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Europe’s Vega-C rocket has resumed operations, achieving a successful launch on December 5, 2024, after a two-year suspension due to a failure during its previous mission. The rocket, operated by French aerospace company Arianespace, carried the Copernicus Sentinel-1C Earth-observation satellite into orbit. The launch took place at 4:20 p.m. EST from the Guiana Space Centre in Kourou, French Guiana, following a postponed attempt caused by a mechanical issue on December 4.

Launch Details and Mission Objectives

As per sources, the Vega-C rocket deployed Sentinel-1C into a sun-synchronous orbit approximately 435 miles (700 km) above Earth. The satellite, part of the European Union’s Copernicus Earth-observation programme, serves as a replacement for Sentinel-1B, which became non-operational due to a technical fault in 2022. Sentinel-1C will work alongside Sentinel-1A to capture high-resolution imagery of Earth’s surface, providing critical data for environmental monitoring and disaster management.

Christoph Kautz, Director of Satellite Navigation and Earth Observation at the Directorate-General for Defence Industry and Space (DG DEFIS), stated during a prelaunch briefing that over 30 petabytes of data have been generated since the Sentinel-1 programme began. He also noted the programme’s significant role in supplying users with over 150,000 products derived from this data.

Technological Updates to Vega-C and Future Plans

Reportedly, the two-year hiatus of Vega-C was attributed to a redesign of its second-stage rocket engine nozzle, following the failure of its second mission in December 2022. Giulio Ranzo, CEO of Avio, which designs the rocket under a European Space Agency (ESA) contract, described the relaunch as a critical step in fulfilling 15 upcoming missions in Vega-C’s backlog, in a statment.

The ESA has also announced plans to replace Vega-C with Vega-E, a next-generation rocket featuring an upgraded liquid oxygen-methane engine, known as the M-10. According to ESA Director of Space Transportation Toni Tolker-Nielsen, in a statement, contracts for its implementation are expected to be signed by year-end.

Sentinel-1A, operational since 2014, is slated for replacement by Sentinel-1D in September 2025, further enhancing the constellation’s observational capabilities.

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New Analysis of 1977 Wow! Signal Reveals Stronger Cosmic Mystery

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The famous 1977 “Wow!” signal — a mysterious radio burst detected by Ohio’s Big Ear telescope — has been reanalyzed using modern computing techniques. Researchers digitized old telescope records, finding the signal was about four times stronger than first thought, peaking at 250 Janskys. The recalculations also refined its frequency and sky location, ruling …

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Astronomers Capture Sharpest-Ever Solar Flare Images with NSF’s DKIST Telescope

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Astronomers have achieved a major breakthrough by capturing the sharpest images of a solar flare ever recorded, using the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST). Observed at the hydrogen-alpha wavelength during the decay of an X1.3-class solar flare, the images unveiled hundreds of ultra-fine coronal loops averaging just 48 kilometers…

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James Webb Detects Carbon Dioxide–Dominated Coma in Interstellar Object 3I/ATLAS

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The James Webb Space Telescope observed 3I/ATLAS, the third interstellar object detected in our solar system. Its coma is unusually rich in carbon dioxide with little water or carbon monoxide, suggesting a CO₂-rich core or an insulating crust. Findings raise new questions about its cosmic origin.

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