#spacephysics — Public Fediverse posts
Live and recent posts from across the Fediverse tagged #spacephysics, aggregated by home.social.
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How the weather in space can affect us on Earth – and the team trying to protect us
At the Met Office headquarters, the screens in one corner of the control centre are focussed on …
#NewsBeep #News #Science #AberystwythUniversity #AU #Australia #BBC #BBC]"This #CarringtonEvent #DrSharman #HelenSharman #HuwMorgan #MetOffice #morgan #NationalRiskRegister #RichardCarrington #RichardStone #RichardStone's #Sharman #spacephysics #stone #Sun #suns #TheMetOffice
https://www.newsbeep.com/au/873016/ -
How the weather in space can affect us on Earth – and the team trying to protect us
At the Met Office headquarters, the screens in one corner of the control centre are focussed on …
#NewsBeep #News #Science #AberystwythUniversity #AU #Australia #BBC #BBC]"This #CarringtonEvent #DrSharman #HelenSharman #HuwMorgan #MetOffice #morgan #NationalRiskRegister #RichardCarrington #RichardStone #RichardStone's #Sharman #spacephysics #stone #Sun #suns #TheMetOffice
https://www.newsbeep.com/au/873016/ -
🌖🌊 Possible liquid #nitrogen flows on #Pluto.
A new study argues that dark features in northern #SputnikPlanitia may be traces of N₂ basal melt that rose through the nitrogen ice sheet, flowed briefly across the surface, and refroze.
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🌖🌊 Possible liquid #nitrogen flows on #Pluto.
A new study argues that dark features in northern #SputnikPlanitia may be traces of N₂ basal melt that rose through the nitrogen ice sheet, flowed briefly across the surface, and refroze.
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🌖🌊 Possible liquid #nitrogen flows on #Pluto.
A new study argues that dark features in northern #SputnikPlanitia may be traces of N₂ basal melt that rose through the nitrogen ice sheet, flowed briefly across the surface, and refroze.
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🌖🌊 Possible liquid #nitrogen flows on #Pluto.
A new study argues that dark features in northern #SputnikPlanitia may be traces of N₂ basal melt that rose through the nitrogen ice sheet, flowed briefly across the surface, and refroze.
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🌖🌊 Possible liquid #nitrogen flows on #Pluto.
A new study argues that dark features in northern #SputnikPlanitia may be traces of N₂ basal melt that rose through the nitrogen ice sheet, flowed briefly across the surface, and refroze.
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Especially interesting: #Reconnection at #Mars is not just a local #plasma process. It can restructure the induced #magnetosphere, generate flux ropes and jets, open magnetic escape pathways, contribute to #auroral activity, and possibly affect #atmospheric ion loss.
Even a planet without a global #MagneticField can have very dynamic #PlasmaPhysics.
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Especially interesting: #Reconnection at #Mars is not just a local #plasma process. It can restructure the induced #magnetosphere, generate flux ropes and jets, open magnetic escape pathways, contribute to #auroral activity, and possibly affect #atmospheric ion loss.
Even a planet without a global #MagneticField can have very dynamic #PlasmaPhysics.
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Especially interesting: #Reconnection at #Mars is not just a local #plasma process. It can restructure the induced #magnetosphere, generate flux ropes and jets, open magnetic escape pathways, contribute to #auroral activity, and possibly affect #atmospheric ion loss.
Even a planet without a global #MagneticField can have very dynamic #PlasmaPhysics.
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Especially interesting: #Reconnection at #Mars is not just a local #plasma process. It can restructure the induced #magnetosphere, generate flux ropes and jets, open magnetic escape pathways, contribute to #auroral activity, and possibly affect #atmospheric ion loss.
Even a planet without a global #MagneticField can have very dynamic #PlasmaPhysics.
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Especially interesting: #Reconnection at #Mars is not just a local #plasma process. It can restructure the induced #magnetosphere, generate flux ropes and jets, open magnetic escape pathways, contribute to #auroral activity, and possibly affect #atmospheric ion loss.
Even a planet without a global #MagneticField can have very dynamic #PlasmaPhysics.
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Nice review on #MagneticReconnection 🧲 ❌ in #Mars’ space environment:
📝 https://doi.org/10.1007/s11038-026-09597-z
Lin, R., Huang, S., Jiang, K. et al. Recent advances in magnetic reconnection in Mars’ space environment
Unlike #Earth, Mars has no global intrinsic dipole field. Its #plasma environment is shaped by the #SolarWind, an induced #magnetosphere, localized crustal #MagneticFields, and heavy planetary ions. …makes Mars a fascinating laboratory for reconnection physics.
