\n\t\t\t\t\t\t\t\tWebb Study Reveals Rocky Planets Can Form in Extreme Environments\t\t\t\t\t\t\t<\/h1>\n<\/p><\/div>\n<\/p><\/div>\n<\/div>\n<\/div>\n![\"The](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/11\/stsci-01hfq5yxz04pf608hqb0krtf3s.jpg?w=1280\")
<\/figure>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\n\n\n\t\t\t\t\t\t\t<\/div>\n<\/p><\/div>\n<\/p><\/div>\nAn international team of astronomers has used NASA\u2019s James Webb Space Telescope to provide the first observation of water and other molecules in the highly irradiated inner, rocky-planet-forming regions of a disk in one of the most extreme environments in our galaxy. These results suggest that the conditions for terrestrial planet formation can occur in a possible broader range of environments than previously thought.\u00a0<\/p>\n
Image: Protoplanetary Disk (Artist Concept)<\/h2>\n\n\n\n<\/figure>\nThis is an artist\u2019s impression of a young star surrounded by a protoplanetary disk in which planets are forming. <\/div>\nESO\/L. Cal\u00e7ada<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nThese are the first results from the eXtreme Ultraviolet Environments (XUE) James Webb Space Telescope program, which focuses on the characterization of planet-forming disks (vast, spinning clouds of gas, dust, and chunks of rock where planets form and evolve) in massive star-forming regions. These regions are likely representative of the environment in which most planetary systems formed. Understanding the impact of environment on planet formation is important for scientists to gain insights into the diversity of the different types of exoplanets.<\/p>\n
The XUE program targets a total of 15 disks in three areas of the Lobster Nebula (also known as NGC 6357), a large emission nebula roughly 5,500 light-years away from Earth in the constellation Scorpius. The Lobster Nebula is one of the youngest and closest massive star-formation complexes, and is host to some of the most massive stars in our galaxy. Massive stars are hotter, and therefore emit more ultraviolet (UV) radiation. This can disperse the gas, making the expected disk lifetime as short as a million years. Thanks to Webb, astronomers can now study the effect of UV radiation on the inner rocky-planet forming regions of protoplanetary disks around stars like our Sun.<\/p>\n
\u201cWebb is the only telescope with the spatial resolution and sensitivity to study planet-forming disks in massive star-forming regions,\u201d said team lead Mar\u00eda Claudia Ram\u00edrez-Tannus of the Max Planck Institute for Astronomy in Germany.<\/p>\n
Astronomers aim to characterize the physical properties and chemical composition of the rocky-planet-forming regions of disks in the Lobster Nebula using the Medium Resolution Spectrometer on Webb\u2019s Mid-Infrared Instrument (MIRI<\/a>). This first result focuses on the protoplanetary disk termed XUE 1, which is located in the star cluster Pismis 24.<\/p>\n\u201cOnly the MIRI wavelength range and spectral resolution allow us to probe the molecular inventory and physical conditions of the warm gas and dust where rocky planets form,\u201d added team member Arjan Bik of Stockholm University in Sweden.<\/p>\n
Image: XUE 1 spectrum detects water<\/h2>\n\n\n\n![\"Graphic](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/11\/stsci-01hfpt6zchm0y1jphbk8d4hs62.jpg?w=1280\")
<\/figure>\nThis spectrum shows data from the protoplanetary disk termed XUE 1, which is located in the star cluster Pismis 24. The inner disk around XUE 1 revealed signatures of water (highlighted here in blue), as well as acetylene (C2H2, green), hydrogen cyanide (HCN, brown), and carbon dioxide (CO2, red). As indicated, some of the emission detected was weaker than some of the predicted models, which might imply a small outer disk radius.<\/div>\nNASA, ESA, CSA, M. Ram\u00edrez-Tannus (Max Planck Institute for Astronomy), J. Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nDue to its location near several massive stars in NGC 6357, scientists expect XUE 1 to have been constantly exposed to high amounts of ultraviolet radiation throughout its life. However, in this extreme environment the team still detected a range of molecules that are the building blocks for rocky planets.<\/p>\n
