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#astrochemistry — Public Fediverse posts

Live and recent posts from across the Fediverse tagged #astrochemistry, aggregated by home.social.

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  1. The detailed mapping of the spatial distribution and chemical composition of interstellar ices within the dense gas and dust shells of early-stage forming stars (Class 0 protostars) in the Orion A molecular cloud.
    #Astrochemistry #Astrophysics #Astronomy #sflorg
    sflorg.com/2026/09/asph0910260

  2. The detailed mapping of the spatial distribution and chemical composition of interstellar ices within the dense gas and dust shells of early-stage forming stars (Class 0 protostars) in the Orion A molecular cloud.
    #Astrochemistry #Astrophysics #Astronomy #sflorg
    sflorg.com/2026/09/asph0910260

  3. The detailed mapping of the spatial distribution and chemical composition of interstellar ices within the dense gas and dust shells of early-stage forming stars (Class 0 protostars) in the Orion A molecular cloud.
    #Astrochemistry #Astrophysics #Astronomy #sflorg
    sflorg.com/2026/09/asph0910260

  4. The detailed mapping of the spatial distribution and chemical composition of interstellar ices within the dense gas and dust shells of early-stage forming stars (Class 0 protostars) in the Orion A molecular cloud.
    #Astrochemistry #Astrophysics #Astronomy #sflorg
    sflorg.com/2026/09/asph0910260

  5. The detailed mapping of the spatial distribution and chemical composition of interstellar ices within the dense gas and dust shells of early-stage forming stars (Class 0 protostars) in the Orion A molecular cloud.
    #Astrochemistry #Astrophysics #Astronomy #sflorg
    sflorg.com/2026/09/asph0910260

  6. Reply to: Evidence for phenylium reactivity under interstellar-relevant conditions

    Loison, J.-C. et al. Evidence of phenylium reactivity under interstellar relevant conditions. Nat. Astron. doi.org/10.1038/s41550-026-029 (2026). Kocheril, G.…
    #NewsBeep #News #Space #Astrochemistry #Astronomy #AstrophysicsandCosmology #AU #Australia #general #Laboratoryastrophysics #Physics #Science
    newsbeep.com/au/883706/

  7. Reply to: Evidence for phenylium reactivity under interstellar-relevant conditions

    Loison, J.-C. et al. Evidence of phenylium reactivity under interstellar relevant conditions. Nat. Astron. doi.org/10.1038/s41550-026-029 (2026). Kocheril, G.…
    #NewsBeep #News #Space #Astrochemistry #Astronomy #AstrophysicsandCosmology #AU #Australia #general #Laboratoryastrophysics #Physics #Science
    newsbeep.com/au/883706/

  8. Reply to: Evidence for phenylium reactivity under interstellar-relevant conditions

    Loison, J.-C. et al. Evidence of phenylium reactivity under interstellar relevant conditions. Nat. Astron. doi.org/10.1038/s41550-026-029 (2026). Kocheril, G.…
    #NewsBeep #News #Space #Astrochemistry #astronomy #AstrophysicsandCosmology #general #Laboratoryastrophysics #Physics #Science #UK #UnitedKingdom
    newsbeep.com/uk/763278/

  9. Reply to: Evidence for phenylium reactivity under interstellar-relevant conditions

    Loison, J.-C. et al. Evidence of phenylium reactivity under interstellar relevant conditions. Nat. Astron. doi.org/10.1038/s41550-026-029 (2026). Kocheril, G.…
    #NewsBeep #News #US #USA #UnitedStates #UnitedStatesOfAmerica #Space #Astrochemistry #Astronomy #AstrophysicsandCosmology #general #Laboratoryastrophysics #Physics #Science
    newsbeep.com/us/839843/

  10. The most common type of planet in the galaxy, known as mini- or sub-Neptunes, may harbor significantly more water than previously estimated by concealing it deep beneath thick, hydrogen-rich atmospheres.
    #Astronomy #Astrophysics #PlanetaryScience #Astrochemistry #sflorg
    sflorg.com/2026/07/astr0713260

  11. The most common type of planet in the galaxy, known as mini- or sub-Neptunes, may harbor significantly more water than previously estimated by concealing it deep beneath thick, hydrogen-rich atmospheres.
    #Astronomy #Astrophysics #PlanetaryScience #Astrochemistry #sflorg
    sflorg.com/2026/07/astr0713260