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Nice review on #MagneticReconnection 🧲 ❌ in #Mars’ space environment:
📝 https://doi.org/10.1007/s11038-026-09597-z
Lin, R., Huang, S., Jiang, K. et al. Recent advances in magnetic reconnection in Mars’ space environment
Unlike #Earth, Mars has no global intrinsic dipole field. Its #plasma environment is shaped by the #SolarWind, an induced #magnetosphere, localized crustal #MagneticFields, and heavy planetary ions. …makes Mars a fascinating laboratory for reconnection physics.
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Nice review on #MagneticReconnection 🧲 ❌ in #Mars’ space environment:
📝 https://doi.org/10.1007/s11038-026-09597-z
Lin, R., Huang, S., Jiang, K. et al. Recent advances in magnetic reconnection in Mars’ space environment
Unlike #Earth, Mars has no global intrinsic dipole field. Its #plasma environment is shaped by the #SolarWind, an induced #magnetosphere, localized crustal #MagneticFields, and heavy planetary ions. …makes Mars a fascinating laboratory for reconnection physics.
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Nice review on #MagneticReconnection 🧲 ❌ in #Mars’ space environment:
📝 https://doi.org/10.1007/s11038-026-09597-z
Lin, R., Huang, S., Jiang, K. et al. Recent advances in magnetic reconnection in Mars’ space environment
Unlike #Earth, Mars has no global intrinsic dipole field. Its #plasma environment is shaped by the #SolarWind, an induced #magnetosphere, localized crustal #MagneticFields, and heavy planetary ions. …makes Mars a fascinating laboratory for reconnection physics.
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Nice review on #MagneticReconnection 🧲 ❌ in #Mars’ space environment:
📝 https://doi.org/10.1007/s11038-026-09597-z
Lin, R., Huang, S., Jiang, K. et al. Recent advances in magnetic reconnection in Mars’ space environment
Unlike #Earth, Mars has no global intrinsic dipole field. Its #plasma environment is shaped by the #SolarWind, an induced #magnetosphere, localized crustal #MagneticFields, and heavy planetary ions. …makes Mars a fascinating laboratory for reconnection physics.
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Groundbreaking research analyzing newly documented explosive releases of magnetic energy and high-energy particle bursts that occur along the boundaries of incoming coronal mass ejections (CMEs) in close proximity to Earth.
#SpacePhysics #Heliophysics #MagnetosphericPhysics #sflorg
https://www.sflorg.com/2026/08/heli08182601.html -
Groundbreaking research analyzing newly documented explosive releases of magnetic energy and high-energy particle bursts that occur along the boundaries of incoming coronal mass ejections (CMEs) in close proximity to Earth.
#SpacePhysics #Heliophysics #MagnetosphericPhysics #sflorg
https://www.sflorg.com/2026/08/heli08182601.html -
Groundbreaking research analyzing newly documented explosive releases of magnetic energy and high-energy particle bursts that occur along the boundaries of incoming coronal mass ejections (CMEs) in close proximity to Earth.
#SpacePhysics #Heliophysics #MagnetosphericPhysics #sflorg
https://www.sflorg.com/2026/08/heli08182601.html -
Groundbreaking research analyzing newly documented explosive releases of magnetic energy and high-energy particle bursts that occur along the boundaries of incoming coronal mass ejections (CMEs) in close proximity to Earth.
#SpacePhysics #Heliophysics #MagnetosphericPhysics #sflorg
https://www.sflorg.com/2026/08/heli08182601.html -
Groundbreaking research analyzing newly documented explosive releases of magnetic energy and high-energy particle bursts that occur along the boundaries of incoming coronal mass ejections (CMEs) in close proximity to Earth.
#SpacePhysics #Heliophysics #MagnetosphericPhysics #sflorg
https://www.sflorg.com/2026/08/heli08182601.html -
@Umbertogaetani One thing that surprised me: I don’t see Roth et al.’s #HST work on #Europa’s #plume/water-vapor signatures cited here, nor Saur et al. or much from the Europa #SpacePlasma community.
Not fatal for their thermo-fluid model I guess, but given the broader claim about limited #ocean–#surface exchange, it feels like a gap in the framing.
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@Umbertogaetani One thing that surprised me: I don’t see Roth et al.’s #HST work on #Europa’s #plume/water-vapor signatures cited here, nor Saur et al. or much from the Europa #SpacePlasma community.
