Results 31 to 40 of about 47,304 (316)

On the origin of planets at very wide orbits from the re-capture of free floating planets [PDF]

open access: bronze, 2012
In recent years several planets have been discovered at wide orbits (>100 AU) around their host stars. Theoretical studies encounter difficulties in explaining their formation and origin.
Adams   +24 more
core   +2 more sources

On the properties of free-floating planets originating in circumbinary planetary systems [PDF]

open access: goldMonthly notices of the Royal Astronomical Society
Free-floating planets are a new class of planets recently discovered. These planets don’t orbit within stellar systems, instead living a nomadic life within the galaxy. How such objects formed remains elusive. Numerous works have explored mechanisms to
Gavin A. L. Coleman
openalex   +3 more sources

Detectability of Free Floating Planets in Open Clusters with JWST [PDF]

open access: bronze, 2013
Recent observations have shown the presence of extra-solar planets in Galactic open stellar clusters, as in the Praesepe (M44). These systems provide a favorable environment for planetary formation due to the high heavy-element content exhibited by the ...
D'Onghia, Elena   +2 more
core   +2 more sources

The microlensing rate and distribution of free-floating planets towards the Galactic bulge [PDF]

open access: yes, 2016
Ground-based optical microlensing surveys have provided tantalising, if inconclusive, evidence for a significant population of free-floating planets (FFPs).
Ban, M., Kerins, E., Robin, A. C.
core   +6 more sources

Disc fragmentation. II. Ejection of low mass Free Floating Planets from growing binary systems

open access: greenMonthly notices of the Royal Astronomical Society
Observations indicate that disc fragmentation due to Gravitational Instability (GI) is the likely origin of massive companions to stars, such as giant planets orbiting M-dwarf stars, Brown Dwarf (BD) companions to FGK stars, and binary stars with ...
Sergei Nayakshin   +6 more
openalex   +2 more sources

ON THE FEASIBILITY OF CHARACTERIZING FREE-FLOATING PLANETS WITH CURRENT AND FUTURE SPACE-BASED MICROLENSING SURVEYS [PDF]

open access: bronze, 2016
Simultaneous space- and ground-based microlensing surveys, such as K2's Campaign 9 (K2C9) and WFIRST, facilitate measuring the masses and distances of free-floating planet (FFP) candidates, which are identified as single-lens events with timescales that ...
Calen B. Henderson, Yossi Shvartzvald
openalex   +3 more sources

The Demographics of Rocky Free-floating Planets and their Detectability by WFIRST [PDF]

open access: yesThe Astrophysical Journal, 2017
Planets are thought to form via accretion from a remnant disk of gas and solids around a newly formed star. During this process, material in the disk either remains bound to the star as part of either a planet, a smaller celestial body, or makes up part ...
T. Barclay   +3 more
semanticscholar   +4 more sources

The coolest 'stars' are free-floating planets [PDF]

open access: green, 2014
We show that the coolest known object that is probably formed in a star-like mode is a free-floating planet. We discovered recently that the free-floating planetary mass object OTS,44 (M9.5, ~12 Jupiter masses, age ~2 Myr) has significant accretion and a substantial disk.
V. Joergens   +4 more
openalex   +3 more sources

A rich population of free-floating planets in the Upper Scorpius young stellar association [PDF]

open access: yesNature Astronomy, 2021
The nature and origin of free-floating planets (FFPs) are still largely unconstrained because of a lack of large homogeneous samples to enable a statistical analysis of their properties.
N. Miret-Roig   +11 more
semanticscholar   +2 more sources

Free-floating planets in stellar clusters? [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2001
We have simulated encounters between planetary systems and single stars in various clustered environments. This allows us to estimate the fraction of systems liberated, the velocity distribution of the liberated planets, and the separation and eccentricity distributions of the surviving bound systems.
K. W. Smith, I. A. Bonnell
openalex   +5 more sources

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