Jordan CP 2’Quick アンスラサイト/赤 バスケットボールショップ SLAM
Jordan CP 2’Quick アンスラサイト/赤 バスケットボールショップ SLAM
Fukushima Daiichi NPS 8 October 2011 Photos
Fukushima Daiichi NPS 8 October 2011 Photos
Fukushima Daiichi Nuclear Power Station 19 November 2011
Fukushima Daiichi Nuclear Power Station 19 November 2011
blacksheepboy-:

Almost Home by David Fleck
blacksheepboy-:

Almost Home by David Fleck
blacksheepboy-:

Travels in New Zealand (by SundrySullen)
blacksheepboy-:

Travels in New Zealand (by SundrySullen)

blacksheepboy-:

Travels in New Zealand (by SundrySullen)

unknownskywalker:

Hubble serves up a holiday snow angel
NASA’s Hubble Space Telescope presents a festive holiday greeting that’s out of this world. The bipolar star-forming region, called Sharpless 2-106, looks like a soaring, celestial snow angel. The outstretched “wings” of the nebula record the contrasting imprint of heat and motion against the backdrop of a colder medium.
Sharpless 2-106 lies nearly 2,000 light-years from us. The nebula measures several light-years in length. It appears in a relatively isolated region of the Milky Way galaxy. Twin lobes of super-hot gas — glowing blue in this image — stretch outward from the massive, young star IRS 4, creating the “wings” of our angel.
A ring of dust and gas orbiting the star acts like a belt, cinching the expanding nebula into an “hourglass” shape, with ripples and ridges in the gas interacting with the cooler interstellar medium. Dusky red veins surround the blue emission from the nebula. The faint light emanating from the central star reflects off of tiny dust particles. This illuminates the environment around the star, showing darker filaments of dust winding beneath the blue lobes.
Infrared observations of the nebula have also uncovered more than 600 brown dwarfs with weighs less than a tenth of our Sun. Because of their low mass, they cannot produce sustained energy through nuclear fusion like our Sun does. They encompass the nebula in a small cluster.
Watch video: Three-dimensional view of Sharpless 2-106
unknownskywalker:

Hubble serves up a holiday snow angel
NASA’s Hubble Space Telescope presents a festive holiday greeting that’s out of this world. The bipolar star-forming region, called Sharpless 2-106, looks like a soaring, celestial snow angel. The outstretched “wings” of the nebula record the contrasting imprint of heat and motion against the backdrop of a colder medium.
Sharpless 2-106 lies nearly 2,000 light-years from us. The nebula measures several light-years in length. It appears in a relatively isolated region of the Milky Way galaxy. Twin lobes of super-hot gas — glowing blue in this image — stretch outward from the massive, young star IRS 4, creating the “wings” of our angel.
A ring of dust and gas orbiting the star acts like a belt, cinching the expanding nebula into an “hourglass” shape, with ripples and ridges in the gas interacting with the cooler interstellar medium. Dusky red veins surround the blue emission from the nebula. The faint light emanating from the central star reflects off of tiny dust particles. This illuminates the environment around the star, showing darker filaments of dust winding beneath the blue lobes.
Infrared observations of the nebula have also uncovered more than 600 brown dwarfs with weighs less than a tenth of our Sun. Because of their low mass, they cannot produce sustained energy through nuclear fusion like our Sun does. They encompass the nebula in a small cluster.
Watch video: Three-dimensional view of Sharpless 2-106

unknownskywalker:

Hubble serves up a holiday snow angel

NASA’s Hubble Space Telescope presents a festive holiday greeting that’s out of this world. The bipolar star-forming region, called Sharpless 2-106, looks like a soaring, celestial snow angel. The outstretched “wings” of the nebula record the contrasting imprint of heat and motion against the backdrop of a colder medium.

Sharpless 2-106 lies nearly 2,000 light-years from us. The nebula measures several light-years in length. It appears in a relatively isolated region of the Milky Way galaxy. Twin lobes of super-hot gas — glowing blue in this image — stretch outward from the massive, young star IRS 4, creating the “wings” of our angel.

A ring of dust and gas orbiting the star acts like a belt, cinching the expanding nebula into an “hourglass” shape, with ripples and ridges in the gas interacting with the cooler interstellar medium. Dusky red veins surround the blue emission from the nebula. The faint light emanating from the central star reflects off of tiny dust particles. This illuminates the environment around the star, showing darker filaments of dust winding beneath the blue lobes.

Infrared observations of the nebula have also uncovered more than 600 brown dwarfs with weighs less than a tenth of our Sun. Because of their low mass, they cannot produce sustained energy through nuclear fusion like our Sun does. They encompass the nebula in a small cluster.

Watch video: Three-dimensional view of Sharpless 2-106

2011年の動物の写真ベスト50  衝撃的な写真ありすぎワロタ:ハムスター速報
2011年の動物の写真ベスト50  衝撃的な写真ありすぎワロタ:ハムスター速報

http://ci.nii.ac.jp/els/110004653923.pdf?id=ART0007378351&type=pdf&lang=jp&host=cinii&order_no=&ppv_type=0&lang_sw=&no=1323686915&cp=

http://ci.nii.ac.jp/els/110004654513.pdf?id=ART0007379157&type=pdf&lang=jp&host=cinii&order_no=&ppv_type=0&lang_sw=&no=1323686677&cp=

http://ci.nii.ac.jp/els/110004654513.pdf?id=ART0007379157&type=pdf&lang=jp&host=cinii&order_no=&ppv_type=0&lang_sw=&no=1323686677&cp=

CiNii 論文 -  特集 建具と空間--〈可変空間〉のための技術

SBA_Glass Shutter House
SBA_Glass Shutter House