(Source: what-do-i-wear, via iwantbigcloset)

IBELIEVEICANFLYYYYYYEOWW!

(via surirumahtangga)

Dolce&Gabbana fw 11\12
Milan Fashion Week

colours. stars. sequins 

(Source: frankfashion)

galaxy dress!

(via hannarabittah)

sleep away the sadness of today.

(via itsabombshell)

(Source: imgfavepopular, via imgfave)

(via isthishardcore)

(Source: highonflowers)

nonverbalmag:

Gorgeous

(via moonhmz)

seeing stars.

(Source: highonflowers)

Supernova Remnant (via APOD: 2009 August 1 - SN 1006 Supernova Remnant)

Explanation: A new star, likely the brightest supernova in recorded human history, lit up planet Earth’s sky in the year 1006 AD. The expanding debris cloud from the stellar explosion, found in the southerly constellation of Lupus, still puts on a cosmic light show across the electromagnetic spectrum. In fact, this composite view includes X-ray data in blue from the Chandra Observatory, optical data in yellowish hues, and radio image data in red. Now known as the SN 1006 supernova remnant, the debris cloud appears to be about 60 light-years across and is understood to represent the remains of a white dwarf star. Part of a binary star system, the compact white dwarf gradually captured material from its companion star. The buildup in mass finally triggered a thermonuclear explosion that destroyed the dwarf star. Because the distance to the supernova remnant is about 7,000 light-years, that explosion actually happened 7,000 years before the light reached Earth in 1006. Shockwaves in the remnant accelerate particles to extreme energies and are thought to be a source of the mysterious cosmic rays.

naked open cluster of stars. (via APOD: 2009 August 2 - Stars, Dust and Nebula in NGC 6559)

Explanation: Visible above are red glowing emission nebulas of hydrogen, blue reflection nebulas of dust, dark absorption nebulas of dust, and the stars that formed from them. The first massive stars formed from the dense gas will emit energetic light and winds that erode, fragment, and sculpt their birthplace. And then they explode. The resulting morass can be as beautiful as it is complex. After tens of millions of years, the dust boils away, the gas gets swept away, and all that is left is a naked open cluster of stars.

A Star is Formed (via APOD: 2009 August 3 - T Tauri: A Star is Formed)

Explanation: What does a star look like when it is forming? The prototypical example is the variable star T Tauri, visible as the bright orange star near the image center. The orange star centered in this remarkable telescopic skyview is T Tauri, prototype of the class of T Tauri variable stars. Surrounding T Tauri is a dusty yellow cosmic cloud named the Hind’s Variable Nebula (NGC 1555/1554). Over 400 light-years away, at the edge of a molecular cloud, both star and nebula are seen to vary significantly in brightness but not necessarily at the same time, adding to the mystery of the intriguing region. T Tauri stars are now generally recognized as young — less than a few million years old — sun-like stars still in the early stages of formation. To further complicate the picture, infrared observations indicate that T Tauri itself is part of a multiple star system. Surprisingly, due to a close gravitational pass near one of these stars, T Tauri may now be headed out of the system. The dramatic color image above captures a region that spans about 4 light-years.

The Milky Way Over Devils Tower (via APOD: 2009 July 29 - The Milky Way Over Devils Tower)