Direct Imaging
92 planets (1.5%)Photographing exoplanets directly by blocking the overwhelming light of their host star.
Direct imaging captures actual photographs of exoplanets by using coronagraphs or starshades to block the host star's light, which can be billions of times brighter than the planet. This technique works best for young, massive planets in wide orbits far from their star, where the contrast ratio is most favorable. Advanced adaptive optics and space-based telescopes are pushing this method's capabilities to detect smaller, cooler planets. Direct imaging is uniquely valuable because it allows astronomers to study a planet's atmosphere by analyzing the light it reflects or emits.
HIP 54515 b
HIP 54515 | 82.8 pc
KOINTREAU-1 b
XEST 17-036 | 158.6 pc
WISPIT 2 b
WISPIT 2 | 134.9 pc
WISPIT 1 c
WISPIT 1 | 230.0 pc
WISPIT 1 b
WISPIT 1 | 230.0 pc
HD 135344 A b
HD 135344 A | 141.6 pc
V2376 Ori b
V2376 Ori
HD 143811 AB b
HD 143811 A | 136.6 pc
2MASS J03590986+2009361 b
2MASS J03590986+2009361 | 117.4 pc
2MASS J21252752-8138278 b
2MASS J21252752-8138278 | 34.1 pc
HIP 39017 b
HIP 39017 | 66.3 pc
2MASS J11550485-7919108 b
2MASS J11550485-7919108 | 100.9 pc
GJ 900 b
GJ 900 A | 20.8 pc
UCAC4 328-061594 b
UCAC4 328-061594 | 39.9 pc
UCAC3 113-933 b
UCAC3 113-933 | 52.6 pc
HIP 77900 b
HIP 77900 | 150.9 pc
2MASS J11011926-7732383 b
2MASS J11011926-7732383
G 196-3 b
G 196-3 | 21.8 pc
ITG 15 b
ITG 15 A | 136.4 pc
HD 169142 b
HD 169142 | 113.6 pc
MWC 758 c
MWC 758 | 159.5 pc
HIP 81208 C b
HIP 81208 C | 147.5 pc
WISE J033605.05-014350.4 b
WISE J033605.05-014350.4
HIP 99770 b
HIP 99770 | 40.1 pc
PZ Tel b
PZ Tel | 47.1 pc
AF Lep b
AF Lep | 26.9 pc
HIP 21152 b
HIP 21152 | 43.4 pc
AB Aur b
AB Aur | 162.1 pc
HD 206893 c
HD 206893 | 40.8 pc
mu2 Sco b
mu2 Sco
COCONUTS-2 b
COCONUTS-2 A | 10.9 pc
HD 206893 b
HD 206893 | 40.8 pc
b Cen AB b
b Cen A | 98.1 pc
BD+60 1417 b
BD+60 1417 | 45.0 pc
2M0437 b
2MASS J04372171+2651014 | 128.5 pc
CFHTWIR-Oph 98 b
CFHTWIR-Oph 98 A
TYC 8998-760-1 c
TYC 8998-760-1 | 94.6 pc
TYC 8998-760-1 b
TYC 8998-760-1 | 94.6 pc
USco1556 b
USco1556 A | 140.6 pc
PDS 70 c
PDS 70 | 113.1 pc
HIP 79098 AB b
HIP 79098 AB | 145.8 pc
USco1621 b
USco1621 A | 137.9 pc
PDS 70 b
PDS 70 | 113.1 pc
2MASS J22501512+2325342 b
2MASS J22501512+2325342 | 57.2 pc
2MASS J0249-0557 c
2MASS J0249-0557 A | 66.1 pc
HD 284149 AB b
HD 284149 A | 117.8 pc
HIP 65426 b
HIP 65426 | 108.9 pc
Luhman 16 b
Luhman 16 A
HR 2562 b
HR 2562 | 34.0 pc
2MASS J22362452+4751425 b
2MASS J22362452+4751425 | 69.6 pc
2MASS J02192210-3925225 b
2MASS J02192210-3925225
51 Eri b
51 Eri | 29.8 pc
LkCa 15 c
LkCa 15 | 158.2 pc
VHS J125601.92-125723.9 b
VHS J125601.92-125723.9
LkCa 15 b
LkCa 15 | 158.2 pc
GU Psc b
GU Psc | 47.6 pc
HD 100546 b
HD 100546 | 109.7 pc
ROXs 42 B b
ROXs 42 B | 143.6 pc
ROXs 12 b
ROXs 12 | 136.7 pc
2MASS J01225093-2439505 b
2MASS J01225093-2439505 | 33.8 pc
HD 106906 b
HD 106906 | 103.0 pc
GJ 504 b
GJ 504 | 17.5 pc
2MASS J01033563-5515561 AB b
2MASS J01033563-5515561 A
HD 95086 b
HD 95086 | 86.2 pc
kap And b
kap And | 50.0 pc
WISEP J121756.91+162640.2 A b
WISEP J121756.91+162640.2 A
CD-35 2722 b
CD-35 2722 | 22.4 pc
WD 0806-661 b
WD 0806-661 | 19.2 pc
CFBDSIR J145829+101343 b
CFBDSIR J145829+101343
HIP 78530 b
HIP 78530 | 136.8 pc
2MASS J04414489+2301513 b
2MASS J04414489+2301513
HR 8799 e
HR 8799 | 41.2 pc
Ross 458 c
Ross 458 | 11.5 pc
GSC 06214-00210 b
GSC 06214-00210 | 108.5 pc
SR 12 AB c
SR 12 AB
HR 8799 b
HR 8799 | 41.2 pc
FU Tau b
FU Tau
USco CTIO 108 b
USco CTIO 108 | 144.0 pc
HR 8799 d
HR 8799 | 41.2 pc
HR 8799 c
HR 8799 | 41.2 pc
bet Pic b
bet Pic | 19.7 pc
1RXS J160929.1-210524 b
1RXS J160929.1-210524 | 139.1 pc
CT Cha b
CT Cha | 190.7 pc
CHXR 73 b
CHXR 73 | 190.4 pc
HN Peg b
HN Peg | 18.1 pc
HD 203030 b
HD 203030 | 39.3 pc
Oph 11 b
Oph 11
LP 261-75 b
LP 261-75 A | 33.9 pc
AB Pic b
AB Pic | 50.0 pc
DH Tau b
DH Tau | 134.8 pc
GQ Lup b
GQ Lup | 151.2 pc
2MASS J12073346-3932539 b
2MASS J12073346-3932539 | 64.3 pc