All posts by Zand Space

Ghost Lights from Earth Orbit

A “Ghost Light” is an unexplained luminescent phenomena. That’s how aliens might see Earth if they arrived with no awareness of its civilizations, atmosphere and climate, and magnetic field. Astronauts aboard the International Space Station are all too familiar with the city lights, the thunderstorms, and the aurorae that turn Earth into a planet of soft glows and flickering beams. This video has been made up of timelapse sequences captured aboard the ISS. Enjoy in 1080p!

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Re-Launching the First Science Rocket to Space

From NASA/JPL. A NASA scientist, physics professor, and model rocket hobbyist recreates an historic rocket launched by aeronautics pioneer Frank Malina. The first WAC Corporal dummy round was launched on September 16, 1945 from White Sands Missile Range near Las Cruces, New Mexico. After a White Sands V-2 rocket had reached 69 miles on May 10, a White Sands WAC Corporal reached 80 km (49 mi) on May 22, 1946 — the first U.S.-designed rocket to reach the edge of space (under the U.S. definition of space at the time). On February 24, 1949, a Bumper (a German V-2 rocket acting as first stage) bearing a WAC Corporal at White Sands accelerated to 5,150 mph to become the first flight of more than five times the speed of sound.

Scientists were later surprised when almost a year after the launch, tail fragments of the WAC Corporal rocket that reached 5,150 mph and an altitude of over 250 miles, were found and identified in the New Mexico desert near the launch site.

A few WAC Corporals survive in museums, including one at the National Air and Space Museum and another in the White Sands Missile Range Museum. Here are its specs:

Diameter: 1 ft Continue reading Re-Launching the First Science Rocket to Space

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The Great Solar Mag Flip

From NASA Heliophysics. The number of sunspots increases and decreases over time in a regular, approximately 11-year cycle, called the sunspot cycle. The exact length of the cycle can vary. It has been as short as eight years and as long as fourteen, but the number of sunspots always increases over time, and then returns to low again.

More sunspots mean increased solar activity, when great blooms of radiation known as solar flares or bursts of solar material known as coronal mass ejections (CMEs) shoot off the sun’s surface. The highest number of sun spots in any given cycle is designated “solar maximum,” while the lowest number is designated “solar minimum.” Each cycle, varies dramatically in intensity, with some solar maxima being so low as to be almost indistinguishable from the preceding minimum.

Sunspots are a magnetic phenomenon and the entire sun is magnetized with a north and a south magnetic pole just like a bar magnet. The comparison to a simple bar magnet ends there, however, as the sun’s interior is constantly on the move.

By tracking sound waves that course through the center of the sun, an area of research known as helioseismology, scientists can gain an understanding of what’s deep Continue reading The Great Solar Mag Flip

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Einstein’s Greatest Blunder

Excerpt from “Mysteries of a Dark Universe.” Albert Einstein sought to explain why the gravity of all the stars and gas out there didnt simply cause the universe to collapse into a heap. Following the discovery of the expanding universe, he admitted to the “greatest blunder” of his career.

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What sets Curiosity apart from other Mars Rovers?

The Mars Science Lab was launched November 26, 2011, and is scheduled to land on Mars at Gale Crater on August 6, 2012. The rover Curiosity, after completing a more precise landing than ever attempted previously, is intended to help assess Mars’ habitability for future human missions. Its primary mission objective is to determine whether Mars is or has ever been an environment able to support life.

Curiosity is five times as large as either of the Mars Exploration Rovers Spirit or Opportunity and carries more than ten times the mass of scientific instruments present on the older vehicles. The rover is expected to operate for at least 686 days as it explores with greater range than any previous Mars rover. Here are some of the specs that help set Curiosity apart from the other rovers:

The rover Curiosity is 3 meters in length, and weighs 900 kg, including 80 kg worth of scientific instruments. It is approximately the size of a Mini Cooper automobile.

Once on the surface, Curiosity will be able to roll over obstacles approaching 75 cm high. Maximum terrain-traverse speed is estimated to be 90 meters per hour by automatic navigation, however, with average speeds likely to be Continue reading What sets Curiosity apart from other Mars Rovers?

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Black Hole Meltdown in the Galactic Center

Black hole extravaganza from ESOcast. Not long ago, watching something being ripped apart as it falls towards a giant black hole would be science fiction. This is now reality.

Observers under dark skies, far from the bright city lights, can marvel at the splendor of the Milky Way, arching in an imposing band across the sky. Zooming in towards the center of our galaxy, about 25000 light years away, you can see that it is composed of myriads of stars.

This is a pretty impressive sight, but much is hidden from view by interstellar dust, and astronomers need to look using a different wavelength, the infrared, that can penetrate the dust clouds. With large telescopes, astronomers can then see in detail the swarm of stars circling the supermassive black hole, in the same way that the Earth orbits the Sun.

The Galactic Center harbors the closest supermassive black hole known, and the one that is also the largest in terms of its angular diameter on the sky, making it the best choice for a detailed study of black holes.

This black hole’s mass is a hefty four million times that of the Sun, earning it the title of supermassive black hole. Although it is Continue reading Black Hole Meltdown in the Galactic Center

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The Violent End Stage of Star Formation

EsoCast showcases a new Hubble image of a giant cloud of hydrogen gas illuminated by a bright young star. The image shows how violent the end stages of the star formation process can be, with the young object shaking up its stellar nursery.

A few thousand light-years away, in the constellation of Cygnus, lies the compact star-forming region Sh 2-106, or S106 for short. Despite the celestial colors of this picture, there is nothing peaceful about this scene. A young star, named S106 IR, is being born at the heart of the nebula. In the violent final stages of its formation, the star is ejecting material at high speed, violently disrupting the gas and dust. 3D visualizations show the extent to which the star has carved its surroundings into a complex shape. In particular, the hourglass-like structure of the nebula is a result of jets from the star slamming into the cloud of hydrogen it is forming from.

At the outer edges of these cavities, the gas has been compressed into shock fronts by the pressure. The star has a mass about 15 times that of the Sun and is in the final stages of its formation. It will soon quiet down Continue reading The Violent End Stage of Star Formation

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The View from Space – Earth’s Countries and Coastlines

These high-res time-lapse sequences captured by astronauts aboard the International Space Station give us a beautiful and clear view of some well-known coastlines and countries around the world. Get a good look at England, France, Italy, Egypt, Algeria, Tunisia, Greece, the island of Crete, Taiwan, South Korea, Japan, the United States, Mexico, Ecuador, Peru, Chile, Argentina, Cuba, and more. We’ve attempted to show as many countries as we would, but inevitably we’ve left many out. Please write to the the astronaut photography office at NASA’s Johnson Space Center to request inclusion in this amazing series of sequences.

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The Spectacle of Star Death

Take a breathtaking journey into the future, five billion years from now, to see the ultimate fate of the Solar System. This gem from HubbleCast showcases stunning Hubble imagery of the death throes of Sun-like stars. The wreckage of these dying stars form the building blocks of new generations of stars.

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