\u201cWe find that the inner disk around XUE 1 is remarkably similar to those in nearby star-forming regions,\u201d said team member Rens Waters of Radboud University in the Netherlands. \u201cWe\u2019ve detected water and other molecules like carbon monoxide, carbon dioxide, hydrogen cyanide, and acetylene. However, the emission found was weaker than some models predicted. This might imply a small outer disk radius.\u201d<\/p>\n
\u201cWe were surprised and excited because this is the first time that these molecules have been detected under these extreme conditions,\u201d added Lars Cuijpers of Radboud University. The team also found small, partially crystalline silicate dust at the disk\u2019s surface. This is considered to be the building blocks of rocky planets.\u00a0<\/p>\n
These results are good news for rocky planet formation, as the science team finds that the conditions in the inner disk resemble those found in the well-studied disks located in nearby star-forming regions, where only low-mass stars form. This suggests that rocky planets can form in a much broader range of environments than previously believed.<\/p>\n
Image: XUE 1 Spectrum detects CO<\/h2>\n\n\n\n![\"Graphic](\"https:\/\/www.nasa.gov\/wp-content\/uploads\/2023\/11\/stsci-01hfptk93qpatd1q966xda0xcs.jpg?w=1280\")
<\/figure>\nThis spectrum shows data from the protoplanetary disk termed XUE 1, which is located in the star cluster Pismis 24. It features the observed signatures of carbon monoxide spanning 4.95 to 5.15 microns. <\/div>\nNASA, ESA, CSA, M. Ram\u00edrez-Tannus (Max Planck Institute for Astronomy), J. Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nThe team notes that the remaining observations from the XUE program are crucial to establish the commonality of these conditions.<\/p>\n
\u201cXUE 1 shows us that the conditions to form rocky planets are there, so the next step is to check how common that is,\u201d said Ram\u00edrez-Tannus. \u201cWe will observe other disks in the same region to determine the frequency with which these conditions can be observed.\u201d<\/p>\n
These results have been published <\/a>in The Astrophysical Journal<\/em>.<\/p>\nThe James Webb Space Telescope is the world\u2019s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.<\/em><\/p>\nMedia Contacts<\/h2>\n
Laura\u00a0Betz<\/strong> \u2013 laura.e.betz@nasa.gov<\/a>, Rob Gutro<\/strong>\u2013 rob.gutro@nasa.gov<\/a>
NASA\u2019s \u00a0Goddard Space Flight Center<\/em><\/a>,\u00a0<\/em>, Greenbelt, Md.<\/p>\nBethany Downer \u2013 \u00a0<\/strong>Bethany.Downer@esawebb.org<\/a>
<\/strong>ESA\/Webb Chief Science Communications Officer<\/p>\nChristine Pulliam<\/strong> cpulliam@stsci.edu<\/a>
Space Telescope Science Institute, Baltimore, Md.<\/p>\n<\/p>\nDownloads<\/h2>\n
Download full resolution images for this article<\/a><\/strong> from the Space Telescope Science Institute.<\/p>\nResearch results published<\/a> <\/strong>in The Astrophysical Journal<\/em>.<\/p>\n<\/p>\nRelated Information<\/h2>\n
Terrestrial Exoplanets<\/a><\/strong><\/p>\nExoplanets 101<\/a><\/strong><\/p>\nLIfe and Death of a Planetary System<\/a><\/strong><\/p>\nWebb Mission<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/<\/p>\nWebb News<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/latestnews\/<\/p>\nWebb Images<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/multimedia\/images\/<\/p>\n<\/p>\nRelated For Kids<\/h2>\n
What is a Planet?<\/a><\/strong><\/p>\nWhat is an Exoplanet?<\/a><\/strong><\/p>\nHow Many Solar Systems are in our Galaxy?<\/a><\/strong><\/p>\nWhat Is a Galaxy?<\/strong><\/a><\/p>\nWhat is the Webb Telescope?<\/strong><\/a><\/p>\nSpacePlace for Kids<\/strong><\/a><\/p>\nEn Espa\u00f1ol<\/h2>\n
Ciencia de la NASA<\/strong><\/a><\/p>\nNASA en espa\u00f1ol\u00a0<\/strong><\/a><\/p>\nSpace Place\u00a0para ni\u00f1os<\/strong><\/a><\/p>\n\n\n\n\nKeep Exploring<\/div>\nRelated Topics<\/h2>\n<\/p><\/div>\n<\/p><\/div>\n\n\t\t\t\t\t<\/p>\n\n
<\/figure>\n<\/p><\/div>\n<\/p><\/div>\n<\/p><\/div>\nAn international team of astronomers has used NASA\u2019s James Webb Space Telescope to provide the first observation of water and other molecules in the highly irradiated inner, rocky-planet-forming regions of a disk in one of the most extreme environments in our galaxy. These results suggest that the conditions for terrestrial planet formation can occur in a possible broader range of environments than previously thought.\u00a0<\/p>\n
