Skip to content
DraconiticResearch
Search Sources API
197,761 studies31 sourcesUpdated 4 min ago
PreprintarXiv licencearXiv

Triggering star formation by free-floating planets

Abstract

Recently, a population of free-floating planets has been discovered in the Galaxy. This paper examines the influence of the planets trapped within a protostellar hydrogen clouds on the processes of gravitational instability in the gas. A sufficiently massive planet can become an alternative dynamic center for the contracting cloud. This occurs due to rapid mass growth from accretion onto the planet within the cloud. Owing to residual velocity and density gradients in the cloud, the planet that triggers star formation is likely to end up in a distant orbit around the newborn star. Some second- and subsequent-generation stars in the Galaxy may have formed via this mechanism.

Related

  1. The Galactic Dynamics of Free-Floating Planets: From Ejection Kicks to Microlensing
    Zara Sayed, Stefano Profumo, Nolan Smyth
    arXivPreprintCC BY 4.0Full textGalaxiesPlanetary science & exoplanetsarXiv
  2. Limits on a Host Star around a Saturn-mass Free-floating Planet Candidate KMT-2024-BLG-0792/OGLE-2024-BLG-0516
    Przemek Mróz, Klara Piotrowska, Antoine Mérand +2
    arXivPreprintCC BY 4.0Full textGalaxiesInstrumentation & methodsarXiv
  3. J-PAS: Exploring the connection between local environment and the triggering of bursty star formation in Extreme Emission Line Galaxies
    Mauro González-Otero, Jose M. Vílchez, Antonio Giménez-Alcázar +45
    arXivPreprintCC BY 4.0Full textGalaxiesarXiv
  4. Contribution of White Dwarf Formation Kicks to the Free-floating Planet Population
    Alexander P. Stephan, Keivan G. Stassun
    The Astrophysical Journal LettersPeer-reviewedCC BY 4.0Full textSolar & stellar physicsCrossref
  5. Contribution of White Dwarf Formation Kicks to the Free-Floating Planet Population
    Alexander P. Stephan, Keivan G. Stassun
    arXivPreprintCC BY 4.0Full textGalaxiesPlanetary science & exoplanetsarXiv
BibTeX
@misc{eroshenko2026triggering,
  title = {{Triggering star formation by free-floating planets}},
  author = {Yu. N. Eroshenko},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.28744},
  eprint = {2609.28744},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.28744},
}
RIS
TY  - UNPB
TI  - Triggering star formation by free-floating planets
AU  - Yu. N. Eroshenko
PY  - 2026
DA  - 2026/09/23
PB  - arXiv
DO  - 10.48550/arxiv.2609.28744
UR  - https://arxiv.org/abs/2609.28744
AB  - Recently, a population of free-floating planets has been discovered in the Galaxy. This paper examines the influence of the planets trapped within a protostellar hydrogen clouds on the processes of gravitational instability in the gas. A sufficiently massive planet can become an alternative dynamic center for the contracting cloud. This occurs due to rapid mass growth from accretion onto the planet within the cloud. Owing to residual velocity and density gradients in the cloud, the planet that triggers star formation is likely to end up in a distant orbit around the newborn star. Some second- and subsequent-generation stars in the Galaxy may have formed via this mechanism.
ER  -