This is a
featured picture, which means that
members of the community have identified it as one of the finest images on the English Wikipedia, adding significantly to its accompanying article. If you have a different image of similar quality, be sure to
upload it using the proper
free license tag,
add it to a relevant article, and
nominate it.
العربية: العُنقُود النجمي
پيسميس 24-1 الواقع في مركز
السديم الإشعاعيNGC 6357 المُمتد لِدرجوٍ واحدةٍ في السماء باتجاه
كوكبة العقرب. جُزءٌ من هذا السديم
مُتأيِّن بسبب أصغر النُجُوم (الأشد ازرقاقًا) وأثقلها في آن، الكامنة في پيسميس 24.
الأشعة فوق البنفسجيَّة المُنبعثة بِشدَّةٍ من النُجُوم المُشتعلة تُسخِّنُ الغازات المُحيطة بِالعُنقُود فيتولَّد عن هذا فُقاعة ضمن سديم NGC 6357. وُجُود سُحب الغازات المُحيطة هذه يجعل خوض غمار هذه المنطقة أكثر صُعُوبة.
English: The star cluster
Pismis 24 lies in the core of the large
emission nebulaNGC 6357 that extends one degree on the sky in the direction of the
Scorpius constellation. Part of the nebula is
ionised by the youngest (bluest) heavy stars in Pismis 24. The intense
ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
Español: El cúmulo estelar
Pismis 24 se encuentra en el núcleo de la gran
nebulosa de emisiónNGC 6357 que se extiende en el cielo un grado en dirección a la
constelación Scorpius. Parte de la nebulosa es ionizada por las estrellas pesadas más jóvenes (más azules) en Pismis 24. La intensa radiación ultravioleta de las estrellas ardientes calienta el gas que rodea el cúmulo y crea una burbuja en NGC 6357. La presencia de estas nubes de gas circundantes hace aún más difícil la exploración de la región.
Polski: Gromada gwazdPismis 24 położona w centrum ogromnej
mgławicy emisyjnejNGC 6357, która na niebie rozciąga się na jeden stopień w kierunku
gwiazdozbioru Skorpiona. Część mgławicy jest
zjonizowana przez najmłodsze (najbardziej niebieskie) ciężkie
gwiazdy z gromady Pismis 24. Intensywne
promieniowanie ultrafioletowe z płonących gwiazd podgrzewa gaz otaczajacy gromadę i tworzy „bąbel” w mgławicy NGC 6357. Obecność tych chmur gazu sprawia, że badanie tego obszaru jest jeszcze trudniejsze.
Italiano: L'
ammasso stellare Pismis 24 nel nucleo della
nebulosa a emissioneNGC 6357. Parte della nebulosa è ionizzata dalle giovani stelle blu in Pismis 24. L'intensa
radiazione ultravioletta dalle stelle infuocate scalda i gas che circondano l'ammasso e creano una bolla in NGC 6357. La presenza di questa nuvola di gas rende l'osservazione della regione ancora più difficile.
한국어: 피스미스 24 성단은
전갈자리 방향의 각도 1도에 펼쳐져 있는 거대한
발광성운NGC 6357의 중심부에 위치한다. 성운의 일부는 피스미스 24 내부의 가장 젊은 (가장 푸른) 무거운 별에 의해
이온화되었다. 이글거리는 별이 내뿜는 강한
자외선 복사가 성단을 둘러싼 기체를 가열하여 NGC 6357의 거품을 만든다. 이러한 주위의 기체 구름의 존재는 해당 부분의 면밀한 조사를 더욱 어렵게 한다.
Português: Pismis 24-1, uma parte de um aglomerado aberto localizado no núcleo da grande
nebulosa de emissãoNGC 6357, que se estende no céu um grau em direção à
constelação Scorpius. Parte da nebulosa é ionizada pelas estrelas massivas mais jovens (mais azuis) em Pismis 24-1. A intensa radiação ultravioleta das estrelas ardentes aquece o gás que envolve o aglomerado e cria uma bolha na NGC 6357.
NASA, ESA and Jesœs Maz Apellÿniz (Instituto de astrofsica de Andaluca, Spain). Acknowledgement: Davide De Martin (ESA/Hubble)
Licensing
Public domainPublic domainfalsefalse
This file is in the public domain because it was created by
NASA and
ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre.
