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In the future, in addition to the continuing spectroscopic observations with Subaru Telescope, the team will conduct observations with the Kyoto University's Okayama 3.8m telescope, which is now under construction. The results of these observations and analysis confirm that stars similar to the Sun can have superflares if they have large starspots. Using this, they investigated the core depth of Ca II 854.2 line, and found that superflare stars have large starspots compared to sunspots (Figure 3). In addition, the measured rotation velocity of some target superflare stars is as slow as that of the Sun.ģ.Based on solar observations, astronomers know that if there are large dark star spots on a stellar surface, the "core depth" (the depth and width of a spectral line) of the Ca II 854.2 (ionized Calcium) absorption line becomes shallow. Spectroscopic observations allow observers to estimate the rotation velocity from the broadening of absorption lines (Figure 2), and confirm that a velocity derived from spectroscopic data matches the brightness variation timescale as the star rotates. Moreover, the timescales of the brightness variations should correspond to the stars' rotation speeds. As shown in Figure 1, the stars seem to become dimmer when their starspots are on their visible sides. Such variations are explained by the rotation of the star and its starspots. The typical periods range from one day to a few tens of days. The team confirmed the characteristics of the target stars as similar to those of the Sun.Ģ.On the basis of the Kepler data, superflare stars show somewhat regular, periodic changes in their brightnesses. From the investigation of the detailed properties of spectral lines, the team obtained the following results:ġ.More than half the observed 50 stars show no evidence of binarity (that is, they are not binary stars).

(Credit: Kyoto University)īased on the initial discovery, the team carried out spectroscopic observations on 50 solar-type superflare stars selected from the Kepler Space Telescope's data.

This figure shows a large superflare (shown in white) occurring in the large starspot area. Right: An artificial image of a superflare star seen with visible light. In addition to the sudden brightenings caused by flares, quasi-periodic brightness variations with periods of about 15 days are seen. However, more detailed observations were needed to investigate detailed properties of superflare stars and whether such massive flares can occur on ordinary single stars similar to our Sun.įigure 1: Left: The brightness variation of solar-type superflare stars (from Kepler data). This discovery was very important since it enabled the astronomers to conduct statistical analysis of superflares for the first time. Nature on 2012 May 24), where the team reported finding several hundred superflares on solar-type stars by analyzing stellar observation data from Kepler Space Telescope. This work follows up on observations made in 2012 (Maehara et al.

Such storms can have severe impacts on our daily life by affecting such systems as communications and power grids.

Large flares often cause massive bursts of high-speed plasma called coronal mass ejections (CMEs), can lead to geomagnetic storms on Earth. Solar flares are energetic explosions in the solar atmosphere and are thought to occur by intense releases of magnetic energy around the sunspots. The team, made up of astronomers from Kyoto University, University of Hyogo, the National Astronomical Observatory of Japan (NAOJ), and Nagoya University, targeted a set of solar-type stars emitting very large flares that release total energies 10-10000 times greater than the biggest solar flares. The investigations focused on the detailed properties of these stars and confirmed that Sun-like stars with large starspots can experience superflares. A team of astronomers has used the High Dispersion Spectrograph on the Subaru Telescope to conduct spectroscopic observations of Sun-like "superflare" stars first observed and cataloged by the Kepler Space Telescope.