Not fatal for their thermo-fluid model I guess, but given the broader claim about limited #ocean–#surface exchange, it feels like a gap in the framing.
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@Umbertogaetani One thing that surprised me: I don’t see Roth et al.’s #HST work on #Europa’s #plume/water-vapor signatures cited here, nor Saur et al. or much from the Europa #SpacePlasma community.
Not fatal for their thermo-fluid model I guess, but given the broader claim about limited #ocean–#surface exchange, it feels like a gap in the framing.
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@Umbertogaetani One thing that surprised me: I don’t see Roth et al.’s #HST work on #Europa’s #plume/water-vapor signatures cited here, nor Saur et al. or much from the Europa #SpacePlasma community.
Not fatal for their thermo-fluid model I guess, but given the broader claim about limited #ocean–#surface exchange, it feels like a gap in the framing.
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@Umbertogaetani One thing that surprised me: I don’t see Roth et al.’s #HST work on #Europa’s #plume/water-vapor signatures cited here, nor Saur et al. or much from the Europa #SpacePlasma community.
Not fatal for their thermo-fluid model I guess, but given the broader claim about limited #ocean–#surface exchange, it feels like a gap in the framing.
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@Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.
If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.
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@Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.
If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.
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@Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.
If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.
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@Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.
If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.
-
@Umbertogaetani Their simulations suggest that #water rising through narrow dykes would freeze too quickly to supply the volumes needed for features such as chaos terrain, pits, domes or ridges. #Turbulence makes this worse by enhancing heat loss, supercooling the water, producing frazil ice, and clogging the dyke.
If correct, shallow liquid reservoirs on #Europa may form more by local in situ melting than by direct #ocean-to-surface exchange.
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RE: https://mastodon.uno/@Umbertogaetani/117077488353005365
🌖🌊 Interesting new #NatureAstronomy paper on #Europa’s #subsurface #ocean:
Ojha, Barik & Buffo argue that direct liquid-water transport from Europa’s deep ocean into shallow subsurface reservoirs may be much more limited than often assumed.
🌍 https://doi.org/10.1038/s41550-026-02918-2
Thanks @Umbertogaetani for sharing ✌️
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RE: https://mastodon.uno/@Umbertogaetani/117077488353005365
🌖🌊 Interesting new #NatureAstronomy paper on #Europa’s #subsurface #ocean:
Ojha, Barik & Buffo argue that direct liquid-water transport from Europa’s deep ocean into shallow subsurface reservoirs may be much more limited than often assumed.
🌍 https://doi.org/10.1038/s41550-026-02918-2
Thanks @Umbertogaetani for sharing ✌️
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RE: https://mastodon.uno/@Umbertogaetani/117077488353005365
🌖🌊 Interesting new #NatureAstronomy paper on #Europa’s #subsurface #ocean:
Ojha, Barik & Buffo argue that direct liquid-water transport from Europa’s deep ocean into shallow subsurface reservoirs may be much more limited than often assumed.
🌍 https://doi.org/10.1038/s41550-026-02918-2
Thanks @Umbertogaetani for sharing ✌️
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RE: https://mastodon.uno/@Umbertogaetani/117077488353005365
🌖🌊 Interesting new #NatureAstronomy paper on #Europa’s #subsurface #ocean:
Ojha, Barik & Buffo argue that direct liquid-water transport from Europa’s deep ocean into shallow subsurface reservoirs may be much more limited than often assumed.
🌍 https://doi.org/10.1038/s41550-026-02918-2
Thanks @Umbertogaetani for sharing ✌️
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RE: https://mastodon.uno/@Umbertogaetani/117077488353005365
🌖🌊 Interesting new #NatureAstronomy paper on #Europa’s #subsurface #ocean:
Ojha, Barik & Buffo argue that direct liquid-water transport from Europa’s deep ocean into shallow subsurface reservoirs may be much more limited than often assumed.
🌍 https://doi.org/10.1038/s41550-026-02918-2
Thanks @Umbertogaetani for sharing ✌️
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This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.
That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥
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This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.
That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥
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This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.
That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥
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This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.
That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥
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This is the exciting part: #KHI can mix magnetized and non-magnetized #plasma, drive #turbulence, transport mass/energy/momentum/ #MagneticFlux, and may contribute to small-scale #magnetic braiding, thus one route by which free #MagneticEnergy is built up in the solar #atmosphere.