Copyright statement at hubblesite.org or
2008 copyright statement at spacetelescope.org. For material created by the
European Space Agency on the spacetelescope.org site since 2009, use the
{{ESA-Hubble}} tag.
English: The star cluster
Pismis 24 lies in the core of the large
emission nebulaNGC 6357 that extends one degree on the sky in the direction of the
Scorpius constellation. Part of the nebula is
ionised by the youngest (bluest) heavy stars in Pismis 24. The intense
ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
English: The star cluster
Pismis 24 lies in the core of the large
emission nebulaNGC 6357 that extends one degree on the sky in the direction of the
Scorpius constellation. Part of the nebula is
ionised by the youngest (bluest) heavy stars in Pismis 24. The intense
ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
Español: El cúmulo estelar
Pismis 24 se encuentra en el núcleo de la gran
nebulosa de emisiónNGC 6357 que se extiende en el cielo un grado en dirección a la
constelación Scorpius. Parte de la nebulosa es ionizada por las estrellas pesadas más jóvenes (más azules) en Pismis 24. La intensa radiación ultravioleta de las estrellas ardientes calienta el gas que rodea el cúmulo y crea una burbuja en NGC 6357. La presencia de estas nubes de gas circundantes hace aún más difícil la exploración de la región.
Italiano: L'
ammasso stellare Pismis 24 nel nucleo della
nebulosa a emissioneNGC 6357. Parte della nebulosa è ionizzata dalle giovani stelle blu in Pismis 24. L'intensa
radiazione ultravioletta dalle stelle infuocate scalda i gas che circondano l'ammasso e creano una bolla in NGC 6357. La presenza di questa nuvola di gas rende l'osservazione della regione ancora più difficile.
Polski: Gromada gwazdPismis 24 położona w centrum ogromnej
mgławicy emisyjnejNGC 6357, która na niebie rozciąga się na jeden stopień w kierunku
gwiazdozbioru Skorpiona. Część mgławicy jest
zjonizowana przez najmłodsze (najbardziej niebieskie) ciężkie
gwiazdy z gromady Pismis 24. Intensywne
promieniowanie ultrafioletowe z płonących gwiazd podgrzewa gaz otaczajacy gromadę i tworzy „bąbel” w mgławicy NGC 6357. Obecność tych chmur gazu sprawia, że badanie tego obszaru jest jeszcze trudniejsze.
Português: Pismis 24-1, uma parte de um aglomerado aberto localizado no núcleo da grande
nebulosa de emissãoNGC 6357, que se estende no céu um grau em direção à
constelação Scorpius. Parte da nebulosa é ionizada pelas estrelas massivas mais jovens (mais azuis) em Pismis 24-1. A intensa radiação ultravioleta das estrelas ardentes aquece o gás que envolve o aglomerado e cria uma bolha na NGC 6357.
한국어: 피스미스 24 성단은
전갈자리 방향의 각도 1도에 펼쳐져 있는 거대한
발광성운NGC 6357의 중심부에 위치한다. 성운의 일부는 피스미스 24 내부의 가장 젊은 (가장 푸른) 무거운 별에 의해
이온화되었다. 이글거리는 별이 내뿜는 강한
자외선 복사가 성단을 둘러싼 기체를 가열하여 NGC 6357의 거품을 만든다. 이러한 주위의 기체 구름의 존재는 해당 부분의 면밀한 조사를 더욱 어렵게 한다.
This is a featured picture on Wikimedia Commons (
Featured pictures) and is considered one of the finest images. See its nomination
here. This is a featured picture on the Arabic language Wikipedia (
صور مختارة) and is considered one of the finest images. See its nomination
here. This is a featured picture on the English language Wikipedia (
Featured pictures) and is considered one of the finest images. See its nomination
here.
{{Information |Description= An
emissionw:nebula, NGC 6357, is on the left. The star Pismis 24-1 (the brightest one) is located to the right of the nubula. |Source= [http://antwrp.gsfc.nasa.gov/apod/image/0612/ngc6357a_hst_big.j
File usage
The following pages on the English Wikipedia use this file (pages on other projects are not listed):
This is a
featured picture, which means that
members of the community have identified it as one of the finest images on the English Wikipedia, adding significantly to its accompanying article. If you have a different image of similar quality, be sure to
upload it using the proper
free license tag,
add it to a relevant article, and
nominate it.
