Centaurus
Constellation in the southern celestial hemisphere
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We include updates on Alpha Centauri, Proxima Centauri, Proxima Centauri b, J1407b, Shapley Supercluster, Omega Centauri, V1400 Centauri, ESO 383-76, Boomerang Nebula, Beta Centauri, 2M1207b, Przybylski's Star, BPM 37093, Southern Crab Nebula, 2M1207, HD 117618 ... and more.
| March 2024 | Follow-up observations of Alpha Centauri A are planned for March 2024 using the James Webb Space Telescope. |
| July 27 2023 | James Webb Space Telescope (JWST) continued coronographic observations of Alpha Centauri A, completing a two-day observation period that resulted in failure. |
| July 26 2023 | James Webb Space Telescope (JWST) conducted coronographic observations of Alpha Centauri A on July 26 and 27, which were ultimately unsuccessful. |
| June 2023 |
HIP 65426 b
The planet was officially named Najsakopajk, with its host star named Matza, based on Zoque words proposed by a Mexican team, meaning 'Mother Earth' and 'star' respectively.
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| 2022 | A study disputed the existence of Proxima Centauri c. |
| 2022 | Proxima Centauri d was detected, with a mass of about 0.26 Earth masses and a periodicity of 5.15 days. |
| September 2022 |
HIP 65426 b
HIP 65426 b became the first exoplanet directly observed by the James Webb Space Telescope, marking a significant milestone in astronomical imaging and exoplanet research.
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| August 2022 |
HIP 65426 b
The first exoplanet observation by the James Webb Space Telescope (JWST) of HIP 65426 b was published as a pre-print, marking the first exoplanet imaged by JWST and the first detected in wavelengths beyond 5 μm.
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| August 2022 |
HIP 65426 b
HIP 65426 b was included among 20 exoplanetary systems selected for naming in the third NameExoWorlds project.
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| 2021 |
Przybylski's Star
Comprehensive experimental analysis of einsteinium isotope signature spectra was conducted, though no confirmation of presence in the star was published.
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| December 2021 | Approximately 70 new rogue planets were discovered in the Upper Scorpius association, a subgroup of the Scorpius-Centaurus association. |
| 2020 |
HIP 65426 b
Spectral analysis of HIP 65426 b was conducted, revealing the planet is carbon-poor and oxygen-rich compared to Solar System gas giants.
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| 2020 | Alpha Centauri A and B components observed with a separation of 5.49 arcseconds through position angle of 345.3°. |
| June 2020 | A possible direct imaging detection suggested the presence of a large ring system around Proxima Centauri c. |
| 2019 | Researchers discovered interstellar iron in Antarctica, potentially related to the Local Interstellar Cloud formed near the Sco-Cen association. |
| August 10 2018 | The International Astronomical Union (IAU) officially approves the name Toliman for α Centauri B and Rigil Kentaurus for α Centauri A. |
| 2017 | Precise radial velocity measurements confirmed that Proxima Centauri is gravitationally bound to Alpha Centauri AB system. |
| 2016 | European Southern Observatory (ESO) astronomers discovered Proxima Centauri b, a terrestrial planet with an estimated minimum mass of 1.17 Earth masses, located in the star's habitable zone. |
| 2016 | The IAU Working Group on Star Names decides to attribute proper names to individual component stars of the Alpha Centauri system. |
| February 2016 | Closest recent approach of Alpha Centauri A and B stars, observed at 4.0 arcseconds through position angle of 300°. |
This contents of the box above is based on material from the Wikipedia articles Alpha Centauri, Scorpius–Centaurus association, Przybylski's Star & HIP 65426 b, which are released under the Creative Commons Attribution-ShareAlike 4.0 International License.