  12. The most common type of planet in the galaxy, known as mini- or sub-Neptunes, may harbor significantly more water than previously estimated by concealing it deep beneath thick, hydrogen-rich atmospheres.
    #Astronomy #Astrophysics #PlanetaryScience #Astrochemistry #sflorg
    sflorg.com/2026/07/astr0713260

  13. The most common type of planet in the galaxy, known as mini- or sub-Neptunes, may harbor significantly more water than previously estimated by concealing it deep beneath thick, hydrogen-rich atmospheres.
    #Astronomy #Astrophysics #PlanetaryScience #Astrochemistry #sflorg
    sflorg.com/2026/07/astr0713260

  14. The most common type of planet in the galaxy, known as mini- or sub-Neptunes, may harbor significantly more water than previously estimated by concealing it deep beneath thick, hydrogen-rich atmospheres.
    #Astronomy #Astrophysics #PlanetaryScience #Astrochemistry #sflorg
    sflorg.com/2026/07/astr0713260

  15. Astronomers Discover Mysterious Compound on Pluto and Titan

    📰 Original title: Mysterious Compound Detected on Pluto and Titan

    🤖 IA: It's not clickbait ✅
    👥 Users: It's not clickbait ✅

    View full AI summary en.killbait.com/astronomers-di

    #science #spectroscopy #planetaryscience #astrochemistry

  16. Astronomers Discover Mysterious Compound on Pluto and Titan

    📰 Original title: Mysterious Compound Detected on Pluto and Titan

    🤖 IA: It's not clickbait ✅
    👥 Users: It's not clickbait ✅

    View full AI summary en.killbait.com/astronomers-di

    #science #spectroscopy #planetaryscience #astrochemistry

  17. Astronomers Discover Mysterious Compound on Pluto and Titan

    📰 Original title: Mysterious Compound Detected on Pluto and Titan

    🤖 IA: It's not clickbait ✅
    👥 Users: It's not clickbait ✅

    View full AI summary en.killbait.com/astronomers-di

    #science #spectroscopy #planetaryscience #astrochemistry

  18. Planetary engulfment is an astronomical event in which a star consumes an orbiting planet. This process rapidly alters the star's chemical composition, leaving behind distinct and measurable elemental signatures.
    #Astronomy #Astrophysics #Astrochemistry #sflorg
    sflorg.com/2026/06/astr0615260

  19. Planetary engulfment is an astronomical event in which a star consumes an orbiting planet. This process rapidly alters the star's chemical composition, leaving behind distinct and measurable elemental signatures.
    #Astronomy #Astrophysics #Astrochemistry #sflorg
    sflorg.com/2026/06/astr0615260

  20. Planetary engulfment is an astronomical event in which a star consumes an orbiting planet. This process rapidly alters the star's chemical composition, leaving behind distinct and measurable elemental signatures.
    #Astronomy #Astrophysics #Astrochemistry #sflorg
    sflorg.com/2026/06/astr0615260

  21. Planetary engulfment is an astronomical event in which a star consumes an orbiting planet. This process rapidly alters the star's chemical composition, leaving behind distinct and measurable elemental signatures.
    #Astronomy #Astrophysics #Astrochemistry #sflorg
    sflorg.com/2026/06/astr0615260

  22. Planetary engulfment is an astronomical event in which a star consumes an orbiting planet. This process rapidly alters the star's chemical composition, leaving behind distinct and measurable elemental signatures.
    #Astronomy #Astrophysics #Astrochemistry #sflorg
    sflorg.com/2026/06/astr0615260

  23. Weekly Update from the Open Journal of Astrophysics 13/06/2026

    It’s Saturday again so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further three papers, bringing the number in Volume 9 (2026) to 122 and the total so far published by OJAp up to 570.

    I will continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week, published on Thursday 11th June, is “Dancing Streams In Merging Halos: Stellar Streams in a MW–LMC-like merger” by (all based in the USA): Sachi Weerasooriya (Carnegie Observatories), Tjitske Starkenburg (Northwestern U.), Emily C. Cunningham (Columbia U.) & Kathryn V. Johnston (Flatiron Institute). This article explores how galaxy mergers, like the Milky Way-Large Magellanic Cloud merger, significantly alter the properties and structures of stellar streams, challenging the recovery of their initial orbits. It is in the folder marked Astrophysics of Galaxies.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/116730200889106529

    The second paper for this week, also published on Thursday 11th June but in the folder Cosmology and Nongalactic Astrophysics is “X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates” by Christopher Hopp, David Wittman, Rodrigo Stancioli, Zhuoran Gao & Faik Bouhrik (UC Davis) and Scott Adler (Rochester), all based in the USA. The X-SORTER program identifies merging galaxy clusters to study dark matter interactions, using optical indicators and X-ray observations. This method efficiently identifies active clusters suitable for detailed dark matter studies.

