Analysis of information sources in references of the Wikipedia article "Júpiter quente" in Portuguese language version.
The mass of WASP-47d is 15.2±7 M⊕. Only an upper limit can be placed on WASP-47e of < 22 M⊕.
The mass of WASP-47d is 15.2±7 M⊕. Only an upper limit can be placed on WASP-47e of < 22 M⊕.
The mass of WASP-47d is 15.2±7 M⊕. Only an upper limit can be placed on WASP-47e of < 22 M⊕.
Studying of a curve of change of shine of WASP-12b has brought to the Russian astronomers unusual result: regular splashes were found out. ... Though stains on a star surface also can cause similar changes of shine, observable splashes are very similar on duration, a profile and amplitude that testifies for benefit of exomoon existence.