, after Kepler-9d and Kepler-11g. The Kepler team considers the statistical method that led to the discovery of Kepler-10c as what will be necessary to confirm many planets in Kepler's field of view.

Kepler-11b is an exoplanet discovered around the star Kepler-11 by the Kepler space telescope, a NASA-led mission to discover Earth-like planets. Kepler-11b is less than about three times as massive and twice as large as Earth, but it has a lower density, and is thus most likely not of Earth-like composition. Kepler-11b is the hottest of the six planets in the Kepler-11 system, and orbits more closely to Kepler-11 than the other planets in the system. Kepler-11b, along with its five counterparts, form the first discovered planetary system with more than three transiting planets—the most densely packed known planetary system. The system is also the flattest known planetary system. The discovery of this planet and its five sister planets was announced on February 2, 2011, after follow-up investigations.

Kepler-11d is an exoplanet discovered in the orbit of the sun-like star Kepler-11. It is named for the telescope that discovered it, a NASA spacecraft named Kepler that is designed to detect Earth-like planets by measuring small dips in the brightness of their host stars as the planets cross in front. This process, known as the transit method, was used to note the presence of six planets in orbit around Kepler-11, of which Kepler-11d is the third from its star. Kepler-11d orbits Kepler-11 well within the orbit of Mercury approximately every 23 days. The planet is approximately six times more massive than the Earth, and has a radius that is three and a half times larger than that of Earth's. It is, however, far hotter than Earth is. Its low density, comparable to that of Saturn, suggests that Kepler-11d has a large hydrogen–helium atmosphere. Kepler-11d was announced with its five sister planets on February 2, 2011 after extensive follow-up studies.

Kepler-11e is an exoplanet discovered in the orbit of the sunlike star Kepler-11. It is the fourth of six planets around Kepler-11 discovered by NASA's Kepler space telescope. Kepler-11e was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. Kepler-11e is most likely a gas giant like Neptune, having a density that is less than that of Saturn, the least dense planet in the Solar System. Its low density can probably be attributed to a large hydrogen and helium atmosphere. Kepler-11e has a mass eight times of Earth's mass and a radius 4.5 times that of Earth. The planet orbits its star every 31 days in an ellipse that would fit within the orbit of Mercury. Kepler-11e was announced on February 2, 2011 with its five sister planets after it was confirmed by several observatories.

Kepler-11f is an exoplanet discovered in the orbit of the Sun-like star Kepler-11 by NASA's Kepler space telescope, which searches for planets that transit their host stars. Kepler-11f is the fifth planet from its star, orbiting one quarter of the distance of the Earth from the Sun every 47 days. It is the furthest of the first five planets in the system. Kepler-11f is the least massive of Kepler-11's six planets, at nearly twice the mass of Earth; it is about 2.6 times the radius of Earth. Along with planets d and e and unlike the two inner planets in the system, Kepler-11f has a density lower than that of water and comparable to that of Saturn. This suggests that Kepler-11f has a significant hydrogen–helium atmosphere. The Kepler-11 planets constitute the first system discovered with more than three transiting planets. Kepler-11f was announced to the public on February 2, 2011, after follow-up investigations at several observatories. Analysis of the planets and study results were published the next day in the journal Nature.

Kepler-47 is a binary star system in the constellation Cygnus located about 3,420 light-years away from Earth. The stars have three exoplanets, all of which orbit both stars at the same time, making this a circumbinary system. The first two planets announced are designated Kepler-47b, and Kepler-47c, and the third, later discovery is Kepler-47d. Kepler-47 is the first circumbinary multi-planet system discovered by the Kepler mission. The outermost of the planets is a gas giant orbiting within the habitable zone of the stars. Because most stars are binary, the discovery that multi-planet systems can form in such a system has impacted previous theories of planetary formation.

Kepler-62e is a super-Earth exoplanet discovered orbiting within the habitable zone of Kepler-62, the second outermost of five such planets discovered by NASA's Kepler spacecraft. Kepler-62e is located about 990 light-years from Earth in the constellation of Lyra. The exoplanet was found using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. Kepler-62e may be a terrestrial or ocean-covered planet; it lies in the inner part of its host star's habitable zone.

Kepler-432b (also known by its Kepler Object of Interest designation KOI-1299.01) is a hot super-Jupiter (or "warm" super-Jupiter) exoplanet orbiting the giant star Kepler-432 A, the innermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 2,830 light-years (870 parsecs, or nearly 2.684×10¹⁶ km) from Earth in the constellation Cygnus. The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured.

Kepler-419c is a super-Jupiter exoplanet orbiting within the habitable zone of the star Kepler-419, the outermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 3,400 light-years from Earth in the constellation Cygnus. The exoplanet was found by using the transit timing variation method, in which the variations of transit data from an exoplanet are studied to reveal a more distant companion.

<span class="mw-page-title-main">K2-33</span> Star in the constellation Scorpius

K2-33 is an extremely young pre-main-sequence star located about 453 light-years (139 pc) away from the Earth in the constellation of Scorpius. It is known to host one planet, a super-Neptune, named K2-33b. It is also notable for its young age.

HATS-36b is a gas giant exoplanet that orbits an F-type star. Its mass is 3.216 Jupiters, it takes 4.2 days to complete one orbit of its star, and is 0.05425 AU from it. It was discovered on June 12, 2017 and was announced in 2018. Its discoverers were 23, namely Daniel Bayliss, Joel Hartman, George Zhou, Gaspar Á. Bakos, Andrew Vanderburg, J. Bento, L. Mancini, S. Ciceri, Rafael Brahm, Andres Jordán, N. Espinoza, M. Rabus, T. G. Tan, K. Penev, W. Bhatti, M. de Val-Borro, V. Suc, Z. Csubry, Th. Henning, P. Sarkis, J. Lázár, I. Papp, P. Sári.

Kepler-93b (KOI-69b) is a hot, dense transiting Super-Earth exoplanet located approximately 313 light-years away in the constellation of Lyra, orbiting the G-type star Kepler-93. Its discovery was announced in February 2014 by American astronomer Geoffrey Marcy and his team. In July 2014, its radius was determined with a mere 1.3% margin of error, the most precise measurement ever made for an exoplanet's radius at the time.

This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.

[:0-1] 1 2 "NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 2024-03-19.

[2] NASA.gov

[scinews-3] 1 2 Astronomers Discover Circumbinary Planet 3,700 Light-Years Away

[sciencedaily-4] 1 2 New planet is largest discovered that orbits two suns

[1]

[2]

[3]

[4]

List of transiting exoplanets

See also

External links and references

Related Research Articles