That makes them relevant to the long-standing puzzle of why the #corona is heated to millions of kelvin while the visible surface is only ~5,800 K. 😎🔥
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For the first time, #KelvinHelmholtzInstabilities 🌀 have been directly observed in the #Sun’s #photosphere ☀️🔭
#DKIST images reveal tiny #vortex-like structures at the edges of #MagneticFlux concentrations. #MHD simulations reproduce them and show that shear flows along these #magnetic boundaries trigger the instability.
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For the first time, #KelvinHelmholtzInstabilities 🌀 have been directly observed in the #Sun’s #photosphere ☀️🔭
#DKIST images reveal tiny #vortex-like structures at the edges of #MagneticFlux concentrations. #MHD simulations reproduce them and show that shear flows along these #magnetic boundaries trigger the instability.
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For the first time, #KelvinHelmholtzInstabilities 🌀 have been directly observed in the #Sun’s #photosphere ☀️🔭
#DKIST images reveal tiny #vortex-like structures at the edges of #MagneticFlux concentrations. #MHD simulations reproduce them and show that shear flows along these #magnetic boundaries trigger the instability.
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For the first time, #KelvinHelmholtzInstabilities 🌀 have been directly observed in the #Sun’s #photosphere ☀️🔭
#DKIST images reveal tiny #vortex-like structures at the edges of #MagneticFlux concentrations. #MHD simulations reproduce them and show that shear flows along these #magnetic boundaries trigger the instability.
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For the first time, #KelvinHelmholtzInstabilities 🌀 have been directly observed in the #Sun’s #photosphere ☀️🔭
#DKIST images reveal tiny #vortex-like structures at the edges of #MagneticFlux concentrations. #MHD simulations reproduce them and show that shear flows along these #magnetic boundaries trigger the instability.
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“A #telescope in #Chile has captured evidence of the impact caused by part of a SpaceX #Falcon9 rocket slamming into the moon while travelling at 8,690km/h (5,400mph).
The European Southern Observatory’s (ESO) Very Large Telescope observed “spectral lines” – a colourful illustration of the #sodium and #lithium gas – in the plume of #LunarDust stirred up by the impact.
The #ESO telescope recorded these “chemical fingerprints” of the plume, which were visible for five to 10 minutes, the #observatory said. The #plume measured a few tens of kilometres in size, according to #CarlSchmidt, an astronomer from #BostonUniversity’s Center for #SpacePhysics.”
#Moon <https://www.theguardian.com/science/2026/aug/06/spacex-rocket-crash-into-moon-impact>
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“A #telescope in #Chile has captured evidence of the impact caused by part of a SpaceX #Falcon9 rocket slamming into the moon while travelling at 8,690km/h (5,400mph).
The European Southern Observatory’s (ESO) Very Large Telescope observed “spectral lines” – a colourful illustration of the #sodium and #lithium gas – in the plume of #LunarDust stirred up by the impact.
The #ESO telescope recorded these “chemical fingerprints” of the plume, which were visible for five to 10 minutes, the #observatory said. The #plume measured a few tens of kilometres in size, according to #CarlSchmidt, an astronomer from #BostonUniversity’s Center for #SpacePhysics.”
#Moon <https://www.theguardian.com/science/2026/aug/06/spacex-rocket-crash-into-moon-impact>
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“A #telescope in #Chile has captured evidence of the impact caused by part of a SpaceX #Falcon9 rocket slamming into the moon while travelling at 8,690km/h (5,400mph).
The European Southern Observatory’s (ESO) Very Large Telescope observed “spectral lines” – a colourful illustration of the #sodium and #lithium gas – in the plume of #LunarDust stirred up by the impact.
The #ESO telescope recorded these “chemical fingerprints” of the plume, which were visible for five to 10 minutes, the #observatory said. The #plume measured a few tens of kilometres in size, according to #CarlSchmidt, an astronomer from #BostonUniversity’s Center for #SpacePhysics.”
#Moon <https://www.theguardian.com/science/2026/aug/06/spacex-rocket-crash-into-moon-impact>
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“A #telescope in #Chile has captured evidence of the impact caused by part of a SpaceX #Falcon9 rocket slamming into the moon while travelling at 8,690km/h (5,400mph).
The European Southern Observatory’s (ESO) Very Large Telescope observed “spectral lines” – a colourful illustration of the #sodium and #lithium gas – in the plume of #LunarDust stirred up by the impact.
The #ESO telescope recorded these “chemical fingerprints” of the plume, which were visible for five to 10 minutes, the #observatory said. The #plume measured a few tens of kilometres in size, according to #CarlSchmidt, an astronomer from #BostonUniversity’s Center for #SpacePhysics.”
