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#protoplanetary — Public Fediverse posts

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

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  1. Winding Motion of Spirals in a Gravitationally Unstable #Protoplanetary Disk: arxiv.org/abs/2509.19761 -> Winding Motion of Planet-Forming Spirals Captured on Video for the First Time: alma-telescope.jp/en/news/pres -> Spirals in Planet-Forming Disk Caught Twisting for the First Time with ALMA: almaobservatory.org/en/press-r

  2. Winding Motion of Spirals in a Gravitationally Unstable #Protoplanetary Disk: arxiv.org/abs/2509.19761 -> Winding Motion of Planet-Forming Spirals Captured on Video for the First Time: alma-telescope.jp/en/news/pres -> Spirals in Planet-Forming Disk Caught Twisting for the First Time with ALMA: almaobservatory.org/en/press-r

  3. A #Protoplanetary #Disk is a rotating circumstellar disk of dense gas and dust surrounding a young, newly formed star.

    This disk is where planets, moons, and other celestial bodies are believed to form through the process of accretion.

    knowledgezone.co.in/kbits/65e8

  4. A #Protoplanetary #Disk is a rotating circumstellar disk of dense gas and dust surrounding a young, newly formed star.

    This disk is where planets, moons, and other celestial bodies are believed to form through the process of accretion.

    knowledgezone.co.in/kbits/65e8

  5. A deep Search for Ethylene Glycol and Glycolonitrile in the V883 Ori #Protoplanetary Disk: arxiv.org/abs/2507.14905 (and two slightly older papers) -> The evolution of life may have its origins in outer space: mpia.de/news/science/2025-05-v - astronomers find signs of complex organic molecules (precursors to sugars and amino acids) in a planet-forming disc.

  6. A deep Search for Ethylene Glycol and Glycolonitrile in the V883 Ori #Protoplanetary Disk: arxiv.org/abs/2507.14905 (and two slightly older papers) -> The evolution of life may have its origins in outer space: mpia.de/news/science/2025-05-v - astronomers find signs of complex organic molecules (precursors to sugars and amino acids) in a planet-forming disc.

  7. Astronomers have made a groundbreaking discovery in the #protoplanetary disc of V883 Orionis, detecting complex #organic molecules such as ethylene glycol and glycolonitrile. These compounds are potential precursors to sugars and #AminoAcids, suggesting that the building blocks of #life may form widely throughout the Universe. 🌌 #Astrophysics #OrganicMolecules

    mpia.de/news/science/2025-05-v

  8. Astronomers have made a groundbreaking discovery in the #protoplanetary disc of V883 Orionis, detecting complex #organic molecules such as ethylene glycol and glycolonitrile. These compounds are potential precursors to sugars and #AminoAcids, suggesting that the building blocks of #life may form widely throughout the Universe. 🌌 #Astrophysics #OrganicMolecules

    mpia.de/news/science/2025-05-v

  9. Initial results are promising: The water tornado's flow behaviour closely matches that of #protoplanetary discs, offering new insights into how dust particles interact and promote #planet formation.

    #PlanetaryScience #Innovation
    #Experiment #Simulation #Astronomy

    @unigreifswald

    mpia.de/news/science/2025-04-w

  10. Initial results are promising: The water tornado's flow behaviour closely matches that of #protoplanetary discs, offering new insights into how dust particles interact and promote #planet formation.

    #PlanetaryScience #Innovation
    #Experiment #Simulation #Astronomy

    @unigreifswald

    mpia.de/news/science/2025-04-w

  11. Refractory solid condensation detected in an embedded #protoplanetary disk: eso.org/public/archives/releas -> For the first time, astronomers witness the dawn of a new solar system: eso.org/public/news/eso2512/

  12. Refractory solid condensation detected in an embedded #protoplanetary disk: eso.org/public/archives/releas -> For the first time, astronomers witness the dawn of a new solar system: eso.org/public/news/eso2512/

  13. Protoplanetary disks from #ALMA.

    Though we have learned much about #exoplanets, there is still much we do not know about the steps of planet formation and the precise cosmic recipes that spawn the wide array of planetary bodies we have already uncovered.

    Astronomers have conducted one of the deepest surveys ever of #protoplanetary disks, the planet-forming dust belts around young #stars.

    The disks are as diverse as are the forming planetary systems.

