Astrophysics, abstract
astro-ph/0603219
From: Jorge Melendez [view email]
Date: Thu, 9 Mar 2006 03:05:17 GMT (24kb)
HD 98618: A Star Closely Resembling our Sun
Authors: Jorge Melendez (1,2), Katie Dodds-Eden (1), Jose A. Robles (1) (1) RSAA/Mt Stromlo Observatory (Australia), (2) Caltech (USA), UNMSM (Peru)
Comments: ApJ letters, in press
Despite the observational effort carried out in the last few decades, no perfect solar twin has been found to date. An important milestone was achieved a decade ago by Porto de Mello & da Silva, who showed that 18 Sco is almost a solar twin. In the present work, we use extremely high resolution (R = 10^5) high S/N Keck HIRES spectra to carry out a differential analysis of sixteen solar twin candidates. We show that HD 98618 is the second closest solar twin, and that the fundamental parameters of both HD 98618 and 18 Sco are very similar (within a few percent) to the host star of our solar system, including the likelihood of hosting a terrestrial planet within their habitable zone. We suggest that these stars should be given top priority in exoplanet and SETI surveys.
http://arxiv.org/abs/astro-ph/0603219
Space/Science » in reply to Spectroscopic rotational velocities of brown dwarfs
HD 98618: A Star Closely Resembling our Sun
The whole thread (12 posts)
- Giant Planet Accretion and Migration: Surviving the Type I Regime
- Dust flow in gas disks in the presence of embedded planets
- Turbulence driven diffusion in protoplanetary disks - chemical effects in the outer disk
- 24-micron Detections of Disks around Very Low-mass Stars and Brown Dwarfs in IC 348: Grain Growth/Settling and Inner Holes?
- Turbulence driven diffusion in protoplanetary disks - chemical effects in the outer disk
- Dust flow in gas disks in the presence of embedded planets