العربية: العُنقُود النجمي
پيسميس 24-1 الواقع في مركز
السديم الإشعاعيNGC 6357 المُمتد لِدرجوٍ واحدةٍ في السماء باتجاه
كوكبة العقرب. جُزءٌ من هذا السديم
مُتأيِّن بسبب أصغر النُجُوم (الأشد ازرقاقًا) وأثقلها في آن، الكامنة في پيسميس 24.
الأشعة فوق البنفسجيَّة المُنبعثة بِشدَّةٍ من النُجُوم المُشتعلة تُسخِّنُ الغازات المُحيطة بِالعُنقُود فيتولَّد عن هذا فُقاعة ضمن سديم NGC 6357. وُجُود سُحب الغازات المُحيطة هذه يجعل خوض غمار هذه المنطقة أكثر صُعُوبة.
English: The star cluster
Pismis 24 lies in the core of the large
emission nebulaNGC 6357 that extends one degree on the sky in the direction of the
Scorpius constellation. Part of the nebula is
ionised by the youngest (bluest) heavy stars in Pismis 24. The intense
ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
Español: El cúmulo estelar
Pismis 24 se encuentra en el núcleo de la gran
nebulosa de emisiónNGC 6357 que se extiende en el cielo un grado en dirección a la
constelación Scorpius. Parte de la nebulosa es ionizada por las estrellas pesadas más jóvenes (más azules) en Pismis 24. La intensa radiación ultravioleta de las estrellas ardientes calienta el gas que rodea el cúmulo y crea una burbuja en NGC 6357. La presencia de estas nubes de gas circundantes hace aún más difícil la exploración de la región.
Polski: Gromada gwazdPismis 24 położona w centrum ogromnej
mgławicy emisyjnejNGC 6357, która na niebie rozciąga się na jeden stopień w kierunku
gwiazdozbioru Skorpiona. Część mgławicy jest
zjonizowana przez najmłodsze (najbardziej niebieskie) ciężkie
gwiazdy z gromady Pismis 24. Intensywne
promieniowanie ultrafioletowe z płonących gwiazd podgrzewa gaz otaczajacy gromadę i tworzy „bąbel” w mgławicy NGC 6357. Obecność tych chmur gazu sprawia, że badanie tego obszaru jest jeszcze trudniejsze.
Italiano: L'
ammasso stellare Pismis 24 nel nucleo della
nebulosa a emissioneNGC 6357. Parte della nebulosa è ionizzata dalle giovani stelle blu in Pismis 24. L'intensa
radiazione ultravioletta dalle stelle infuocate scalda i gas che circondano l'ammasso e creano una bolla in NGC 6357. La presenza di questa nuvola di gas rende l'osservazione della regione ancora più difficile.
한국어: 피스미스 24 성단은
전갈자리 방향의 각도 1도에 펼쳐져 있는 거대한
발광성운NGC 6357의 중심부에 위치한다. 성운의 일부는 피스미스 24 내부의 가장 젊은 (가장 푸른) 무거운 별에 의해
이온화되었다. 이글거리는 별이 내뿜는 강한
자외선 복사가 성단을 둘러싼 기체를 가열하여 NGC 6357의 거품을 만든다. 이러한 주위의 기체 구름의 존재는 해당 부분의 면밀한 조사를 더욱 어렵게 한다.
Português: Pismis 24-1, uma parte de um aglomerado aberto localizado no núcleo da grande
nebulosa de emissãoNGC 6357, que se estende no céu um grau em direção à
constelação Scorpius. Parte da nebulosa é ionizada pelas estrelas massivas mais jovens (mais azuis) em Pismis 24-1. A intensa radiação ultravioleta das estrelas ardentes aquece o gás que envolve o aglomerado e cria uma bolha na NGC 6357.
NASA, ESA and Jesœs Maz Apellÿniz (Instituto de astrofsica de Andaluca, Spain). Acknowledgement: Davide De Martin (ESA/Hubble)
Licensing
Public domainPublic domainfalsefalse
This file is in the public domain because it was created by
NASA and
ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre.
