Friday, August 19, 2022

Setting The Dark on Fire in Orion | ESO's APEX Telescope

Setting The Dark on Fire in Orion | ESO's APEX Telescope

An image from the Atacama Pathfinder Experiment (APEX) telescope in Chile shows a beautiful view of clouds of cosmic dust in the region of Orion. While these dense interstellar clouds seem dark and obscured in visible-light observations, APEX’s LABOCA camera can detect the heat glow of the dust and reveal the hiding places where new stars are being formed. The image shows the region around the reflection nebula NGC 1999 in visible light, with the APEX observations overlaid in brilliant orange tones that seem to set the dark clouds on fire.

Distance: 1,500 light years


Credit: European Southern Observatory (ESO)/APEX (MPIfR/ESO/OSO)/T. Stanke et al./Digitized Sky Survey 2

Release Date: January 23, 2013


#NASA #ESO #Astronomy #Space #Science #Stars #OrionNebula #Nebula #NGC1999 #Orion #Constellation #Cosmos #Universe #Telescopes #APEX #Chile #Europe #STEM #Education

Artemis I Moon Rocket Arrives at Launchpad for Flight Test | This Week @NASA

Artemis I Moon Rocket Arrives at Launchpad for Flight Test | This Week @NASA

Week of August 19, 2022: The move to the launchpad ahead of our Artemis I flight test, discussing priorities for national space activities, and cargo and science head home from the space station . . . a few of the stories to tell you about—This Week at NASA!


Credit: National Aeronautics and Space Administration (NASA) 

Duration: 3 minutes, 49 seconds

Release date: August 19, 2022


#NASA #ESA #Space #ISS #Moon #Artemis #ArtemisI #Orion #Spacecraft #SLS #Rocket #DeepSpace #Orion #Spacecraft #Astronauts #Science #Engineering #Technology #Exploration #SolarSystem #KennedySpaceCenter #Florida #UnitedStates #Europe #STEM #Education #HD #Video

NASA Artemis I Path to the Pad: The Spacecraft

NASA Artemis I Path to the Pad: The Spacecraft

Named after one of the largest constellations in the night sky, Orion is the name given to the spacecraft that will carry the first woman and first person of color to the Moon. However, before we fly astronauts aboard, the spacecraft, powered by our Space Launch System (SLS) rocket, will travel tens of thousands of miles on a flight test around the Moon. Watch as teams at NASA's Kennedy Space Center prepare Orion for that journey, outfitting the spacecraft with its necessary components as it moves along its path to the pad.

All about Artemis I: https://www.nasa.gov/specials/artemis-i/


Writer: Danielle Sempsrott 

Editor: Francisco Martin

Producers: John Sackman, Michael Justice & Madison Tuttle

Credit: National Aeronautics and Space Administration (NASA) 

Duration: 10 minutes

Release Date: August 19, 2022


#NASA #ESA #Space #Moon #MSFC #Artemis #ArtemisI #Orion #Spacecraft #SLS #NASASLS #SpaceLaunchSystem #Rocket #DeepSpace #Astronauts #Mars #MoonToMars #JourneyToMars #Science #Engineering #Technology #Exploration #SolarSystem #UnitedStates #Europe #STEM #Education #HD #Video

NASA Artemis III Moon Mission: Candidate Regions for Landing Humans

NASA Artemis III Moon Mission: Candidate Regions for Landing Humans

Shown here is a rendering of 13 candidate landing regions for Artemis III. Each region is approximately 9.3 by 9.3 miles (15 by 15 kilometers). A landing site is a location within those regions with an approximate 328-foot (100-meter) radius.

As NASA prepares to send astronauts back to the Moon under Artemis, the agency has identified 13 candidate landing regions near the lunar South Pole. Each region contains multiple potential landing sites for Artemis III, which will be the first of the Artemis missions to bring crew to the lunar surface, including the first woman to set foot on the Moon.

NASA identified the following candidate regions for an Artemis III lunar landing:

Faustini Rim A

Peak Near Shackleton

Connecting Ridge

Connecting Ridge Extension

de Gerlache Rim 1

de Gerlache Rim 2

de Gerlache-Kocher Massif

Haworth

Malapert Massif

Leibnitz Beta Plateau

Nobile Rim 1

Nobile Rim 2

Amundsen Rim

Each of these regions is located within six degrees of latitude of the lunar South Pole and, collectively, contain diverse geologic features. Together, the regions provide landing options for all potential Artemis III launch opportunities. Specific landing sites are tightly coupled to the timing of the launch window, so multiple regions ensure flexibility to launch throughout the year.

To select the regions, an agencywide team of scientists and engineers assessed the area near the lunar South Pole using data from NASA’s Lunar Reconnaissance Orbiter and decades of publications and lunar science findings. In addition to considering launch window availability, the team evaluated regions based on their ability to accommodate a safe landing, using criteria including terrain slope, ease of communications with Earth, and lighting conditions. To determine accessibility, the team also considered combined capabilities of the Space Launch System rocket, the Orion spacecraft, and the SpaceX-provided Starship human landing system.

