HD 23079 is a star in the southern constellation of Reticulum. Since the star has an apparent visual magnitude of 7.12, [2] it is not visible to the naked eye, but at least in binoculars it should be easily visible.

Oct 24, 2024 · HD 23079 b is a gas giant exoplanet that orbits a F-type star. Its mass is 2.61 Jupiters, it takes 2 years to complete one orbit of its star, and is 1.6 AU from its star. Its discovery was announced in 2001.

HD 23079 b, formally named Guarani, is an exoplanet approximately 109 light years away in the constellation Reticulum. The planet has mass of at least 2.45 Jupiters, although only the minimum mass is known since inclination is unknown.

Star HD 23079 is a main sequence star that fuses hydrogen atoms into helium. It is is approximately 13 % bigger than the Sun and temperature on its surface is around 5848 K (5575 °C), which is about 101 % of Sun's temperature.

HD 23079 is a yellowish dwarf star of spectral and luminosity type F8-G0 V. It has about 1.10 times Sol's mass (exoplanets.org), probably a larger diameter, and over 1.4 times its luminosity.

Exoplanet HD 23079 b orbits star HD 23079 that lies 109 light years away from the Sun. It weighs about 778.9 Earth masses and orbits its star further than Earth orbits Sun.

Three exoplanet systems (GJ 86, HD 41004, andγ Cep) have potentially close-in stellar companions, with planetsat roughly Mercury-Mars distances from the host star and stellarcompanions at projected separations of ~20 AU, similar to the Sun-Uranusdistance.

Spectroscopic [Fe/H] for 98 extra-solar planet-host stars. Exploring the probability of planet formation. Statistical properties of exoplanets. II. Metallicity, orbital parameters, and space velocities.

The star HD 23079 has apparent magnitude of 7.1, with absolute magnitude of 4.5. It is 1.1 times more massive and 1.1 times bigger compared with our Sun. The surface temperature is 5848 with its spectral types of F8/G0 V.

We re-evaluate the outer edge of orbital stability for possible exomoons orbiting the radial velocity planet discovered in the HD 23079 system. In this system, a solar-type star hosts a Jupiter-mass planet in a nearly circular orbit in the outer stellar habitable zone.