    The overlay for this one looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/116730279994960097

    The third and final paper of the week, published on Friday 12th June in the folder Earth and Planetary Astrophysics, is “JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS” by Jason T. Hinkle (U. Illinois, USA) and 6 others based in the USA and Chile. This article presents observations of the third Interstellar Object, 3I/ATLAS, providing early sub-mm constraints on its activity. The findings suggest a steeper production rate slope than typical Solar System comets.

    The overlay for this one is here:

    The final, accepted version can be found on arXiv here and the Mastodon announcement is here:

    https://fediscience.org/@OJ_Astro/116735805179724489

    And that concludes this week’s update. It has been a slow week on the publishing front, but the main reason is that we have a big backlog of papers accepted but waiting for the authors to put their final versions on arXiv and we can’t do anything about that! I’ll do another update next Saturday.

    #3IAtlas #arXiv250514792v2 #arXiv251202106v3 #arXiv260305596v4 #astrochemistry #AstrophysicsOfGalaxies #CO #cosmologicalSimulations #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #EarthAndPlanetaryAstrophysics #galaxyClusters #GalaxyHalos #galaxyMergers #HCN #HighEnergyAstrophysicalPhenomena #interstellarObjects #OpenAccess #OpenAccessPublishing #spectroscopy #StellarStreams #XSORTER
  24. Weekly Update from the Open Journal of Astrophysics 13/06/2026

    It’s Saturday again so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further three papers, bringing the number in Volume 9 (2026) to 122 and the total so far published by OJAp up to 570.

    I will continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week, published on Thursday 11th June, is “Dancing Streams In Merging Halos: Stellar Streams in a MW–LMC-like merger” by (all based in the USA): Sachi Weerasooriya (Carnegie Observatories), Tjitske Starkenburg (Northwestern U.), Emily C. Cunningham (Columbia U.) & Kathryn V. Johnston (Flatiron Institute). This article explores how galaxy mergers, like the Milky Way-Large Magellanic Cloud merger, significantly alter the properties and structures of stellar streams, challenging the recovery of their initial orbits. It is in the folder marked Astrophysics of Galaxies.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/116730200889106529

    The second paper for this week, also published on Thursday 11th June but in the folder Cosmology and Nongalactic Astrophysics is “X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates” by Christopher Hopp, David Wittman, Rodrigo Stancioli, Zhuoran Gao & Faik Bouhrik (UC Davis) and Scott Adler (Rochester), all based in the USA. The X-SORTER program identifies merging galaxy clusters to study dark matter interactions, using optical indicators and X-ray observations. This method efficiently identifies active clusters suitable for detailed dark matter studies.

    The overlay for this one looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/116730279994960097

    The third and final paper of the week, published on Friday 12th June in the folder Earth and Planetary Astrophysics, is “JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS” by Jason T. Hinkle (U. Illinois, USA) and 6 others based in the USA and Chile. This article presents observations of the third Interstellar Object, 3I/ATLAS, providing early sub-mm constraints on its activity. The findings suggest a steeper production rate slope than typical Solar System comets.

    The overlay for this one is here:

    The final, accepted version can be found on arXiv here and the Mastodon announcement is here:

    https://fediscience.org/@OJ_Astro/116735805179724489

    And that concludes this week’s update. It has been a slow week on the publishing front, but the main reason is that we have a big backlog of papers accepted but waiting for the authors to put their final versions on arXiv and we can’t do anything about that! I’ll do another update next Saturday.

    #3IAtlas #arXiv250514792v2 #arXiv251202106v3 #arXiv260305596v4 #astrochemistry #AstrophysicsOfGalaxies #CO #cosmologicalSimulations #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #EarthAndPlanetaryAstrophysics #galaxyClusters #GalaxyHalos #galaxyMergers #HCN #HighEnergyAstrophysicalPhenomena #interstellarObjects #OpenAccess #OpenAccessPublishing #spectroscopy #StellarStreams #XSORTER
  25. Weekly Update from the Open Journal of Astrophysics 13/06/2026

    It’s Saturday again so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further three papers, bringing the number in Volume 9 (2026) to 122 and the total so far published by OJAp up to 570.

