File:A changing fan.jpg

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摘要

描述A changing fan.jpg	English: The Universe is rarely static, although the timescales involved can be very long. Since modern astronomical observations began we have been observing the birthplaces of new stars and planets, searching for and studying the subtle changes that help us to figure out what is happening within. The bright spot located at the edge of the bluish fan-shaped structure in this Hubble image is a young star called V* PV Cephei, or PV Cep. It is a favourite target for amateur astronomers because the fan-shaped nebulosity, known as GM 1-29 or Gyulbudaghian’s Nebula, changes over a timescale of months. The brightness of the star has also varied over time. Images of PV Cep taken in 1952 showed a nebulous streak, similar to a comet’s tail. However, these had vanished when new images of the star were obtained some twenty-five years later. Instead, the blue fan-shaped nebula had appeared. Twenty-five years is a very short period on cosmic timescales, so astronomers think that the mysterious streak may have been a temporary phenomenon, such as the remnants of a massive stellar flare — similar to the solar flares we are used to seeing in the Solar System. At the same time as this was happening, the star itself was brightening. This provided the light to illuminate the newly formed fan-shaped nebula. This brightening might be related to the start of the hydrogen-burning phase of the star, which would mean that it was reaching maturity. PV Cep is thought to be surrounded by a disc of gas and dust, which would stop light from escaping in all directions. The fan-like appearance is therefore probably a result of starlight escaping from the dust disc and projecting onto the nebula. PV Cep is located in the northern constellation of Cepheus at a distance of over 1600 light-years from Earth. A version of this image was entered into the Hubble’s Hidden Treasures competition by contestant Alexey Romashin.
日期	2013年4月22日, 10:00:00
来源	http://www.spacetelescope.org/images/potw1316a/
作者	ESA/Hubble & NASA. Acknowledgement: Alexey Romashin

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署名

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文件历史

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	日期/时间	缩⁠略⁠图	大小	用户	备注
当前	2013年4月22日 (一) 11:20		1,465 × 945（678 KB）	Jmencisom	User created page with UploadWizard

文件用途

以下页面使用本文件：

仙王座PV

全域文件用途

以下其他wiki使用此文件：

en.wikipedia.org上的用途
- PV Cephei
- Gyulbudaghian's Nebula
sv.wikipedia.org上的用途
- PV Cephei
www.wikidata.org上的用途
- Q14559458

元数据

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来源	ESA/Hubble
提供者	ESA/Hubble & NASA.Acknowledgement: Alexey Romashin
图像标题	The Universe is rarely static, although the timescales involved can be very long. Since modern astronomical observations began we have been observing the birthplaces of new stars and planets, searching for and studying the subtle changes that help us to figure out what is happening within. The bright spot located at the edge of the bluish fan-shaped structure in this Hubble image is a young star called V* PV Cephei, or PV Cep. It is a favourite target for amateur astronomers because the fan-shaped nebulosity, known as GM 1-29 or Gyulbudaghian’s Nebula, changes over a timescale of months. The brightness of the star has also varied over time. Images of PV Cep taken in 1952 showed a nebulous streak, similar to a comet’s tail. However, these had vanished when new images of the star were obtained some twenty-five years later. Instead, the blue fan-shaped nebula had appeared. Twenty-five years is a very short period on cosmic timescales, so astronomers think that the mysterious streak may have been a temporary phenomenon, such as the remnants of a massive stellar flare — similar to the solar flares we are used to seeing in the Solar System. At the same time as this was happening, the star itself was brightening. This provided the light to illuminate the newly formed fan-shaped nebula. This brightening might be related to the start of the hydrogen-burning phase of the star, which would mean that it was reaching maturity. PV Cep is thought to be surrounded by a disc of gas and dust, which would stop light from escaping in all directions. The fan-like appearance is therefore probably a result of starlight escaping from the dust disc and projecting onto the nebula. PV Cep is located in the northern constellation of Cepheusat a distance of over 1600 light-years from Earth. A version of this image was entered into the Hubble’s Hidden Treasures competition by contestant Alexey Romashin.
简短标题	A changing fan
使用条款	Creative Commons Attribution 3.0 Unported license
数据生成日期时间	2013年4月22日 (一) 10:00
关键词	GM 1-29 Gyulbudaghian’s Nebula PV Cephei
联系信息	http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei M√ºnchen, , D-85748 Germany

File:A changing fan.jpg

摘要

许可协议

说明

此文件中描述的项目

描绘内容

版权状态

版权所有

许可协议

知识共享署名4.0国际

成立或创建时间

22 4 2013

媒体类型

image/jpeg

校验和

2a0f961bb34f846a7964b48ff730e7d5e9ad0525

数据大小

694,456 字节

高度

945 像素

宽度

1,465 像素

文件历史

文件用途

全域文件用途

元数据