    #astronomy
    almaobservatory.org/en/press-r

  14. Protoplanetary disks from #ALMA.

    Though we have learned much about #exoplanets, there is still much we do not know about the steps of planet formation and the precise cosmic recipes that spawn the wide array of planetary bodies we have already uncovered.

    Astronomers have conducted one of the deepest surveys ever of #protoplanetary disks, the planet-forming dust belts around young #stars.

    The disks are as diverse as are the forming planetary systems.

    #astronomy
    almaobservatory.org/en/press-r

  15. A high-resolution survey of #protoplanetary disks in Lupus and the nature of compact disks: arxiv.org/abs/2503.19504 -> Protoplanetary discs are much smaller than previously thought: astronomie.nl/nieuws/en/protop

  16. A high-resolution survey of #protoplanetary disks in Lupus and the nature of compact disks: arxiv.org/abs/2503.19504 -> Protoplanetary discs are much smaller than previously thought: astronomie.nl/nieuws/en/protop

  17. For decades, scientists have debated how small #exoplanets form.

    New model suggests that #planets form in narrow rings at specific locations in the #protoplanetary disk, making #planet formation more organized than previously believed.

    Simulations also imply that up to about 1% of super-Earth and mini-Neptune systems could host Earth-like planets within the #habitable zone.

    This implies an occurrence rate of approximately one Earth-like planet per 300 sun-like stars.

    astrobiology.com/2025/03/resea

  18. For decades, scientists have debated how small #exoplanets form.

    New model suggests that #planets form in narrow rings at specific locations in the #protoplanetary disk, making #planet formation more organized than previously believed.

    Simulations also imply that up to about 1% of super-Earth and mini-Neptune systems could host Earth-like planets within the #habitable zone.

    This implies an occurrence rate of approximately one Earth-like planet per 300 sun-like stars.

    astrobiology.com/2025/03/resea

  19. A new NASA/ESA/CSA James Webb Space Telescope Picture of the Month presents HH 30 in unprecedented resolution: esawebb.org/images/potm2501a/ - it is an edge-on #protoplanetary disc that is surrounded by jets and a disc wind, and is located in the dark cloud LDN 1551 in the Taurus Molecular Cloud.

  20. A new NASA/ESA/CSA James Webb Space Telescope Picture of the Month presents HH 30 in unprecedented resolution: esawebb.org/images/potm2501a/ - it is an edge-on #protoplanetary disc that is surrounded by jets and a disc wind, and is located in the dark cloud LDN 1551 in the Taurus Molecular Cloud.

  21. High-resolution #ALMA Observations of Richly Structured #Protoplanetary Disks in σ Orionis: iopscience.iop.org/article/10. -> Research Collaboration Shows That #Planets Can Form Under Harsh Radiation: news.columbia.edu/news/columbi - a team of astronomers including professor Jane Huang have shown that extreme astrophysical environments can foster new planets.

  22. High-resolution #ALMA Observations of Richly Structured #Protoplanetary Disks in σ Orionis: iopscience.iop.org/article/10. -> Research Collaboration Shows That #Planets Can Form Under Harsh Radiation: news.columbia.edu/news/columbi - a team of astronomers including professor Jane Huang have shown that extreme astrophysical environments can foster new planets.

  23. Photoevaporation and Close Encounters - How the Environment around Cygnus OB2 Affects the Evolution of #Protoplanetary Disks / Diffuse X-Ray Emission in the Cygnus OB2 Association: iopscience.iop.org/article/10. / iopscience.iop.org/article/10. -> Planets Beware - NASA Unburies Danger Zones of Star Cluster: chandra.si.edu/photo/2024/cygo

  24. Photoevaporation and Close Encounters - How the Environment around Cygnus OB2 Affects the Evolution of #Protoplanetary Disks / Diffuse X-Ray Emission in the Cygnus OB2 Association: iopscience.iop.org/article/10. / iopscience.iop.org/article/10. -> Planets Beware - NASA Unburies Danger Zones of Star Cluster: chandra.si.edu/photo/2024/cygo

  25. Astronomers have made a breakthrough in revealing how #planets are made.

    By observing water vapor in #protoplanetary disks, #JWST observations have confirmed a physical process involving the drifting of ice-coated solids from the outer regions of the disk into the rocky-planet zone.