All regions considered are scientifically significant because of their proximity to the lunar South Pole, which is an area that contains permanently shadowed regions rich in resources and in terrain unexplored by humans.

The analysis team weighed other landing criteria with specific Artemis III science objectives, including the goal to land close enough to a permanently shadowed region to allow crew to conduct a moonwalk, while limiting disturbance when landing. This will allow crew to collect samples and conduct scientific analysis in an uncompromised area, yielding important information about the depth, distribution, and composition of water ice that was confirmed at the Moon’s South Pole.

The team identified regions that can fulfill the moonwalk objective by ensuring proximity to permanently shadowed regions, and also factored in other lighting conditions. All 13 regions contain sites that provide continuous access to sunlight throughout a 6.5-day period – the planned duration of the Artemis III surface mission. Access to sunlight is critical for a long-term stay at the Moon because it provides a power source and minimizes temperature variations.

NASA will discuss the 13 regions with broader science and engineering communities through conferences and workshops to solicit input about the merits of each region. This feedback will inform site selections in the future, and NASA may identify additional regions for consideration. The agency will also continue to work with SpaceX to confirm Starship’s landing capabilities and assess the options accordingly.

NASA will select sites within regions for Artemis III after it identifies the mission’s target launch dates, which dictate transfer trajectories and surface environment conditions.

Through Artemis, NASA will land the first woman and the first person of color on the Moon, paving the way for a long-term, sustainable lunar presence and serving as a steppingstone for future astronaut missions to Mars.

For more information on Artemis, visit: https://www.nasa.gov/specials/artemis/


Credit: National Aeronautics and Space Administration (NASA)

Release Date: August 19, 2022


#NASA #Space #Moon #LunarSouthPole #Artemis #ArtemisIII #HLS #HumanLandingSites #Topography #Astronauts #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #GSFC #USRA #UnitedStates #HumanSpaceflight #Infographic #STEM #Education

NASA Artemis III Moon Mission: Human Landing—South Pole Region Candidates

NASA Artemis III Moon Mission: Human LandingSouth Pole Region Candidates

NASA has announced the selection of 13 regions near the Moon's South Pole as candidates for the landing site of the Artemis III mission—the first crewed mission to the Moon's surface since 1972. This video features a data visualization showing the locations of all 13 regions, and highlights the interesting lunar topography and exploration potential of these areas.


Credit: NASA’s Goddard Space Flight Center

Video Produced & Edited by: David Ladd (AIMM)

Visualizations by: Ernie Wright (USRA)

LRO spacecraft animations by: Adriana Manrique Gutierrez (KBRwyle)

Orion/Artemis I animation by: Liam Yanulis

Narration by: Lauren Ward (KBRwyle)

Duration: 2 minutes

Release Date: Aug 19, 2022


#NASA #Space #Moon #LunarSouthPole #Artemis #ArtemisIII #HLS #HumanLandingSites #Topography #Astronauts #MoonToMars #Science #Engineering #Technology #Exploration #SolarSystem #GSFC #USRA #UnitedStates #HumanSpaceflight #STEM #Education #Visualization #HD #Video

NASA's Space to Ground: A Critical Steppingstone | Week of August 19, 2022

NASA's Space to Ground: A Critical Steppingstone | Week of August 19, 2022

NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station. At 11:00 a.m. on August 19, 2022, EDT, flight controllers on the ground sent commands to release the uncrewed SpaceX Dragon spacecraft from the forward port of the International Space Station’s Harmony module. At the time of release at 11:05 a.m., the station was flying about 259 miles over the Pacific Ocean. The Dragon spacecraft successfully departed the space station one month after arriving at the orbiting laboratory to deliver about 4,000 pounds of scientific investigations and supplies.

Tomorrow, ground controllers at SpaceX in Hawthorne, California, will command a deorbit burn. After re-entering Earth’s atmosphere, the spacecraft will make a parachute-assisted splashdown off the coast of Florida. NASA TV will not broadcast the de-orbit burn and splashdown.

During a four-hour and one-minute spacewalk on Wednesday, August 17, 2022, Commander Oleg Artemyev and Flight Engineer Denis Matveev installed a pair of cameras on the European robotic arm (ERA) and removed parts attached to the arm’s end effector. On Thursday, the cosmonauts powered down their Orlan spacesuits and removed suit components. Flight Engineer Sergey Korsakov reconfigured the Poisk module back to normal operations.

Just over two hours after Thursday’s spacewalk began, Artemyev informed Russian mission controllers his spacesuit was experiencing abnormal battery readings. Mission controllers directed Artemyev to return to the Poisk’s airlock and connect his spacesuit to the station’s power supply. Matveev continued his tasks before cleaning up and heading back to Poisk after managers called off the robotic maintenance excursion. Korsakov maneuvered the ERA to a safe post-spacewalk configuration while the cosmonaut spacewalkers were never in any danger.

