Personal tools
Log in

Skip to content. | Skip to navigation

INAF

Istituto italiano di astrofisica - national institute for astrophisics

Sections
Ciao
You are here: Home › Surprises from Kepler's supernova

Surprises from Kepler's supernova

The supernova observed for the first time in 1604 by Kepler was not only more powerful, but might have also occurred at a greater distance, than previously thought.
Surprises from Kepler's supernova

According to the latest observations of NASA's Chandra telescope, the supernova observed for the first time in 1604 by Kepler was not only more powerful, but might have also occurred at a greater distance, than previously thought. Astronomers have long studied the Kepler supernova remnant and tried to determine exactly what happened when the star exploded to create it. New analysis of a long observation from NASA's Chandra X-ray Observatory is providing more clues.

Read the full story here: http://www.media.inaf.it/2012/09/13/la-supernova-di-keplero-sorprende-ancora/

Lake Como Schools on Astrophysics, Cosmology and Gravitation

Jul 08, 2025

Lake Como Schools on Astrophysics, Cosmology and Gravitation It has been held at Como – Villa del Grumello, 23-27 June, the 2025 edition of the “Lake Como Schools on Astrophysics, Cosmology and Gravitation” on the theme “Dark Matter, Dark Energy and the Cosmological Tensions”

The Lucchin Schools Return

Jun 01, 2025

The Lucchin Schools Return First Edition of the New INAF PhD School Series Concludes in Asiago

MISTRAL, a wind of change in the SRT observations

May 29, 2025

MISTRAL, a wind of change in the SRT observations MISTRAL is a new-generation receiver for observations at millimeter wavelengths, built as part of the recent project to upgrade the Sardinia Radio Telescope for the study of the high-frequency radio universe. The main features of this instrument are the very high number of detectors cooled to temperatures close to absolute zero and a dedicated cold optical system, which allow for extremely sharp images. MISTRAL made its “first light” by observing three different celestial objects: the Orion Nebula, the radio lobes of the supermassive black hole in the galaxy M87, and the supernova remnant Cassiopeia A. These images represent the first scientific observations at 90 GHz ever obtained using the SRT