Copyright statement at hubblesite.org or
2008 copyright statement at spacetelescope.org. For material created by the
European Space Agency on the spacetelescope.org site since 2009, use the
{{ESA-Hubble}} tag.
English: The star cluster
Pismis 24 lies in the core of the large
emission nebulaNGC 6357 that extends one degree on the sky in the direction of the
Scorpius constellation. Part of the nebula is
ionised by the youngest (bluest) heavy stars in Pismis 24. The intense
ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
English: The star cluster
Pismis 24 lies in the core of the large
emission nebulaNGC 6357 that extends one degree on the sky in the direction of the
Scorpius constellation. Part of the nebula is
ionised by the youngest (bluest) heavy stars in Pismis 24. The intense
ultraviolet radiation from the blazing stars heats the gas surrounding the cluster and creates a bubble in NGC 6357. The presence of these surrounding gas clouds makes probing into the region even harder.
Español: El cúmulo estelar
Pismis 24 se encuentra en el núcleo de la gran
nebulosa de emisiónNGC 6357 que se extiende en el cielo un grado en dirección a la
constelación Scorpius. Parte de la nebulosa es ionizada por las estrellas pesadas más jóvenes (más azules) en Pismis 24. La intensa radiación ultravioleta de las estrellas ardientes calienta el gas que rodea el cúmulo y crea una burbuja en NGC 6357. La presencia de estas nubes de gas circundantes hace aún más difícil la exploración de la región.
Italiano: L'
ammasso stellare Pismis 24 nel nucleo della
nebulosa a emissioneNGC 6357. Parte della nebulosa è ionizzata dalle giovani stelle blu in Pismis 24. L'intensa
radiazione ultravioletta dalle stelle infuocate scalda i gas che circondano l'ammasso e creano una bolla in NGC 6357. La presenza di questa nuvola di gas rende l'osservazione della regione ancora più difficile.
Polski: Gromada gwazdPismis 24 położona w centrum ogromnej
mgławicy emisyjnejNGC 6357, która na niebie rozciąga się na jeden stopień w kierunku
gwiazdozbioru Skorpiona. Część mgławicy jest
zjonizowana przez najmłodsze (najbardziej niebieskie) ciężkie
gwiazdy z gromady Pismis 24. Intensywne
promieniowanie ultrafioletowe z płonących gwiazd podgrzewa gaz otaczajacy gromadę i tworzy „bąbel” w mgławicy NGC 6357. Obecność tych chmur gazu sprawia, że badanie tego obszaru jest jeszcze trudniejsze.
Português: Pismis 24-1, uma parte de um aglomerado aberto localizado no núcleo da grande
nebulosa de emissãoNGC 6357, que se estende no céu um grau em direção à
constelação Scorpius. Parte da nebulosa é ionizada pelas estrelas massivas mais jovens (mais azuis) em Pismis 24-1. A intensa radiação ultravioleta das estrelas ardentes aquece o gás que envolve o aglomerado e cria uma bolha na NGC 6357.
한국어: 피스미스 24 성단은
전갈자리 방향의 각도 1도에 펼쳐져 있는 거대한
발광성운NGC 6357의 중심부에 위치한다. 성운의 일부는 피스미스 24 내부의 가장 젊은 (가장 푸른) 무거운 별에 의해
이온화되었다. 이글거리는 별이 내뿜는 강한
자외선 복사가 성단을 둘러싼 기체를 가열하여 NGC 6357의 거품을 만든다. 이러한 주위의 기체 구름의 존재는 해당 부분의 면밀한 조사를 더욱 어렵게 한다.
This is a featured picture on Wikimedia Commons (
Featured pictures) and is considered one of the finest images. See its nomination
here. This is a featured picture on the Arabic language Wikipedia (
صور مختارة) and is considered one of the finest images. See its nomination
here. This is a featured picture on the English language Wikipedia (
Featured pictures) and is considered one of the finest images. See its nomination
here.
{{Information |Description= An
emissionw:nebula, NGC 6357, is on the left. The star Pismis 24-1 (the brightest one) is located to the right of the nubula. |Source= [http://antwrp.gsfc.nasa.gov/apod/image/0612/ngc6357a_hst_big.j
File usage
The following pages on the English Wikipedia use this file (pages on other projects are not listed):