Friday, May 17, 2013

spaceplasma:

Reflection and Emission Nebulas
— Rho Ophiuchi Cloud Complex

Credit:Gerald Rhemann // Astrostudio

(via the-science-llama)

Sunday, May 5, 2013

(Source: apo11o-11)

Friday, May 3, 2013

jetgreguar:

adimals:

spaceplasma:

NASA Probe Gets Close Views of Large Saturn Hurricane

NASA’s Cassini spacecraft has provided scientists the first close-up, visible-light views of a behemoth hurricane swirling around Saturn’s north pole.

In high-resolution pictures and video, scientists see the hurricane’s eye is about 1,250 miles (2,000 kilometers) wide, 20 times larger than the average hurricane eye on Earth. Thin, bright clouds at the outer edge of the hurricane are traveling 330 mph(150 meters per second). The hurricane swirls inside a large, mysterious, six-sided weather pattern known as the hexagon.

“We did a double take when we saw this vortex because it looks so much like a hurricane on Earth,” said Andrew Ingersoll, a Cassini imaging team member at the California Institute of Technology in Pasadena. “But there it is at Saturn, on a much larger scale, and it is somehow getting by on the small amounts of water vapor in Saturn’s hydrogen atmosphere.”

Scientists will be studying the hurricane to gain insight into hurricanes on Earth, which feed off warm ocean water. Although there is no body of water close to these clouds high in Saturn’s atmosphere, learning how these Saturnian storms use water vapor could tell scientists more about how terrestrial hurricanes are generated and sustained.

Both a terrestrial hurricane and Saturn’s north polar vortex have a central eye with no clouds or very low clouds. Other similar features include high clouds forming an eye wall, other high clouds spiraling around the eye, and a counter-clockwise spin in the northern hemisphere.

A major difference between the hurricanes is that the one on Saturn is much bigger than its counterparts on Earth and spins surprisingly fast. At Saturn, the wind in the eye wall blows more than four times faster than hurricane-force winds on Earth. Unlike terrestrial hurricanes, which tend to move, the Saturnian hurricane is locked onto the planet’s north pole. On Earth, hurricanes tend to drift northward because of the forces acting on the fast swirls of wind as the planet rotates. The one on Saturn does not drift and is already as far north as it can be.

“The polar hurricane has nowhere else to go, and that’s likely why it’s stuck at the pole,” said Kunio Sayanagi, a Cassini imaging team associate at Hampton University in Hampton, Va.

Scientists believe the massive storm has been churning for years. When Cassini arrived in the Saturn system in 2004, Saturn’s north pole was dark because the planet was in the middle of its north polar winter. During that time, the Cassini spacecraft’s composite infrared spectrometer and visual and infrared mapping spectrometer detected a great vortex, but a visible-light view had to wait for the passing of the equinox in August 2009. Only then did sunlight begin flooding Saturn’s northern hemisphere. The view required a change in the angle of Cassini’s orbits around Saturn so the spacecraft could see the poles.

“Such a stunning and mesmerizing view of the hurricane-like storm at the north pole is only possible because Cassini is on a sportier course, with orbits tilted to loop the spacecraft above and below Saturn’s equatorial plane,” said Scott Edgington, Cassini deputy project scientist at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “You cannot see the polar regions very well from an equatorial orbit. Observing the planet from different vantage points reveals more about the cloud layers that cover the entirety of the planet.”

Cassini changes its orbital inclination for such an observing campaign only once every few years. Because the spacecraft uses flybys of Saturn’s moon Titan to change the angle of its orbit, the inclined trajectories require attentive oversight from navigators. The path requires careful planning years in advance and sticking very precisely to the planned itinerary to ensure enough propellant is available for the spacecraft to reach future planned orbits and encounters.

