Happy birthday!! 🥳 🎉

After the well-deserved afternoon break, get back at 18:00 IST (12:30 UTC) to Anamudi where Enrico Zini, in his talk "Adulting", want to start figuring out how to address practical issues around the sustainability of the Debian community, in a way that fits the needs and peculiarities of the community. Watch the talk online at: https://debconf23.debconf.org/schedule/venue/1/ and the crowd at DebConf23 will move towards the traditional "Cheese and Wine party" after that. #debian #debconf #debconf23 #freesoftware #dc23 #kochi #debconfkochi #debianindia

The second day of DebConf23 has ended, we start again tomorrow, Tuesday 12, September at 10:30 IST (05:00 UTC). The schedule for the day will be https://debconf23.debconf.org/schedule/?block=3 Thank you to all our contributors, viewers, and to our Debconf Video team! See you tomorrow! #debian #debconf #freesoftware #dc23 #debconf23 #kochi #debconfkochi #debianindia

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2023 June 1

Explanation: Massive stars in our Milky Way Galaxy live spectacular lives. Collapsing from vast cosmic clouds, their nuclear furnaces ignite and create heavy elements in their cores. After a few million years, the enriched material is blasted back into interstellar space where star formation can begin anew. The expanding debris cloud known as Cassiopeia A is an example of this final phase of the stellar life cycle. Light from the explosion which created this supernova remnant would have been first seen in planet Earth's sky about 350 years ago, although it took that light about 11,000 years to reach us. This false-color image, composed of X-ray and optical image data from the Chandra X-ray Observatory and Hubble Space Telescope, shows the still hot filaments and knots in the remnant. It spans about 30 light-years at the estimated distance of Cassiopeia A. High-energy X-ray emission from specific elements has been color coded, silicon in red, sulfur in yellow, calcium in green and iron in purple, to help astronomers explore the recycling of our galaxy's star stuff. Still expanding, the outer blast wave is seen in blue hues. The bright speck near the center is a neutron star, the incredibly dense, collapsed remains of the massive stellar core.

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2023 April 19

Explanation: On some nights the sky is the best show in town. On this night, auroras ruled the sky, and the geomagnetic storm that created this colorful sky show originated from an increasingly active Sun. Surprisingly, since the approaching solar CME the day before had missed the Earth, it was not expected that this storm would create auroras. In the foreground, two happily surprised aurora hunters contemplate the amazing and rapidly changing sky. Regardless of forecasts, though, auroras were reported in the night skies of Earth not only in the far north, but as far south as New Mexico, USA. As captured in a wide-angle image above Saariselkä in northern Finnish Lapland, a bright aurora was visible with an unusually high degree of detail, range of colors, and breadth across the sky. The vivid yellow, green, red and purple auroral colors are caused by oxygen and nitrogen atoms high in Earth's atmosphere reacting to incoming electrons.

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