    I will continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week, published on Thursday 11th June, is “Dancing Streams In Merging Halos: Stellar Streams in a MW–LMC-like merger” by (all based in the USA): Sachi Weerasooriya (Carnegie Observatories), Tjitske Starkenburg (Northwestern U.), Emily C. Cunningham (Columbia U.) & Kathryn V. Johnston (Flatiron Institute). This article explores how galaxy mergers, like the Milky Way-Large Magellanic Cloud merger, significantly alter the properties and structures of stellar streams, challenging the recovery of their initial orbits. It is in the folder marked Astrophysics of Galaxies.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/116730200889106529

    The second paper for this week, also published on Thursday 11th June but in the folder Cosmology and Nongalactic Astrophysics is “X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates” by Christopher Hopp, David Wittman, Rodrigo Stancioli, Zhuoran Gao & Faik Bouhrik (UC Davis) and Scott Adler (Rochester), all based in the USA. The X-SORTER program identifies merging galaxy clusters to study dark matter interactions, using optical indicators and X-ray observations. This method efficiently identifies active clusters suitable for detailed dark matter studies.

    The overlay for this one looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/116730279994960097

    The third and final paper of the week, published on Friday 12th June in the folder Earth and Planetary Astrophysics, is “JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS” by Jason T. Hinkle (U. Illinois, USA) and 6 others based in the USA and Chile. This article presents observations of the third Interstellar Object, 3I/ATLAS, providing early sub-mm constraints on its activity. The findings suggest a steeper production rate slope than typical Solar System comets.

    The overlay for this one is here:

    The final, accepted version can be found on arXiv here and the Mastodon announcement is here:

    https://fediscience.org/@OJ_Astro/116735805179724489

    And that concludes this week’s update. It has been a slow week on the publishing front, but the main reason is that we have a big backlog of papers accepted but waiting for the authors to put their final versions on arXiv and we can’t do anything about that! I’ll do another update next Saturday.

    #3IAtlas #arXiv250514792v2 #arXiv251202106v3 #arXiv260305596v4 #astrochemistry #AstrophysicsOfGalaxies #CO #cosmologicalSimulations #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #EarthAndPlanetaryAstrophysics #galaxyClusters #GalaxyHalos #galaxyMergers #HCN #HighEnergyAstrophysicalPhenomena #interstellarObjects #OpenAccess #OpenAccessPublishing #spectroscopy #StellarStreams #XSORTER
  26. Weekly Update from the Open Journal of Astrophysics 13/06/2026

    It’s Saturday again so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further three papers, bringing the number in Volume 9 (2026) to 122 and the total so far published by OJAp up to 570.

    I will continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week, published on Thursday 11th June, is “Dancing Streams In Merging Halos: Stellar Streams in a MW–LMC-like merger” by (all based in the USA): Sachi Weerasooriya (Carnegie Observatories), Tjitske Starkenburg (Northwestern U.), Emily C. Cunningham (Columbia U.) & Kathryn V. Johnston (Flatiron Institute). This article explores how galaxy mergers, like the Milky Way-Large Magellanic Cloud merger, significantly alter the properties and structures of stellar streams, challenging the recovery of their initial orbits. It is in the folder marked Astrophysics of Galaxies.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/116730200889106529

    The second paper for this week, also published on Thursday 11th June but in the folder Cosmology and Nongalactic Astrophysics is “X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates” by Christopher Hopp, David Wittman, Rodrigo Stancioli, Zhuoran Gao & Faik Bouhrik (UC Davis) and Scott Adler (Rochester), all based in the USA. The X-SORTER program identifies merging galaxy clusters to study dark matter interactions, using optical indicators and X-ray observations. This method efficiently identifies active clusters suitable for detailed dark matter studies.

    The overlay for this one looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/116730279994960097

    The third and final paper of the week, published on Friday 12th June in the folder Earth and Planetary Astrophysics, is “JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS” by Jason T. Hinkle (U. Illinois, USA) and 6 others based in the USA and Chile. This article presents observations of the third Interstellar Object, 3I/ATLAS, providing early sub-mm constraints on its activity. The findings suggest a steeper production rate slope than typical Solar System comets.

