South Pole Of Jupiter Photographed By Voyager 1 on March 1, 1979

Young Stellar Grouping in Cygnus X

Cygnus X hosts many young stellar groupings. The combined outflows and ultraviolet radiation from the region’s numerous massive stars have heated and pushed gas away from the clusters, producing cavities of hot, lower-density gas.

In this 8-micron infrared image, ridges of denser gas mark the boundaries of the cavities. Bright spots within these ridges show where stars are forming today.

Credit: NASA/IPAC/MSX

Solar ❤

Neptune Clouds

This Voyager 2 high resolution color image, taken 2 hours before closest approach, provides obvious evidence of vertical relief in Neptune’s bright cloud streaks. 

Credit: NASA / Voyager 2

The Largest Black Hole Merger Of All-Time Is Coming, And Soon

“Over in Andromeda, the nearest large galaxy to the Milky Way, a number of unusual systems have been found.  One of them, J0045+41, was originally thought to be two stars orbiting one another with a period of just 80 days. When additional observations were taken in the X-ray, they revealed a surprise: J0045+41 weren’t stars at all.”

When you look at any narrow region of the sky, you don’t simply see what’s in front of you. Rather, you see everything along your line-of-sight, as far as your observing power can take you. In the case of the Panchromatic Hubble Andromeda Treasury, where hundreds of millions of stars were captured in impressive fashion, background objects thousands of times as distant can also be seen. One of them, J0045+41, was originally thought to be a binary star system that was quite tight: with just an 80 day orbital period. Follow-up observations in the X-ray, however, revealed that it wasn’t a binary star system after all, but an ultra-distant supermassive black hole pair, destined to merge in as little as 350 years. If we build the right observatory in space, we’ll be able to observe the entire inspiral-and-merger process for as long as we like!

Come get the full story, and some incredible pictures and visuals, on today’s Mostly Mute Monday!

2017 October 30

Orionid Meteors from Orion Image Credit & Copyright: Lu Shupei

Explanation: Meteors have been shooting out from the constellation of Orion. This was expected, as October is the time of year for the Orionids Meteor Shower. Pictured here, over a dozen meteors were caught in successively added exposures last weekend over Wulan Hada volcano in Inner Mongolia, China. The featured image shows multiple meteor streaks that can all be connected to a single small region on the sky called the radiant, here visible just above and to the left of the belt of Orion, The Orionids meteors started as sand sized bits expelled from Comet Halley during one of its trips to the inner Solar System. Comet Halley is actually responsible for two known meteor showers, the other known as the Eta Aquarids and visible every May. Next month, the Leonids Meteor Shower from Comet Tempel-Tuttle should also result in some bright meteor streaks.

∞ Source: apod.nasa.gov/apod/ap171030.html

(CNN) On October 19, the Pan-STARRS 1 telescope in Hawaii spotted something strange zooming through our solar system. It turned out to be a visitor from beyond our solar system, and it's unlike anything astronomers have seen before.

Hubble peeks inside a stellar cloud

These bright stars shining through what looks like a haze in the night sky are part of a young stellar grouping in one of the largest known star formation regions of the Large Magellanic Cloud (LMC), a dwarf satellite galaxy of the Milky Way. The image was captured by the NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2.

The stellar grouping is known to stargazers as NGC 2040 or LH 88. It is essentially a very loose star cluster whose stars have a common origin and are drifting together through space. There are three different types of stellar associations defined by their stellar properties. NGC 2040 is an OB association, a grouping that usually contains 10–100 stars of type O and B — these are high-mass stars that have short but brilliant lives. It is thought that most of the stars in the Milky Way were born in OB associations.

There are several such groupings of stars in the LMC, including one previously featured as a Hubble Picture of the Week. Just like the others, LH 88 consists of several high-mass young stars in a large nebula of partially ionised hydrogen gas, and lies in what is known to be a supergiant shell of gas called LMC 4.

Over a period of several million years, thousands of stars may form in these supergiant shells, which are the largest interstellar structures in galaxies. The shells themselves are believed to have been created by strong stellar winds and clustered supernova explosions of massive stars that blow away surrounding dust and gas, and in turn trigger further episodes of star formation.

The LMC is the third closest galaxy to our Milky Way. It is located some 160 000 light-years away, and is about 100 times smaller than our own.

This image, which shows ultraviolet, visible and infrared light, covers a field of view of approximately 1.8 by 1.8 arcminutes.

A version of this image was entered into the Hubble’s Hidden Treasures Image Processing Competition by contestant Eedresha Sturdivant. Hidden Treasures is an initiative to invite astronomy enthusiasts to search the Hubble archive for stunning images that have never been seen by the general public.

These bright stars shining through what looks like a haze in the night sky are part of a young stellar grouping in one of the largest known star formation regions of the Large Magellanic Cloud (LMC), a dwarf satellite galaxy of the Milky Way. The image was captured by the NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2.

