EARTHSIGN

Mar 18

flapjacksblog2 asked: Do you like to go on adventures?

Sometimes.. Pictures and Videos are just as much an adventure as to me as actually going on one. :D

alladylike asked: diff i am not. lol. if u had to go through what my bf goes through for me. then u would understand ahah

if i had to go through you to understand. then im all for it. :P just know u are a good person and special girl. u should never have to appoligize for being yourself.

Aug 05

Thanks For The Follow

So many people to thank….Too many to thank! I’ve been on vacation sorry I haven’t blogged in a month! U know who you are!!! THANKS!

Jun 18

South Georgia Island
South Georgia Island is notable on several fronts. The first recorded  explorer to land on the island was Captain James Cook aboard the HMS  Resolution in 1775. He mapped part of the coastline, but was discouraged  by the thick ice cover, lack of vegetation, and steep mountains. Mt.  Paget, the highest peak, rises to 9,625 feet above sea level, and the  island supports 161 glaciers. Cook named the southernmost point of the  island “Cape Disappointment” when he realized he had not reached  Antarctica.

South Georgia Island

South Georgia Island is notable on several fronts. The first recorded explorer to land on the island was Captain James Cook aboard the HMS Resolution in 1775. He mapped part of the coastline, but was discouraged by the thick ice cover, lack of vegetation, and steep mountains. Mt. Paget, the highest peak, rises to 9,625 feet above sea level, and the island supports 161 glaciers. Cook named the southernmost point of the island “Cape Disappointment” when he realized he had not reached Antarctica.

 Aurora From Space
What do auroras look like from space? From the ground, auroras dance  high above clouds, frequently causing spectacular displays. The  International Space Station (ISS) orbits just at the same height as many  auroras, though. Therefore, sometimes it flies over them, but also  sometimes it flies right through. The auroral electron and proton  streams are too thin to be a danger to the ISS, just as clouds pose  little danger to airplanes. ISS Science Officer Don Pettit captured a  green aurora, pictured above in a digitally sharpened image. From orbit,  Dr. Pettit reports, changing auroras can appear to crawl around like  giant green amoebas. Far below, on planet Earth, the Manicouagan Impact  Crater can be seen in northern Canada.

Aurora From Space

What do auroras look like from space? From the ground, auroras dance high above clouds, frequently causing spectacular displays. The International Space Station (ISS) orbits just at the same height as many auroras, though. Therefore, sometimes it flies over them, but also sometimes it flies right through. The auroral electron and proton streams are too thin to be a danger to the ISS, just as clouds pose little danger to airplanes. ISS Science Officer Don Pettit captured a green aurora, pictured above in a digitally sharpened image. From orbit, Dr. Pettit reports, changing auroras can appear to crawl around like giant green amoebas. Far below, on planet Earth, the Manicouagan Impact Crater can be seen in northern Canada.

Fish-Eye View of Atlantis
Fish-eye view of the Space Shuttle Atlantis as seen from the Russian Mir  space station during the STS-71 mission.

Fish-Eye View of Atlantis

Fish-eye view of the Space Shuttle Atlantis as seen from the Russian Mir space station during the STS-71 mission.

A Long Way From Home
This image of the Earth and moon in a single frame, the first of its  kind ever taken by a spacecraft, was recorded on Sept. 18, 1977, by  Voyager 1 when it was 7.25 million miles from Earth. The moon is at the  top of the picture and beyond the Earth as viewed by Voyager. In the picture are eastern Asia, the western Pacific Ocean and part of  the Arctic. Voyager 1 was directly above Mt. Everest (on the night side  of the planet at 25 degrees north latitude) when the picture was taken. The photo was made from three images taken through color filters, then  processed at NASA’s Jet Propulsion Laboratory. Because the Earth is many  times brighter than the moon, the moon was artificially brightened so  that both bodies would show clearly in the prints.

A Long Way From Home

This image of the Earth and moon in a single frame, the first of its kind ever taken by a spacecraft, was recorded on Sept. 18, 1977, by Voyager 1 when it was 7.25 million miles from Earth. The moon is at the top of the picture and beyond the Earth as viewed by Voyager. In the picture are eastern Asia, the western Pacific Ocean and part of the Arctic. Voyager 1 was directly above Mt. Everest (on the night side of the planet at 25 degrees north latitude) when the picture was taken. The photo was made from three images taken through color filters, then processed at NASA’s Jet Propulsion Laboratory. Because the Earth is many times brighter than the moon, the moon was artificially brightened so that both bodies would show clearly in the prints.