Image: Protoplanetary Disk (Artist Concept)<\/h2>\n\n\n\n<\/figure>\nThis is an artist\u2019s impression of a young star surrounded by a protoplanetary disk in which planets are forming. <\/div>\nESO\/L. Cal\u00e7ada<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nThese are the first results from the eXtreme Ultraviolet Environments (XUE) James Webb Space Telescope program, which focuses on the characterization of planet-forming disks (vast, spinning clouds of gas, dust, and chunks of rock where planets form and evolve) in massive star-forming regions. These regions are likely representative of the environment in which most planetary systems formed. Understanding the impact of environment on planet formation is important for scientists to gain insights into the diversity of the different types of exoplanets.<\/p>\n
The XUE program targets a total of 15 disks in three areas of the Lobster Nebula (also known as NGC 6357), a large emission nebula roughly 5,500 light-years away from Earth in the constellation Scorpius. The Lobster Nebula is one of the youngest and closest massive star-formation complexes, and is host to some of the most massive stars in our galaxy. Massive stars are hotter, and therefore emit more ultraviolet (UV) radiation. This can disperse the gas, making the expected disk lifetime as short as a million years. Thanks to Webb, astronomers can now study the effect of UV radiation on the inner rocky-planet forming regions of protoplanetary disks around stars like our Sun.<\/p>\n
\u201cWebb is the only telescope with the spatial resolution and sensitivity to study planet-forming disks in massive star-forming regions,\u201d said team lead Mar\u00eda Claudia Ram\u00edrez-Tannus of the Max Planck Institute for Astronomy in Germany.<\/p>\n
Astronomers aim to characterize the physical properties and chemical composition of the rocky-planet-forming regions of disks in the Lobster Nebula using the Medium Resolution Spectrometer on Webb\u2019s Mid-Infrared Instrument (MIRI<\/a>). This first result focuses on the protoplanetary disk termed XUE 1, which is located in the star cluster Pismis 24.<\/p>\n\u201cOnly the MIRI wavelength range and spectral resolution allow us to probe the molecular inventory and physical conditions of the warm gas and dust where rocky planets form,\u201d added team member Arjan Bik of Stockholm University in Sweden.<\/p>\n
Image: XUE 1 spectrum detects water<\/h2>\n\n\n\n<\/figure>\nThis spectrum shows data from the protoplanetary disk termed XUE 1, which is located in the star cluster Pismis 24. The inner disk around XUE 1 revealed signatures of water (highlighted here in blue), as well as acetylene (C2H2, green), hydrogen cyanide (HCN, brown), and carbon dioxide (CO2, red). As indicated, some of the emission detected was weaker than some of the predicted models, which might imply a small outer disk radius.<\/div>\nNASA, ESA, CSA, M. Ram\u00edrez-Tannus (Max Planck Institute for Astronomy), J. Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nDue to its location near several massive stars in NGC 6357, scientists expect XUE 1 to have been constantly exposed to high amounts of ultraviolet radiation throughout its life. However, in this extreme environment the team still detected a range of molecules that are the building blocks for rocky planets.<\/p>\n
\u201cWe find that the inner disk around XUE 1 is remarkably similar to those in nearby star-forming regions,\u201d said team member Rens Waters of Radboud University in the Netherlands. \u201cWe\u2019ve detected water and other molecules like carbon monoxide, carbon dioxide, hydrogen cyanide, and acetylene. However, the emission found was weaker than some models predicted. This might imply a small outer disk radius.\u201d<\/p>\n
\u201cWe were surprised and excited because this is the first time that these molecules have been detected under these extreme conditions,\u201d added Lars Cuijpers of Radboud University. The team also found small, partially crystalline silicate dust at the disk\u2019s surface. This is considered to be the building blocks of rocky planets.\u00a0<\/p>\n
These results are good news for rocky planet formation, as the science team finds that the conditions in the inner disk resemble those found in the well-studied disks located in nearby star-forming regions, where only low-mass stars form. This suggests that rocky planets can form in a much broader range of environments than previously believed.<\/p>\n