#Moon <https://www.theguardian.com/science/2026/aug/06/spacex-rocket-crash-into-moon-impact>
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“A #telescope in #Chile has captured evidence of the impact caused by part of a SpaceX #Falcon9 rocket slamming into the moon while travelling at 8,690km/h (5,400mph).
The European Southern Observatory’s (ESO) Very Large Telescope observed “spectral lines” – a colourful illustration of the #sodium and #lithium gas – in the plume of #LunarDust stirred up by the impact.
The #ESO telescope recorded these “chemical fingerprints” of the plume, which were visible for five to 10 minutes, the #observatory said. The #plume measured a few tens of kilometres in size, according to #CarlSchmidt, an astronomer from #BostonUniversity’s Center for #SpacePhysics.”
#Moon <https://www.theguardian.com/science/2026/aug/06/spacex-rocket-crash-into-moon-impact>
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This made me very happy to read: An #asteroid has been named after Susanne Pfalzner.
I attended her lectures on #ComputationalAstrophysics and #StarFormation during my studies, and she later served as the 2nd examiner for my Master’s thesis. She is an outstanding scientist and lecturer, and this is such a well-deserved honor. My warmest congratulations to her! 👏👏👏
🌍 https://www.fz-juelich.de/en/jsc/news/news-items/news-flashes/2026/asteroid-pfalzner
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This made me very happy to read: An #asteroid has been named after Susanne Pfalzner.
I attended her lectures on #ComputationalAstrophysics and #StarFormation during my studies, and she later served as the 2nd examiner for my Master’s thesis. She is an outstanding scientist and lecturer, and this is such a well-deserved honor. My warmest congratulations to her! 👏👏👏
🌍 https://www.fz-juelich.de/en/jsc/news/news-items/news-flashes/2026/asteroid-pfalzner
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This made me very happy to read: An #asteroid has been named after Susanne Pfalzner.
I attended her lectures on #ComputationalAstrophysics and #StarFormation during my studies, and she later served as the 2nd examiner for my Master’s thesis. She is an outstanding scientist and lecturer, and this is such a well-deserved honor. My warmest congratulations to her! 👏👏👏
🌍 https://www.fz-juelich.de/en/jsc/news/news-items/news-flashes/2026/asteroid-pfalzner
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This made me very happy to read: An #asteroid has been named after Susanne Pfalzner.
I attended her lectures on #ComputationalAstrophysics and #StarFormation during my studies, and she later served as the 2nd examiner for my Master’s thesis. She is an outstanding scientist and lecturer, and this is such a well-deserved honor. My warmest congratulations to her! 👏👏👏
🌍 https://www.fz-juelich.de/en/jsc/news/news-items/news-flashes/2026/asteroid-pfalzner
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This made me very happy to read: An #asteroid has been named after Susanne Pfalzner.
I attended her lectures on #ComputationalAstrophysics and #StarFormation during my studies, and she later served as the 2nd examiner for my Master’s thesis. She is an outstanding scientist and lecturer, and this is such a well-deserved honor. My warmest congratulations to her! 👏👏👏
🌍 https://www.fz-juelich.de/en/jsc/news/news-items/news-flashes/2026/asteroid-pfalzner
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Save Hubble: the race to preserve the space telescope kicks off
Remnants of an exploded star, captured by the Hubble Space Telesope.Credit: NASA, ESA, and F. Summers, G. Bacon,…
#NewsBeep #News #US #USA #UnitedStates #UnitedStatesOfAmerica #Science #AstronomyandAstrophysics #HumanitiesandSocialSciences #multidisciplinary #Policy #Spacephysics
https://www.newsbeep.com/us/750030/ -
Save Hubble: the race to preserve the space telescope kicks off
Remnants of an exploded star, captured by the Hubble Space Telesope.Credit: NASA, ESA, and F. Summers, G. Bacon,…
#NewsBeep #News #US #USA #UnitedStates #UnitedStatesOfAmerica #Science #AstronomyandAstrophysics #HumanitiesandSocialSciences #multidisciplinary #Policy #Spacephysics
https://www.newsbeep.com/us/750030/ -
Save Hubble: the race to preserve the space telescope kicks off
Remnants of an exploded star, captured by the Hubble Space Telesope.Credit: NASA, ESA, and F. Summers, G. Bacon,…
#NewsBeep #News #Science #Astronomyandastrophysics #GB #HumanitiesandSocialSciences #multidisciplinary #Policy #Spacephysics #UK #UnitedKingdom
https://www.newsbeep.com/uk/679269/