The Heart Nebula or IC 1805, lies some 7500 light years away from Earth and is located in the Perseus Arm of the Galaxy in the constellation Cassiopeia. This is an emission nebula showing glowing ionized hydrogen gas and darker dust lanes.
Image Credit: Simon Addis
NASAs Solar Dynamics Observatory captured this image of a significant solar flare as seen in the bright flash on the right on Dec. 19, 2014. The image shows a subset of extreme ultraviolet light that highlights the extremely hot material in flares
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South pole of Jupiter photographed by Voyager 1 on March 1, 1979
Credit: NASA / Voyager 1
Ghost Nebula
This stunning multi-mission picture shows off the many sides of the supernova remnant Cassiopeia A. It is made up of images taken by three of NASA’s Great Observatories, using three different wavebands of light. Infrared data from the Spitzer Space Telescope are colored red; visible data from the Hubble Space Telescope are yellow; and X-ray data from the Chandra X-ray Observatory are green and blue.
Image credit: NSA/JPL
Weather permitting, you can observe the Moon most nights, unless it’s a new moon, when the lighted side of the Moon faces away from Earth. The Moon is by far the brightest object in the night sky and there’s plenty to see. But this week is special…
…October 28 is International Observe the Moon Night (also known as InOMN).
Everyone on Earth is invited to join the celebration by hosting or attending an InOMN event and uniting on one day each year to look at and learn about the Moon together.
October’s night skies are full of sights, from the first quarter Moon on InOMN to Saturn making a cameo appearance above the Moon October 23 and 24. Watch our What’s Up video for details.
Hundreds of events are planned around the globe. Click the top link on this page for a handy map. You can also register your own event.
Here are some activities for enhanced Moon watching.
Download InOMN flyers and handouts, Moon maps and even some pre-made presentations. There’s even a certificate to mark your participation.
Almost dead center on the Earth-facing side of the Moon is the Surveyor 6 robotic spacecraft impact side. Apollo 12 and 14 are a bit to the left. And Apollo 11 - the first steps on the moon - are to the right. This retro graphic tells the whole story.
NASA photographers have done some exceptional work capturing views of the Moon from Earth. Here are a few galleries:
You can’t have a solar eclipse without the Moon.
The 2016 “Supermoon” was pretty spectacular.
The Moon gets eclipsed, too.
That IS a Moon - AND the International Space Station.
The Moon is always a great photo subject.
Some spooky shots of the 2014 “Supermoon.”
And 2013.
Tips from a NASA pro for photographing the Moon.
Twelve human beings walked on the face of the Moon. Here are some of the best shots from the Apollo program.
Our Lunar Reconnaissance Orbiter is up there right now, mapping the moon and capturing some spectacular high-resolution shots.
Make our Moon portal your base for further lunar exploration.
Check out the full version of ‘Ten Things to Know This Week’ HERE.
Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.
Lucy Reading-Ikkanda/Quanta Magazine; Source: Feryal Özel
December 13, 1965 – Truly spectacular images of our planet captured by the astronauts of Gemini 7 as they zoomed around the Earth. In this era when we receive a daily dose of awesomeness from hi-res cameras on the ISS and various satellites, it’s easy to take beautiful Earth images for granted. I will never cease to be amazed by the stunning photography produced during the Project Gemini missions.
(NASA/Arizona State University)
“5.) Are there galaxies moving away faster than the speed of light, and isn’t that forbidden? From our point of view, the space in between us and any distant point is expanding. The farther away something is, the faster it appears to recede from us. Even if the expansion rate were tiny, an object far enough away would eventually cross that threshold of any finite speed, since an expansion rate (a speed-per-distance) multiplied by a great enough distance will give you a speed as fast as you want. But this is okay in General Relativity! The law that nothing can travel faster than the speed of light only applies to an object’s motion through space, not to the expansion of space itself. In reality, the galaxies themselves only move around at speeds that are hundreds or thousands of km/s, much lower than the 300,000 km/s speed limit set by the speed of light. It’s the expansion of the Universe that causes this recession and the redshift, not a true galactic motion.”
The idea that the spatial fabric of the Universe itself is expanding, and that’s what’s behind the observed relationship between redshift and distance has long been controversial, and also long-misunderstood. After all, if more distant objects appear to recede more quickly, couldn’t there be a different explanation, like an explosion that flung many things outward? As it turns out, this isn’t a mere difference in interpretation, there are observations we can make that tell us the answer! The Universe is not expanding ‘into’ anything, despite what your intuition might tell you. The Hubble ‘constant’ isn’t actually a constant, but is rather decreasing as time goes on. The Universe looks like it’s going to expand forever, but even that scientific conclusion is subject to revision depending on what data shows in the future. And although 97% of the galaxies in the Universe are already unreachable, it isn’t a violation of relativity or a faster-than-light phenomenon that’s to blame.
Come learn the answers to five questions about the expanding Universe that many are too embarrassed to ask!
evosia Chasing auroras is much like living life: if you show up, always be prepared for the amazing to happen.
NGC 6960 (Western Veil nebula) & Horsehead Nebula and the Flame Nebula
by David Wills
For more content, Click Here and experience this XYHor in its entirety!Space...the Final Frontier. Let's boldly go where few have gone before with XYHor: Space: Astronomy & Spacefaring: the collection of the latest finds and science behind exploring our solar system, how we'll get there and what we need to be prepared for!
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