Image: XUE 1 Spectrum detects CO<\/h2>\n\n\n\n<\/figure>\nThis spectrum shows data from the protoplanetary disk termed XUE 1, which is located in the star cluster Pismis 24. It features the observed signatures of carbon monoxide spanning 4.95 to 5.15 microns. <\/div>\nNASA, ESA, CSA, M. Ram\u00edrez-Tannus (Max Planck Institute for Astronomy), J. Olmsted (STScI)<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\nThe team notes that the remaining observations from the XUE program are crucial to establish the commonality of these conditions.<\/p>\n
\u201cXUE 1 shows us that the conditions to form rocky planets are there, so the next step is to check how common that is,\u201d said Ram\u00edrez-Tannus. \u201cWe will observe other disks in the same region to determine the frequency with which these conditions can be observed.\u201d<\/p>\n
These results have been published <\/a>in The Astrophysical Journal<\/em>.<\/p>\nThe James Webb Space Telescope is the world\u2019s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.<\/em><\/p>\nMedia Contacts<\/h2>\n
Laura\u00a0Betz<\/strong> \u2013 laura.e.betz@nasa.gov<\/a>, Rob Gutro<\/strong>\u2013 rob.gutro@nasa.gov<\/a>
NASA\u2019s \u00a0Goddard Space Flight Center<\/em><\/a>,\u00a0<\/em>, Greenbelt, Md.<\/p>\nBethany Downer \u2013 \u00a0<\/strong>Bethany.Downer@esawebb.org<\/a>
<\/strong>ESA\/Webb Chief Science Communications Officer<\/p>\nChristine Pulliam<\/strong> cpulliam@stsci.edu<\/a>
Space Telescope Science Institute, Baltimore, Md.<\/p>\n<\/p>\nDownloads<\/h2>\n
Download full resolution images for this article<\/a><\/strong> from the Space Telescope Science Institute.<\/p>\nResearch results published<\/a> <\/strong>in The Astrophysical Journal<\/em>.<\/p>\n<\/p>\nRelated Information<\/h2>\n
Terrestrial Exoplanets<\/a><\/strong><\/p>\nExoplanets 101<\/a><\/strong><\/p>\nLIfe and Death of a Planetary System<\/a><\/strong><\/p>\nWebb Mission<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/<\/p>\nWebb News<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/latestnews\/<\/p>\nWebb Images<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/multimedia\/images\/<\/p>\n<\/p>\nRelated For Kids<\/h2>\n
What is a Planet?<\/a><\/strong><\/p>\nWhat is an Exoplanet?<\/a><\/strong><\/p>\nHow Many Solar Systems are in our Galaxy?<\/a><\/strong><\/p>\nWhat Is a Galaxy?<\/strong><\/a><\/p>\nWhat is the Webb Telescope?<\/strong><\/a><\/p>\nSpacePlace for Kids<\/strong><\/a><\/p>\nEn Espa\u00f1ol<\/h2>\n
Ciencia de la NASA<\/strong><\/a><\/p>\nNASA en espa\u00f1ol\u00a0<\/strong><\/a><\/p>\nSpace Place\u00a0para ni\u00f1os<\/strong><\/a><\/p>\n\n\n\n\nKeep Exploring<\/div>\nRelated Topics<\/h2>\n<\/p><\/div>\n<\/p><\/div>\n\n\t\t\t\t\t<\/p>\n\n
<\/figure>These are the first results from the eXtreme Ultraviolet Environments (XUE) James Webb Space Telescope program, which focuses on the characterization of planet-forming disks (vast, spinning clouds of gas, dust, and chunks of rock where planets form and evolve) in massive star-forming regions. These regions are likely representative of the environment in which most planetary systems formed. Understanding the impact of environment on planet formation is important for scientists to gain insights into the diversity of the different types of exoplanets.<\/p>\n
The XUE program targets a total of 15 disks in three areas of the Lobster Nebula (also known as NGC 6357), a large emission nebula roughly 5,500 light-years away from Earth in the constellation Scorpius. The Lobster Nebula is one of the youngest and closest massive star-formation complexes, and is host to some of the most massive stars in our galaxy. Massive stars are hotter, and therefore emit more ultraviolet (UV) radiation. This can disperse the gas, making the expected disk lifetime as short as a million years. Thanks to Webb, astronomers can now study the effect of UV radiation on the inner rocky-planet forming regions of protoplanetary disks around stars like our Sun.<\/p>\n
\u201cWebb is the only telescope with the spatial resolution and sensitivity to study planet-forming disks in massive star-forming regions,\u201d said team lead Mar\u00eda Claudia Ram\u00edrez-Tannus of the Max Planck Institute for Astronomy in Germany.<\/p>\n
