Sailing Across the Sun

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harkwhostalking:

needleless clock (by I.E.)
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harkwhostalking:

needleless clock (by I.E.)

(via vintage-kisses)

Source: Flickr / ikumixx

  • 2 hours ago > harkwhostalking
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independiente:

yerba buena gardens (by Débora-Gonzales)
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independiente:

yerba buena gardens (by Débora-Gonzales)

(via vintage-kisses)

Source: Flickr / deboragonzales

  • 2 hours ago > independiente
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eternityonwings:

287 bucinnums by dd21207 on Flickr.
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eternityonwings:

287 bucinnums by dd21207 on Flickr.

(via vintage-kisses)

Source: eternityonwings

  • 2 hours ago > eternityonwings
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(via grayisme)

Source: weheartit.com

  • 2 hours ago > moncheriette
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(via elegance-is-a-nuisance)

Source: 4spen

  • 2 hours ago > 4spen
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cataclysm:

h2o br0 on We Heart It. http://weheartit.com/entry/27018940
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cataclysm:

h2o br0 on We Heart It. http://weheartit.com/entry/27018940

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Source: weheartit.com

  • 3 hours ago > cataclysm
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(via hisprincesss)

Source: weheartit.com

  • 6 hours ago > c-h-o-c-o-l-a-t-e-r-i-e
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fyeahuniverse:

White Dwarf Star Measurements Bring Milky Way Into Focus

Understanding the masses of stars in the early stages of their lives, before they became white dwarfs is key to understanding the formation of galaxies. New research by astronomer, Jason Kalirai, has described a new technique for calculating this through the use of the mass of the white dwarf stars they become.
The age of a star is directly related to its mass. The more massive a star, the more pressure at its core and the faster it burns through its hydrogen supply. This is key. The increasing precision with which we can calculate age and mass helps us resolve the entire sequence of stellar evolution.

(Image credit:Sere Brunier)
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fyeahuniverse:

White Dwarf Star Measurements Bring Milky Way Into Focus

Understanding the masses of stars in the early stages of their lives, before they became white dwarfs is key to understanding the formation of galaxies. New research by astronomer, Jason Kalirai, has described a new technique for calculating this through the use of the mass of the white dwarf stars they become.

The age of a star is directly related to its mass. The more massive a star, the more pressure at its core and the faster it burns through its hydrogen supply. This is key. The increasing precision with which we can calculate age and mass helps us resolve the entire sequence of stellar evolution.

(Image credit:Sere Brunier)

Source: fyeahuniverse

  • 6 hours ago > fyeahuniverse
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I’ve always wanted to visit a vintage drive in :/
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I’ve always wanted to visit a vintage drive in :/

(via elegance-is-a-nuisance)

Source: weheartit.com

  • 6 hours ago > awanderingbrunette
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Source: glowinthedarkdildo

  • 6 hours ago > glowinthedarkdildo
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