Stellar Quakes
In December 2004, a neutron star flared up so brightly, it temporarily  blinded all the x-ray satellites in space, and lit up the Earth’s upper  atmosphere. This tremendous blast of energy was from a giant flare  created by the neutron star’s twisting magnetic field. Objects like this  are called magnetars, and they produce magnetic fields trillions of  time more powerful than those here on Earth. These fields are so strong  they can actually buckle the surface of the neutron star causing these  powerful star quakes.

Stellar Quakes

In December 2004, a neutron star flared up so brightly, it temporarily blinded all the x-ray satellites in space, and lit up the Earth’s upper atmosphere. This tremendous blast of energy was from a giant flare created by the neutron star’s twisting magnetic field. Objects like this are called magnetars, and they produce magnetic fields trillions of time more powerful than those here on Earth. These fields are so strong they can actually buckle the surface of the neutron star causing these powerful star quakes.

Quintuplet Cluster
Penetrating 25,000 light-years of obscuring dust and myriad stars, the  Hubble Space Telescope has provided the clearest view yet of one of the  largest young clusters of stars inside our Milky Way galaxy, located  less than 100 light-years from the very center of the Galaxy. Having the  equivalent mass greater than 10,000 stars like our sun, the monster  cluster is ten times larger than typical young star clusters scattered  throughout our Milky Way. It is destined to be ripped apart in just a  few million years by gravitational tidal forces in the galaxy’s core.  But in its brief lifetime it shines more brightly than any other star  cluster in the Galaxy. The 4-million-year-old Quintuplet Cluster also is  home to the brightest star seen in the galaxy, the so-called Pistol  star.

Quintuplet Cluster

Penetrating 25,000 light-years of obscuring dust and myriad stars, the Hubble Space Telescope has provided the clearest view yet of one of the largest young clusters of stars inside our Milky Way galaxy, located less than 100 light-years from the very center of the Galaxy. Having the equivalent mass greater than 10,000 stars like our sun, the monster cluster is ten times larger than typical young star clusters scattered throughout our Milky Way. It is destined to be ripped apart in just a few million years by gravitational tidal forces in the galaxy’s core. But in its brief lifetime it shines more brightly than any other star cluster in the Galaxy. The 4-million-year-old Quintuplet Cluster also is home to the brightest star seen in the galaxy, the so-called Pistol star.

Galaxy NGC 4013
An amazing “edge-on” view of a spiral galaxy 55 million light years from  Earth has been captured by the Hubble Space Telescope. The image  reveals in great detail huge clouds of dust and gas extending along and  above the galaxy’s main disk.

Galaxy NGC 4013

An amazing “edge-on” view of a spiral galaxy 55 million light years from Earth has been captured by the Hubble Space Telescope. The image reveals in great detail huge clouds of dust and gas extending along and above the galaxy’s main disk.

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Jun 17

The Unveiling
On its 100,000th orbit of planet Earth, the Hubble Space Telescope  peered into a small portion of the Tarantula Nebula near the star  cluster NGC 2074, unveiling its stellar nursery. The region is a  firestorm of raw stellar creation, triggered perhaps by a nearby  supernova. The image reveals dramatic ridges and valleys of dust, serpent-headed  “pillars of creation,” and gaseous filaments glowing fiercely under  torrential ultraviolet radiation. The region is on the edge of a dark  molecular cloud that is an incubator for the birth of new stars. The high-energy radiation blazing out from clusters of hot young stars  is slowly eroding nebula, and another young cluster may be hidden  beneath the circle of brilliant blue gas. The region is in the Large Magellanic Cloud, a satellite of our Milky  Way galaxy that is a fascinating laboratory for observing star-formation  regions and their evolution. Dwarf galaxies like the Large Magellanic  Cloud are considered to be the primitive building blocks of larger  galaxies.

