Add to ORKGIn this paper we discuss an alternative track for migration that can explain the existence of Hot Jupiters observed in close orbits around their stars based on a novel interpretation of established work. We also discuss the population of sub-Earth rogue planets that would be created via this migration method, which would be on the order of 2 to 40 billion, many of which would still be present in the Galaxy and potentially detectable
The first planets discovered outside of our solar system were very different from the solar system p...
Planets are believed to form in primordial gas-dust discs surrounding newborn stars. An important br...
After centuries of wondering about the presence of other worlds outside our Solar System, the first ...
In this paper we discuss an alternative track for migration that can explain the existence of Hot Ju...
The discovery of "hot Jupiters" very close to their parent stars confirmed that Jovian planets migra...
In this dissertation, we present three complementary studies of the processes that drive planetary m...
The existence of hot Jupiters has challenged theories of planetary formation since the first extraso...
Gas giant planets orbiting within 0.1 AU of their host stars are unlikely to have formed in situ and...
Soon after the discovery of Jupiter-sized planets in extremely close orbits around Sun-like stars, i...
Hot Jupiters, giant extrasolar planets with orbital periods shorter than ~10 days, have long been th...
The migration history of Jupiter in the sun's natal disk remains poorly constrained. Here we conside...
The origin of warm Jupiters (gas giant planets with periods between 10 and 200 days) is an open ques...
The recent discovery of Jupiter-mass planets orbiting at a few AU from their stars compliments earli...
It is now accepted that the Solar system's youth was a dynamic and chaotic time. The giant planets m...
Despite decades of inquiry, the origin of giant planets residing within a few tenths of an astronomi...
The first planets discovered outside of our solar system were very different from the solar system p...
Planets are believed to form in primordial gas-dust discs surrounding newborn stars. An important br...
After centuries of wondering about the presence of other worlds outside our Solar System, the first ...
In this paper we discuss an alternative track for migration that can explain the existence of Hot Ju...
The discovery of "hot Jupiters" very close to their parent stars confirmed that Jovian planets migra...
In this dissertation, we present three complementary studies of the processes that drive planetary m...
The existence of hot Jupiters has challenged theories of planetary formation since the first extraso...
Gas giant planets orbiting within 0.1 AU of their host stars are unlikely to have formed in situ and...
Soon after the discovery of Jupiter-sized planets in extremely close orbits around Sun-like stars, i...
Hot Jupiters, giant extrasolar planets with orbital periods shorter than ~10 days, have long been th...
The migration history of Jupiter in the sun's natal disk remains poorly constrained. Here we conside...
The origin of warm Jupiters (gas giant planets with periods between 10 and 200 days) is an open ques...
The recent discovery of Jupiter-mass planets orbiting at a few AU from their stars compliments earli...
It is now accepted that the Solar system's youth was a dynamic and chaotic time. The giant planets m...
Despite decades of inquiry, the origin of giant planets residing within a few tenths of an astronomi...
The first planets discovered outside of our solar system were very different from the solar system p...
Planets are believed to form in primordial gas-dust discs surrounding newborn stars. An important br...
After centuries of wondering about the presence of other worlds outside our Solar System, the first ...