Astronomers aim to characterize the physical properties and chemical composition of the rocky-planet-forming regions of disks in the Lobster Nebula using the Medium Resolution Spectrometer on Webb\u2019s Mid-Infrared Instrument (MIRI<\/a>). This first result focuses on the protoplanetary disk termed XUE 1, which is located in the star cluster Pismis 24.<\/p>\n \u201cOnly the MIRI wavelength range and spectral resolution allow us to probe the molecular inventory and physical conditions of the warm gas and dust where rocky planets form,\u201d added team member Arjan Bik of Stockholm University in Sweden.<\/p>\n Due to its location near several massive stars in NGC 6357, scientists expect XUE 1 to have been constantly exposed to high amounts of ultraviolet radiation throughout its life. However, in this extreme environment the team still detected a range of molecules that are the building blocks for rocky planets.<\/p>\n \u201cWe find that the inner disk around XUE 1 is remarkably similar to those in nearby star-forming regions,\u201d said team member Rens Waters of Radboud University in the Netherlands. \u201cWe\u2019ve detected water and other molecules like carbon monoxide, carbon dioxide, hydrogen cyanide, and acetylene. However, the emission found was weaker than some models predicted. This might imply a small outer disk radius.\u201d<\/p>\n \u201cWe were surprised and excited because this is the first time that these molecules have been detected under these extreme conditions,\u201d added Lars Cuijpers of Radboud University. The team also found small, partially crystalline silicate dust at the disk\u2019s surface. This is considered to be the building blocks of rocky planets.\u00a0<\/p>\n These results are good news for rocky planet formation, as the science team finds that the conditions in the inner disk resemble those found in the well-studied disks located in nearby star-forming regions, where only low-mass stars form. This suggests that rocky planets can form in a much broader range of environments than previously believed.<\/p>\n The team notes that the remaining observations from the XUE program are crucial to establish the commonality of these conditions.<\/p>\n \u201cXUE 1 shows us that the conditions to form rocky planets are there, so the next step is to check how common that is,\u201d said Ram\u00edrez-Tannus. \u201cWe will observe other disks in the same region to determine the frequency with which these conditions can be observed.\u201d<\/p>\n These results have been published <\/a>in The Astrophysical Journal<\/em>.<\/p>\n The James Webb Space Telescope is the world\u2019s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.<\/em><\/p>\n Laura\u00a0Betz<\/strong> \u2013 laura.e.betz@nasa.gov<\/a>, Rob Gutro<\/strong>\u2013 rob.gutro@nasa.gov<\/a> Bethany Downer \u2013 \u00a0<\/strong>Bethany.Downer@esawebb.org<\/a> Christine Pulliam<\/strong> cpulliam@stsci.edu<\/a> Download full resolution images for this article<\/a><\/strong> from the Space Telescope Science Institute.<\/p>\n Research results published<\/a> <\/strong>in The Astrophysical Journal<\/em>.<\/p>\n<\/p>\n Terrestrial Exoplanets<\/a><\/strong><\/p>\n Exoplanets 101<\/a><\/strong><\/p>\n LIfe and Death of a Planetary System<\/a><\/strong><\/p>\n Webb Mission<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/<\/p>\n Webb News<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/latestnews\/<\/p>\n Webb Images<\/a><\/strong> \u2013 https:\/\/science.nasa.gov\/mission\/webb\/multimedia\/images\/<\/p>\n<\/p>\n What is a Planet?<\/a><\/strong><\/p>\n What is an Exoplanet?<\/a><\/strong><\/p>\n How Many Solar Systems are in our Galaxy?<\/a><\/strong><\/p>\n What Is a Galaxy?<\/strong><\/a><\/p>\n What is the Webb Telescope?<\/strong><\/a><\/p>\n SpacePlace for Kids<\/strong><\/a><\/p>\n Ciencia de la NASA<\/strong><\/a><\/p>\n NASA en espa\u00f1ol\u00a0<\/strong><\/a><\/p>\n Space Place\u00a0para ni\u00f1os<\/strong><\/a><\/p>\nImage: XUE 1 spectrum detects water<\/h2>\n
<\/figure>Image: XUE 1 Spectrum detects CO<\/h2>\n
<\/figure>Media Contacts<\/h2>\n
NASA\u2019s \u00a0Goddard Space Flight Center<\/em><\/a>,\u00a0<\/em>, Greenbelt, Md.<\/p>\n
<\/strong>ESA\/Webb Chief Science Communications Officer<\/p>\n
Space Telescope Science Institute, Baltimore, Md.<\/p>\n<\/p>\nDownloads<\/h2>\n
Related Information<\/h2>\n
Related For Kids<\/h2>\n
En Espa\u00f1ol<\/h2>\n
Related Topics<\/h2>\n<\/p><\/div>\n<\/p><\/div>\n