1 00:00:00,567 --> 00:00:04,170 A, B, C, M, X – oops! 2 00:00:04,170 --> 00:00:05,605 Those aren't the ABCs, 3 00:00:05,605 --> 00:00:08,875 they're the categories used to measure the intensity of solar flares. 4 00:00:09,376 --> 00:00:11,311 On October 3, 2024, 5 00:00:11,311 --> 00:00:15,749 NASA's Solar Dynamics Observatory captured this X9.0 flare. 6 00:00:16,516 --> 00:00:19,519 Solar flares are powerful bursts of light from the Sun. 7 00:00:19,753 --> 00:00:23,223 X-class is a classification saved for the most intense flares, 8 00:00:23,556 --> 00:00:27,193 with less intense flares classified as A, B, C, or M. 9 00:00:27,494 --> 00:00:31,297 Scientists observe these flares in various wavelengths to better understand how 10 00:00:31,297 --> 00:00:35,068 the Sun releases material that can affect Earth and technology in space. 11 00:00:35,402 --> 00:00:39,039 The wavelength seen here shows the hottest material in a solar flare. 12 00:00:39,172 --> 00:00:41,074 When this Earth-directed flare occurred, 13 00:00:41,074 --> 00:00:43,443 an eruption of electromagnetic radiation 14 00:00:43,443 --> 00:00:47,680 blasted toward our planet resulting in radio blackouts over the Atlantic Ocean. 15 00:00:47,680 --> 00:00:51,151 These blackouts affect high-frequency radio signals – aka 16 00:00:51,151 --> 00:00:53,053 the ones often used by commercial airlines 17 00:00:53,053 --> 00:00:54,754 and first responders, like FEMA.