The stellar grouping is known to stargazers as NGC 2040 or LH 88. It is essentially a very loose star cluster whose stars have a common origin and are drifting together through space. There are three different types of stellar associations defined by their stellar properties. NGC 2040 is an OB association, a grouping that usually contains 10–100 stars of type O and B — these are high-mass stars that have short but brilliant lives. It is thought that most of the stars in the Milky Way were born in OB associations.

There are several such groupings of stars in the LMC, including one previously featured as a Hubble Picture of the Week. Just like the others, LH 88 consists of several high-mass young stars in a large nebula of partially ionised hydrogen gas, and lies in what is known to be a supergiant shell of gas called LMC 4.

Over a period of several million years, thousands of stars may form in these supergiant shells, which are the largest interstellar structures in galaxies. The shells themselves are believed to have been created by strong stellar winds and clustered supernova explosions of massive stars that blow away surrounding dust and gas, and in turn trigger further episodes of star formation.

The LMC is the third closest galaxy to our Milky Way. It is located some 160 000 light-years away, and is about 100 times smaller than our own.

This image, which shows ultraviolet, visible and infrared light, covers a field of view of approximately 1.8 by 1.8 arcminutes.

A version of this image was entered into the Hubble’s Hidden Treasures Image Processing Competition by contestant Eedresha Sturdivant. Hidden Treasures is an initiative to invite astronomy enthusiasts to search the Hubble archive for stunning images that have never been seen by the general public.

ESA/Hubble, NASA and D. A Gouliermis. Acknowledgement: Flickr user Eedresha Sturdivant

https://www.spacetelescope.org/images/potw

OSIRIS-REx view of Earth and Moon                      

This color composite image of Earth and the Moon was taken October 2, 2017, 10 days after OSIRIS-REx performed its Earth Gravity Assist maneuver, using MapCam, the mid-range scientific camera onboard the spacecraft. The distance to Earth was approximately 5,120,000 km—about 13 times the distance between the Earth and Moon.

MapCam, part of the OSIRIS-REx Camera Suite (OCAMS) operated by the University of Arizona, has four color filters. To produce this image, three of them (b, v and w) were treated as a blue-green-red triplet, co-registered and stacked. The Earth and Moon were each color-corrected, and the Moon was “stretched” (brightened) to make it more easily visible.

via: The Planetary Society

image: NASA / GSFC / University of Arizona

An irregular island

This image, courtesy of the NASA/ESA Hubble Space Telescope’s Advanced Camera for Surveys (ACS), captures the glow of distant stars within NGC 5264, a dwarf galaxy located just over 15 million light-years away in the constellation of Hydra (The Sea Serpent).

Dwarf galaxies like NGC 5264 typically possess around a billion stars — just one per cent of the number of stars found within the Milky Way. They are usually found orbiting other, larger, galaxies such as our own, and are thought to form from the material left over from the messy formation of their larger cosmic relatives.

NGC 5264 clearly possesses an irregular shape — unlike the more common spiral or elliptical galaxies — with knots of blue star formation. Astronomers believe that this is due to the gravitational interactions between NGC 5264 and other galaxies nearby. These past flirtations sparked the formation of new generations of stars, which now glow in bright shades of blue.

https://www.spacetelescope.org/images/potw

The NASA Village

Today in the NASA Village… Making More with Less

Stacey Boland works at NASA’s Jet Propulsion Laboratory (JPL) on missions that use remote sensing instruments for Earth observation.  From space, we can learn so much about our changing environment here on Earth.

Maximizing science research requires finding creative and cost effective ways to do it!  Her team developed the ISS-RapidScat instrument using left over equipment NASA had in storage from a program launched in the 1990’s.  ISS-RapidScat is an external payload mounted to the outside of the Columbus module, part of the International Space Station. ISS-RapidScat measures ocean wind speed and direction to help track tropical cyclones and hurricanes. Stacey’s team was able to get a functioning piece of hardware for about a tenth the cost of a traditional “small” Earth science mission.

Stacey said, “It wasn’t easy, but it was worth it!  Working in the space program doesn’t require perfection - but it does require passion and hard work!  We work as a team here at NASA and everyone’s role is important.  We rely on each other to do our best, regardless of what part of the mission is “ours.”  All the parts need to work together for it to be a success and that takes teamwork and good communication!”

Stacey’s story represents how being creative in the NASA Village can really make a difference!

Where did Stacey get her hunger for space?  “When I was growing up, my dad and I would learn about each shuttle mission and then watch launches on TV together. It was fun learning about science and exploration together. Now, as a parent, I’m continuing on that tradition with my son”

“I was able to watch the SpaceX-4 launch in person with my mom, dad, husband, and son”, Stacy said. “It was absolutely incredible to share that experience with them.  My son still talks about it and has been practicing drawing rockets ever since. He often asks when we can go back to Florida to see another one!”

Experiencing a rocket launch in person is amazing.  Feeling the sound waves from the engines push against your body is quite a rush.  And when it is hardware you helped create, on its way into space, it makes that experience even more special.

Next time on the NASA Village… A visit to the NASA Village inspires a lifelong career.

Do you want more stories?  Find our NASA Villagers here!