Giant Nemesis candidate HD 107914 / HIP 60503 for the perforation of Oort cloud
Igor Yu. Potemine

TL;DR
This paper identifies potential stellar candidates, especially HD 107914, that could pass close to the solar system, possibly influencing the Oort cloud or creating peculiar trans-Neptunian object trajectories.
Contribution
It reexamines stellar candidates for close solar system encounters using updated astrometric data, highlighting HD 107914 as a significant potential passerby.
Findings
HD 107914 could pass within 8380 AU of the Sun with certain radial velocities.
The star's trajectory could significantly influence the Oort cloud or TNO orbits.
Precise radial velocity and proper motion data are crucial for accurate encounter predictions.
Abstract
So far, GJ 710 is the only known star supposed to pass through outskirts of the solar system within 1 ly. We have reexamined the SIMBAD database for additional stellar candidates (from highest ratios of squared parallax to total proper motion) and compared them with new HIP2 parallaxes and known radial velocities. At the moment, the best nominee is double star HD 107914 in the constellation Centaurus at 78.3 pc from the Sun whose principal component is a white (A-type) giant. It does not seem to appear neither in general catalogues of radial velocities available at SIMBAD nor in authoritative Garcia-Sanchez et al. papers on stellar encounters with the solar system. Awaiting for the value of its radial velocity, uknown to the author, we have calculated limits of necessary to this star to pass within 1 ly and 1 pc from the Sun in linear approximation. A very…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