    The overlay for this one is here:

    The final, accepted version can be found on arXiv here and the Mastodon announcement is here:

    https://fediscience.org/@OJ_Astro/116735805179724489

    And that concludes this week’s update. It has been a slow week on the publishing front, but the main reason is that we have a big backlog of papers accepted but waiting for the authors to put their final versions on arXiv and we can’t do anything about that! I’ll do another update next Saturday.

    #3IAtlas #arXiv250514792v2 #arXiv251202106v3 #arXiv260305596v4 #astrochemistry #AstrophysicsOfGalaxies #CO #cosmologicalSimulations #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #EarthAndPlanetaryAstrophysics #galaxyClusters #GalaxyHalos #galaxyMergers #HCN #HighEnergyAstrophysicalPhenomena #interstellarObjects #OpenAccess #OpenAccessPublishing #spectroscopy #StellarStreams #XSORTER
  27. Weekly Update from the Open Journal of Astrophysics 13/06/2026

    It’s Saturday again so it’s time for another update of activity at the Open Journal of Astrophysics. Since the last update we have published a further three papers, bringing the number in Volume 9 (2026) to 122 and the total so far published by OJAp up to 570.

    I will continue to include the posts made on our Mastodon account (on Fediscience); these announcements also show the DOI for each paper.

    The first paper to report this week, published on Thursday 11th June, is “Dancing Streams In Merging Halos: Stellar Streams in a MW–LMC-like merger” by (all based in the USA): Sachi Weerasooriya (Carnegie Observatories), Tjitske Starkenburg (Northwestern U.), Emily C. Cunningham (Columbia U.) & Kathryn V. Johnston (Flatiron Institute). This article explores how galaxy mergers, like the Milky Way-Large Magellanic Cloud merger, significantly alter the properties and structures of stellar streams, challenging the recovery of their initial orbits. It is in the folder marked Astrophysics of Galaxies.

    The overlay for this paper is here

    You can find the officially accepted version on arXiv here and the announcement on Fediverse here:

    https://fediscience.org/@OJ_Astro/116730200889106529

    The second paper for this week, also published on Thursday 11th June but in the folder Cosmology and Nongalactic Astrophysics is “X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates” by Christopher Hopp, David Wittman, Rodrigo Stancioli, Zhuoran Gao & Faik Bouhrik (UC Davis) and Scott Adler (Rochester), all based in the USA. The X-SORTER program identifies merging galaxy clusters to study dark matter interactions, using optical indicators and X-ray observations. This method efficiently identifies active clusters suitable for detailed dark matter studies.

    The overlay for this one looks like this:

    The official version of the paper can be found on arXiv here and the Fediverse announcement here:

    https://fediscience.org/@OJ_Astro/116730279994960097

    The third and final paper of the week, published on Friday 12the June in the folder Earth and Planetary Astrophysics, is “JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS” by Jason T. Hinkle (U. Illinois, USA) and 6 others based in the USA and Chile. This article presents observations of the third Interstellar Object, 3I/ATLAS, providing early sub-mm constraints on its activity. The findings suggest a steeper production rate slope than typical Solar System comets.

    The overlay for this one is here:

    The final, accepted version can be found on arXiv here and the Mastodon announcement is here:

    https://fediscience.org/@OJ_Astro/116735805179724489

    And that concludes this week’s update. It has been a slow week on the publishing front, but the main reason is that we have a big backlog of papers accepted but waiting for the authors to put their final versions on arXiv and we can’t do anything about that! I’ll do another update next Saturday.

    #3IAtlas #arXiv250514792v2 #arXiv251202106v3 #arXiv260305596v4 #astrochemistry #AstrophysicsOfGalaxies #CO #cosmologicalSimulations #CosmologyAndNonGalacticAstrophysics #DiamondOpenAccess #DiamondOpenAccessPublishing #EarthAndPlanetaryAstrophysics #galaxyClusters #GalaxyHalos #galaxyMergers #HCN #HighEnergyAstrophysicalPhenomena #interstellarObjects #OpenAccess #OpenAccessPublishing #spectroscopy #StellarStreams #XSORTER
  28. This event marks the simultaneous observation of the interstellar comet 3I/ATLAS by Ultraviolet Spectrograph (UVS) instruments aboard ESA's Juice and NASA's Europa Clipper spacecraft. The informally coordinated effort successfully captured the comet's ultraviolet emissions, gas breakdown, and scattered dust from both hemispheres.
    #Astronomy #PlanetaryScience #Astrochemistry #Astrophysics #Spacecrafts #sflorg
    sflorg.com/2026/05/astr0513260