Image credit: NASA/JPL-Caltech/SSI

SPACE IS FUCKING COOL

this is so incredible 

Wednesday, April 24, 2013
Friday, April 19, 2013
spaceplasma:




Hubble Sees a Horsehead of a Different Color
Astronomers have used NASA’s Hubble Space Telescope to photograph the iconic Horsehead Nebula in a new, infrared light to mark the 23rd anniversary of the famous observatory’s launch aboard the space shuttle Discovery on April 24, 1990.  Looking like an apparition rising from whitecaps of interstellar foam, the iconic Horsehead Nebula has graced astronomy books ever since its discovery more than a century ago. The nebula is a favorite target for amateur and professional astronomers. It is shadowy in optical light. It appears transparent and ethereal when seen at infrared wavelengths. The rich tapestry of the Horsehead Nebula pops out against the backdrop of Milky Way stars and distant galaxies that easily are visible in infrared light. Hubble has been producing ground-breaking science for two decades. During that time, it has benefited from a slew of upgrades from space shuttle missions, including the 2009 addition of a new imaging workhorse, the high-resolution Wide Field Camera 3 that took the new portrait of the Horsehead.Image Credit: NASA/ESA/Hubble Heritage Team

spaceplasma:

Friday, April 12, 2013

(Source: noirlac)

Monday, April 8, 2013

How the sky would look if the planets were as close as the moon

propertyofroonilwazlib:

quiescense:

guceubcuesu:

Moon…

image

Mercury…

image

Venus…

image

Mars…

image

Jupiter…

image

Saturn…

image

Uranus…

image

Neptune…

image

Pluto can suck a dick

This is so interesting. Jupiter and Saturn look fucking scary

I am more interested in the OP’s hostility toward Pluto

Thursday, March 28, 2013

popmech:

Building MAVEN, the NASA probe that will try to figure out why Mars’ magnetic field—and thus its atmosphere—disappeared.

Saturday, March 9, 2013

(Source: neptunesbounty)

ikenbot:

Saturn’s Hexagon
This is a view of Saturn’s north polar region, taken by Cassini’s Imaging Science Subsystem (ISS) on February 26, 2013. You can see the rings in the top of this image as well as its mysterious hexagon. — Val Klavans

ikenbot:

Saturn’s Hexagon

This is a view of Saturn’s north polar region, taken by Cassini’s Imaging Science Subsystem (ISS) on February 26, 2013. You can see the rings in the top of this image as well as its mysterious hexagon. — Val Klavans

Friday, February 8, 2013

Attention Puella Magi Madoka Magica Fans!

mitsuki-hoshino:

If you are unaware, there was a new nebula found and many Anime fans claim it looked like Goddess Madoka, now there is a petition going around to name the nebula “Madokami Nebula”.

image

It only needs 1.2k more signs, so please sign it! It is a Madoka Magica fan dream come true!

Here is the link to sign the petition [link]! We are so close to the goal!

image

*please re-blog to spread the news!*

immortalizing madoka in the stars forever

YEAH OKAY I CAN GET BEHIND THAT…

Wednesday, January 30, 2013
zawoesi:

Oh hey, not a big deal, but the hubble took a picture of a star that’s nearing supernova status 

aaaaAAAAAAAAAAAAAHHHHHHHHHHHHHHHHHH

zawoesi:

Oh hey, not a big deal, but the hubble took a picture of a star that’s nearing supernova status 

aaaaAAAAAAAAAAAAAHHHHHHHHHHHHHHHHHH

Tuesday, January 1, 2013

ne0ndreams:

sosuperawesome:

NASA on Tumblr, http://n-a-s-a.tumblr.com/

This is way too much space porn for one post.

Monday, December 31, 2012

(Source: astrodidact)

Sunday, December 30, 2012
science-junkie:

Tri-Color Sun
This composite image combines EIT images from three wavelengths (171Å, 195Å and 284Å) into one that reveals solar features unique to each wavelength. Since the EIT images come to us from the spacecraft in black and white, they are color coded for easy identification. For this image, the nearly simultaneous images from May 1998 were each given a color code (red, yellow and blue) and merged into one.
Image: NASA/SOHO

science-junkie:

Tri-Color Sun

This composite image combines EIT images from three wavelengths (171Å, 195Å and 284Å) into one that reveals solar features unique to each wavelength. Since the EIT images come to us from the spacecraft in black and white, they are color coded for easy identification. For this image, the nearly simultaneous images from May 1998 were each given a color code (red, yellow and blue) and merged into one.

Image: NASA/SOHO