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| Autors principals: | , |
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| Format: | Recurso digital |
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| Publicat: |
Zenodo
2025
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| Accés en línia: | https://doi.org/10.5281/zenodo.17755401 |
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- Orbital observatories have revolutionized our understanding of the universe across an immense range of phenomena and scales. Beginning with the pioneering X-ray missions of the early 1970s, these space-based telescopes unlocked a "hot and energetic universe" previously hidden by Earth's atmosphere, revealing the dynamics of black holes, neutron stars, and galaxy clusters. Concurrently, a new frontier emerged with the advent of dedicated exoplanet hunting missions, shifting the paradigm from speculation to statistical certainty regarding planets beyond our solar system. Missions like Kepler and TESS, utilizing transit photometry, have cataloged thousands of exoplanets, including Earth-sized worlds in habitable zones, while observatories such as Hubble and JWST have begun characterizing their atmospheres. This paper comprehensively reviews the multi-decade legacy of orbital observatories, tracing their evolution from the initial forays into X-ray astronomy to the current golden age of exoplanet discovery and characterization. It delves into the technological advancements, scientific breakthroughs, and synergistic approaches that have enabled these missions to fundamentally reshape our cosmic perspective, highlighting the profound impact on astrophysics and the search for life beyond Earth.