  29. This event marks the simultaneous observation of the interstellar comet 3I/ATLAS by Ultraviolet Spectrograph (UVS) instruments aboard ESA's Juice and NASA's Europa Clipper spacecraft. The informally coordinated effort successfully captured the comet's ultraviolet emissions, gas breakdown, and scattered dust from both hemispheres.
    #Astronomy #PlanetaryScience #Astrochemistry #Astrophysics #Spacecrafts #sflorg
    sflorg.com/2026/05/astr0513260

  30. This event marks the simultaneous observation of the interstellar comet 3I/ATLAS by Ultraviolet Spectrograph (UVS) instruments aboard ESA's Juice and NASA's Europa Clipper spacecraft. The informally coordinated effort successfully captured the comet's ultraviolet emissions, gas breakdown, and scattered dust from both hemispheres.
    #Astronomy #PlanetaryScience #Astrochemistry #Astrophysics #Spacecrafts #sflorg
    sflorg.com/2026/05/astr0513260

  31. This event marks the simultaneous observation of the interstellar comet 3I/ATLAS by Ultraviolet Spectrograph (UVS) instruments aboard ESA's Juice and NASA's Europa Clipper spacecraft. The informally coordinated effort successfully captured the comet's ultraviolet emissions, gas breakdown, and scattered dust from both hemispheres.
    #Astronomy #PlanetaryScience #Astrochemistry #Astrophysics #Spacecrafts #sflorg
    sflorg.com/2026/05/astr0513260

  32. This event marks the simultaneous observation of the interstellar comet 3I/ATLAS by Ultraviolet Spectrograph (UVS) instruments aboard ESA's Juice and NASA's Europa Clipper spacecraft. The informally coordinated effort successfully captured the comet's ultraviolet emissions, gas breakdown, and scattered dust from both hemispheres.
    #Astronomy #PlanetaryScience #Astrochemistry #Astrophysics #Spacecrafts #sflorg
    sflorg.com/2026/05/astr0513260

  33. Detecting Molecules in Space: Excitement and Caution in the Search for Life

    📰 Original title: Potential signs of life on distant planets sound exciting – but confirmation can take years

    🤖 IA: It's clickbait ⚠️
    👥 Usuarios: It's clickbait ⚠️

    View full AI summary: killbait.com/en/detecting-mole

    #astronomy #astrochemistry #exoplanets #biosignatures

  34. Detecting Molecules in Space: Excitement and Caution in the Search for Life

    📰 Original title: Potential signs of life on distant planets sound exciting – but confirmation can take years

    🤖 IA: It's clickbait ⚠️
    👥 Usuarios: It's clickbait ⚠️

    View full AI summary: killbait.com/en/detecting-mole

    #astronomy #astrochemistry #exoplanets #biosignatures

  35. Detecting Molecules in Space: Excitement and Caution in the Search for Life

    📰 Original title: Potential signs of life on distant planets sound exciting – but confirmation can take years

    🤖 IA: It's clickbait ⚠️
    👥 Usuarios: It's clickbait ⚠️

    View full AI summary: killbait.com/en/detecting-mole

    #astronomy #astrochemistry #exoplanets #biosignatures

  36. Detecting Molecules in Space: Excitement and Caution in the Search for Life

    📰 Original title: Potential signs of life on distant planets sound exciting – but confirmation can take years

    🤖 IA: It's clickbait ⚠️
    👥 Usuarios: It's clickbait ⚠️

    View full AI summary: killbait.com/en/detecting-mole

    #astronomy #astrochemistry #exoplanets #biosignatures

  37. Moons orbiting free-floating planets can maintain liquid water oceans and potentially support complex life for billions of years without a parent star, utilizing dense hydrogen atmospheres and tidal heating.
    #Astrophysics #Astrochemistry #Biophysics #sflorg
    sflorg.com/2026/03/asph0311260

  38. Moons orbiting free-floating planets can maintain liquid water oceans and potentially support complex life for billions of years without a parent star, utilizing dense hydrogen atmospheres and tidal heating.
    #Astrophysics #Astrochemistry #Biophysics #sflorg
    sflorg.com/2026/03/asph0311260

  39. Moons orbiting free-floating planets can maintain liquid water oceans and potentially support complex life for billions of years without a parent star, utilizing dense hydrogen atmospheres and tidal heating.
    #Astrophysics #Astrochemistry #Biophysics #sflorg
    sflorg.com/2026/03/asph0311260

