HD 179949 is a 6th magnitude star in the constellation of Sagittarius. It is a yellow-white dwarf (spectral class F8 V), a type of star hotter and more luminous than the Sun. The star is located about 90 light years from Earth and might be visible under exceptionally good conditions to an experienced observer without technical aid; usually binoculars are needed. The star HD 179949 is named Gumala. The name was selected in the NameExoWorlds campaign by Brunei, during the 100th anniversary of the IAU. Gumala is a Malay word, which means a magic bezoar stone found in snakes, dragons, etc. Properties This is an F-type main-sequence star classified with a spectral type of F8V. It has an estimated mass of 1.23 times the solar mass and a radius of 1.20 times the solar radius. Its photosphere is shining with 1.95 times the solar luminosity at an effective temperature of 6,220 K. Its metallicity, the abundance of elements other than hydrogen and helium, is high, with 162% the solar iron abundance, following the trend that stars with giant planets are more metal-rich. With an estimated age of 1.2 billion years, HD 179949 is a chromospherically active star and has a complex magnetic field with a maximum strength of 10 G. Like the Sun, this star has differential rotation, with the equatorial region having a faster rotation period, of 7.62 ± 0.07 days, compared to a rotation period of 10.3 ± 0.8 days in the poles. The star's projected rotational velocity is 7.0 km/s, corresponding to an inclination angle of about 60°. HD 179949 has been classified as a BY Draconis variable, which varies in brightness due to rotational modulation of spots on the surface. Monitoring of the star's spectral lines suggested a possible correlation between the star's chromospheric activity and the orbital period of its planet HD 179949 b. Later observations showed that this correlation is not present, with the star's activity being in synchrony with the star's rotation, instead of the exoplanet's orbit. By 2022, stellar X-ray flares correlation with the planetary orbit was not detected too. Planetary system The discovery of an extrasolar planet orbiting HD 179949 with a period of only 3.1 days was published in 2001. It was detected with the radial velocity method from observations of the star with the UCLES spectrograph, in the Anglo-Australian Telescope, as part of the Anglo-Australian Planet Search. With a