    Theories have long proposed that icy pebbles forming in the cold, outer disk regions should be the fundamental seeds of #planet formation.

    #astronomy #exoplanets
    astrobiology.com/2023/11/webb-

  26. Astronomers have made a breakthrough in revealing how #planets are made.

    By observing water vapor in #protoplanetary disks, #JWST observations have confirmed a physical process involving the drifting of ice-coated solids from the outer regions of the disk into the rocky-planet zone.

    Theories have long proposed that icy pebbles forming in the cold, outer disk regions should be the fundamental seeds of #planet formation.

    #astronomy #exoplanets
    astrobiology.com/2023/11/webb-

  27. Solving the mystery of how #planets like Earth form is an important question for understanding the origin of life.

    Planets are thought to form when interstellar dust and gas collect in a #protoplanetary disk surrounding a #protostar, but it has been unclear how #planet formation begins.

    By observing protoplanetary disks without dark rings, astronomers can study systems where giant planets have not yet formed.

    phys.org/news/2023-10-astronom

    Paper by Ohashi et al. (2023):
    iopscience.iop.org/article/10.

  28. Solving the mystery of how #planets like Earth form is an important question for understanding the origin of life.

    Planets are thought to form when interstellar dust and gas collect in a #protoplanetary disk surrounding a #protostar, but it has been unclear how #planet formation begins.

    By observing protoplanetary disks without dark rings, astronomers can study systems where giant planets have not yet formed.

    phys.org/news/2023-10-astronom

    Paper by Ohashi et al. (2023):
    iopscience.iop.org/article/10.

  29. Solving the mystery of how #planets like Earth were formed is an important question for understanding the origin of life. Planets are thought to form when #interstellar dust and gas collect in a #protoplanetary disk surrounding a #protostar, but it has been unclear where, when, or how planet formation begins.
    #Astronomy #SpaceScience #sflorg
    sflorg.com/2023/10/astr1006230

  30. Solving the mystery of how #planets like Earth were formed is an important question for understanding the origin of life. Planets are thought to form when #interstellar dust and gas collect in a #protoplanetary disk surrounding a #protostar, but it has been unclear where, when, or how planet formation begins.
    #Astronomy #SpaceScience #sflorg
    sflorg.com/2023/10/astr1006230

  31. A rich hydrocarbon chemistry and high C to O ratio in the inner disk around a very low-mass star / JWST/MIRI Spectroscopy of the Disk of the Young Eruptive Star EX Lup in Quiescence / MINDS - the detection of 13CO2 with JWST-MIRI indicates abundant CO2 in a #protoplanetary disk: arxiv.org/abs/2304.05954 / arxiv.org/abs/2301.08770 / arxiv.org/abs/2212.08047 -> #JWST peeks into the birthplaces of #exoplanets - a rich and diverse chemistry: mpia.de/news/science/2023-05-j

  32. A rich hydrocarbon chemistry and high C to O ratio in the inner disk around a very low-mass star / JWST/MIRI Spectroscopy of the Disk of the Young Eruptive Star EX Lup in Quiescence / MINDS - the detection of 13CO2 with JWST-MIRI indicates abundant CO2 in a #protoplanetary disk: arxiv.org/abs/2304.05954 / arxiv.org/abs/2301.08770 / arxiv.org/abs/2212.08047 -> #JWST peeks into the birthplaces of #exoplanets - a rich and diverse chemistry: mpia.de/news/science/2023-05-j

  33. Discovery of Line Pressure Broadening and Direct Constraint on Gas Surface Density in a #Protoplanetary Disk: iopscience.iop.org/article/10. -> Model-Independent Method to Weigh Protoplanetary Disks: nao.ac.jp/en/news/science/2023

  34. Discovery of Line Pressure Broadening and Direct Constraint on Gas Surface Density in a #Protoplanetary Disk: iopscience.iop.org/article/10. -> Model-Independent Method to Weigh Protoplanetary Disks: nao.ac.jp/en/news/science/2023

  35. Emergence of vortices at the edges of planet-driven gaps in #protoplanetary discs: academic.oup.com/mnras/article / Vortex weighing and dating of planets in protoplanetary discs: arxiv.org/abs/2301.01789 -> Astronomers use ‘little hurricanes’ to weigh and date planets around young stars: cam.ac.uk/research/news/astron