  40. Moons orbiting free-floating planets can maintain liquid water oceans and potentially support complex life for billions of years without a parent star, utilizing dense hydrogen atmospheres and tidal heating.
    #Astrophysics #Astrochemistry #Biophysics #sflorg
    sflorg.com/2026/03/asph0311260

  41. Moons orbiting free-floating planets can maintain liquid water oceans and potentially support complex life for billions of years without a parent star, utilizing dense hydrogen atmospheres and tidal heating.
    #Astrophysics #Astrochemistry #Biophysics #sflorg
    sflorg.com/2026/03/asph0311260

  42. Researchers have definitively identified nitrous oxide (N₂O), commonly known as "laughing gas," within the solid ice mantles coating dust particles around young #protostars
    #Astrophysics #Astrochemistry #Astronomy #sflorg
    sflorg.com/2026/01/asph0124260

  43. Researchers have definitively identified nitrous oxide (N₂O), commonly known as "laughing gas," within the solid ice mantles coating dust particles around young #protostars
    #Astrophysics #Astrochemistry #Astronomy #sflorg
    sflorg.com/2026/01/asph0124260

  44. Researchers have definitively identified nitrous oxide (N₂O), commonly known as "laughing gas," within the solid ice mantles coating dust particles around young #protostars
    #Astrophysics #Astrochemistry #Astronomy #sflorg
    sflorg.com/2026/01/asph0124260

  45. Researchers have definitively identified nitrous oxide (N₂O), commonly known as "laughing gas," within the solid ice mantles coating dust particles around young #protostars
    #Astrophysics #Astrochemistry #Astronomy #sflorg
    sflorg.com/2026/01/asph0124260

  46. Researchers have definitively identified nitrous oxide (N₂O), commonly known as "laughing gas," within the solid ice mantles coating dust particles around young #protostars
    #Astrophysics #Astrochemistry #Astronomy #sflorg
    sflorg.com/2026/01/asph0124260

  47. Weiter geht's mit 25 Jahre First Lasing #FLASH #TTF @DESY

    Melanie Schnell: From FLASH to the Stars - Photochemistry of Polycyclic Aromatic Hydrocarbons

    Heute ein faszinierender Blick „von FLASH bis zu den Sternen“: Melanie Schnell zeigt, wie wir mit modernen Laser- und Röntgenquellen die Photochemie polyzyklischer aromatischer Kohlenwasserstoffe (PAHs) untersuchen.

    Diese komplexen Kohlenstoffringe finden sich nicht nur in Flammen und unserer Atmosphäre, sondern auch im interstellaren Medium – überall in der Galaxie. Überraschend: Rund 10–20 % des gesamten galaktischen Kohlenstoffs steckt in PAH-Molekülen!

    Mit präzisen Labormethoden lassen sich ihre Strukturen und Reaktionen entschlüsseln – ein wichtiger Schritt, um besser zu verstehen, wie sich Moleküle im Weltraum bilden, verändern und vielleicht sogar Bausteine des Lebens hervorbringen. ✨🌌

    #Astrochemistry #PAH #FLASH #PhotonScience [Tröt unterstützt durch ein LLM]

  48. Weiter geht's mit 25 Jahre First Lasing #FLASH #TTF @DESY

    Melanie Schnell: From FLASH to the Stars - Photochemistry of Polycyclic Aromatic Hydrocarbons

    Heute ein faszinierender Blick „von FLASH bis zu den Sternen“: Melanie Schnell zeigt, wie wir mit modernen Laser- und Röntgenquellen die Photochemie polyzyklischer aromatischer Kohlenwasserstoffe (PAHs) untersuchen.

    Diese komplexen Kohlenstoffringe finden sich nicht nur in Flammen und unserer Atmosphäre, sondern auch im interstellaren Medium – überall in der Galaxie. Überraschend: Rund 10–20 % des gesamten galaktischen Kohlenstoffs steckt in PAH-Molekülen!

    Mit präzisen Labormethoden lassen sich ihre Strukturen und Reaktionen entschlüsseln – ein wichtiger Schritt, um besser zu verstehen, wie sich Moleküle im Weltraum bilden, verändern und vielleicht sogar Bausteine des Lebens hervorbringen. ✨🌌

    #Astrochemistry #PAH #FLASH #PhotonScience [Tröt unterstützt durch ein LLM]