The Unveiling

On its 100,000th orbit of planet Earth, the Hubble Space Telescope peered into a small portion of the Tarantula Nebula near the star cluster NGC 2074, unveiling its stellar nursery. The region is a firestorm of raw stellar creation, triggered perhaps by a nearby supernova. The image reveals dramatic ridges and valleys of dust, serpent-headed “pillars of creation,” and gaseous filaments glowing fiercely under torrential ultraviolet radiation. The region is on the edge of a dark molecular cloud that is an incubator for the birth of new stars. The high-energy radiation blazing out from clusters of hot young stars is slowly eroding nebula, and another young cluster may be hidden beneath the circle of brilliant blue gas. The region is in the Large Magellanic Cloud, a satellite of our Milky Way galaxy that is a fascinating laboratory for observing star-formation regions and their evolution. Dwarf galaxies like the Large Magellanic Cloud are considered to be the primitive building blocks of larger galaxies.

Dark Clouds of the Carina Nebula
What dark forms lurk in the mists of the Carina Nebula? These ominous  figures are actually molecular clouds, knots of molecular gas and dust  so thick they have become opaque. In comparison, however, these clouds  are typically much less dense than Earth’s atmosphere. Pictured above is part of the most detailed image of the Carina Nebula  ever taken where dark molecular clouds are particularly prominent. The  entire Carina Nebula spans more than 300 light years and lies about  7,500 light-years away in the constellation of Carina. NGC 3372, known as the Great Nebula in Carina, is home to massive stars  and changing nebula. Eta Carinae, the most energetic star in the nebula,  was one of the brightest stars in the sky in the 1830s, but then faded  dramatically. Wide-field annotated and zoomable versions of the larger  image composite are also available.

Dark Clouds of the Carina Nebula

What dark forms lurk in the mists of the Carina Nebula? These ominous figures are actually molecular clouds, knots of molecular gas and dust so thick they have become opaque. In comparison, however, these clouds are typically much less dense than Earth’s atmosphere. Pictured above is part of the most detailed image of the Carina Nebula ever taken where dark molecular clouds are particularly prominent. The entire Carina Nebula spans more than 300 light years and lies about 7,500 light-years away in the constellation of Carina. NGC 3372, known as the Great Nebula in Carina, is home to massive stars and changing nebula. Eta Carinae, the most energetic star in the nebula, was one of the brightest stars in the sky in the 1830s, but then faded dramatically. Wide-field annotated and zoomable versions of the larger image composite are also available.

Terrible Twos
Young stars, like toddlers, want to start showing their independence.  This Spitzer view shows a stellar version of the “terrible twos” — the  stars are beginning to move away from their formative cloud, seen in red  and green. Jets can be seen coming off the young stars as they make  their way into the cosmos. Located 1,000 light-years from Earth in the constellation Perseus, the  reflection nebula NGC 1333 epitomizes the beautiful chaos of a dense  group of stars being born.

Terrible Twos

Young stars, like toddlers, want to start showing their independence. This Spitzer view shows a stellar version of the “terrible twos” — the stars are beginning to move away from their formative cloud, seen in red and green. Jets can be seen coming off the young stars as they make their way into the cosmos. Located 1,000 light-years from Earth in the constellation Perseus, the reflection nebula NGC 1333 epitomizes the beautiful chaos of a dense group of stars being born.

Cat’s Eye Nebula Redux

This composite of data from NASA’s Chandra X-ray  Observatory and Hubble Space Telescope gives astronomers a new look for  NGC 6543, better known as the Cat’s Eye nebula. This planetary nebula  represents a phase of stellar evolution that our sun may well experience  several billion years from now. When a star like the sun begins to run out of fuel, it becomes a red  giant. In this phase, a star sheds some of its outer layers, eventually  leaving behind a hot core that collapses to form a dense white dwarf  star. A fast wind emanating from the hot core rams into the ejected  atmosphere, pushes it outward, and creates the graceful filamentary  structures seen with optical telescopes. In the case of the Cat’s Eye, material shed by the star is flying away  at a speed of about 4 million miles per hour. The star itself is  expected to collapse to become a white dwarf star in a few million  years.

Cat’s Eye Nebula Redux

This composite of data from NASA’s Chandra X-ray Observatory and Hubble Space Telescope gives astronomers a new look for NGC 6543, better known as the Cat’s Eye nebula. This planetary nebula represents a phase of stellar evolution that our sun may well experience several billion years from now. When a star like the sun begins to run out of fuel, it becomes a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes. In the case of the Cat’s Eye, material shed by the star is flying away at a speed of about 4 million miles per hour. The star itself is expected to collapse to become a white dwarf star in a few million years.