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NASA’s Roman and ESA’s Euclid Will Team Up To Investigate Dark Energy

NASA Looks Back at 50 Years of Gamma-Ray Burst Science

Goddard Team Builds, Tests Calibrator for NASA’s Roman in Record Time

Historic Nebula Seen Like Never Before With NASA’s IXPE

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This image represents a view of NASA Kepler supernova remnant taken in X-rays, visible light, and infrared radiation, indicating that the bubble of gas that makes up the supernova remnant appears different in various types of light.

The images indicate that the bubble of gas that makes up the supernova remnant appears different in various types of light. Chandra reveals the hottest gas [colored blue and colored green], which radiates in X-rays.

Seen as a red dusty cloud in this image from NASA Wide-field Infrared Survey Explorer, Puppis A is the remnant of a supernova explosion.

A massive star left, which has created elements as heavy as iron in its interior, blows up in a tremendous explosion middle, scattering its outer layers in a structure called a supernova remnant right.

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BalNeO

Figure 2. (left) aerosol concentration and temperature profiles obtained during the first BalNeO flight from Bauru/Brazil on 1 June 2024. (right) Another flight took place 3 days after from Reims/France.

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