Expedition 67 Crew

Commander Oleg Artemyev (Russia)

Roscosmos Flight Engineers: Denis Matveev and Sergey Korsakov (Russia)

NASA Flight Engineers: Kjell Lindgren, Bob Hines, Jessica Watkins (USA)

European Space Agency (ESA) Flight Engineer: Samantha Cristoforetti (Italy)

An international partnership of space agencies provides and operates the elements of the  International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada. The ISS has been the most politically complex space exploration program ever undertaken.


Credit: NASA's Johnson Space Center (JSC)

Release Date: August 19, 2022

Duration: 3 minutes, 23 seconds


#NASA #Space #Earth #ISS #SpaceX #SpaceXDragon #SpaceXCRS25 #Spacecraft #Cosmonauts #Astronauts #Europe #Italia #Italy #Canada #Japan #日本 #Russia #Россия #Science #Research #International #Expedition67 #STEM #Education #HD #Video

The Sombrero Galaxy in 60 Seconds | NASA's Chandra X-ray Observatory

The Sombrero Galaxy in 60 Seconds | NASA's Chandra X-ray Observatory

Like the Milky Way, Sombrero is a spiral galaxy. However, we see Sombrero edge-on from our vantage point from Earth, rather than the face-down perspective that is more familiar.

We begin with the Hubble Space Telescope’s optical light view of the Sombrero galaxy, also known as M104. Sombrero is one of the largest galaxies in the nearby Virgo cluster, about 30 million light years from Earth. Some of the prominent features of the Sombrero, which are highlighted in Hubble’s image, include its large bulge of stars in the center and the thick band of dust that appears as the dark lane across the galaxy’s mid-section. Like the Milky Way, Sombrero is a spiral galaxy. However, we see Sombrero edge-on from our vantage point from Earth, rather than the face-down perspective that is more familiar. A Great Observatories view of the same Sombrero reveals different aspects of the galaxy. 

The X-ray image from the Chandra X-ray Observatory shows hot gas in the galaxy that appears as a diffuse glow that extends over 60,000 light years from the Sombrero’s center. Also, Chandra detects many point-like sources of X-ray emission that are mostly stars within Sombrero but some are quasars in the distant background. The rim of dust that blocks the starlight in the Hubble image glows brightly in the Spitzer Space Telescope’s infrared image. Also, the central bulge of stars strongly emits infrared emission detected by Spitzer.


Credit: NASA/Chandra X-ray Center (CXC)

Narrator: Megan Watzke, CXC

Duration: 1 minute, 45 seconds

Release Date: May 29, 2008


#NASA #Astronomy  #Space #Science #Stars #Galaxy #Spiral #SombreroGalaxy #Messier104 #M104 #NGC4594 #Virgo #Constellation #Cosmos #Universe #Xray #Chandra #Observatory #MSFC #UnitedStates #STEM #Education #HD #Video

The Sombrero Galaxy: Infrared View | Hubble

The Sombrero Galaxy: Infrared View | Hubble & Spitzer


NASA/European Space Agency Hubble Space Telescope and NASA's Spitzer Space Telescope joined forces to create this striking composite image of one of the most popular sights in the universe. Messier 104 is commonly known as the Sombrero galaxy because in visible light, it resembles the broad-brimmed Mexican hat. However, in Spitzer's striking infrared view, the galaxy looks more like a "bull's eye."

Spitzer's full view shows the disk is warped, which is often the result of a gravitational encounter with another galaxy, and clumpy areas spotted in the far edges of the ring indicate young star-forming regions.

The Sombrero galaxy is located some 30 million light-years away. Viewed from Earth, it is just six degrees south of its equatorial plane. Spitzer detected infrared emission not only from the ring, but from the center of the galaxy too, where there is a huge black hole, believed to be a billion times more massive than our Sun.

The Spitzer picture is composed of four images taken at 3.6 (blue), 4.5 (green), 5.8 (orange), and 8.0 (red) microns. The contribution from starlight (measured at 3.6 microns) has been subtracted from the 5.8 and 8-micron images to enhance the visibility of the dust features.


Credit: NASA/JPL-Caltech and The Hubble Heritage Team (STScI/AURA)

Release Date: October 2, 2003


#NASA #ESA #Hubble #Spitzer #Astronomy #Space #Science #Stars #Galaxy #Infrared #SombreroGalaxy #Messier104 #M104 #NGC4594 #Virgo #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #AURA #UnitedStates #Europe #STEM #Education

The Fine Shades of The Sombrero Galaxy | ESO

The Fine Shades of The Sombrero Galaxy | ESO


Image of the famous early-type spiral galaxy Messier 104, widely known as the "Sombrero" (the Mexican hat) because of its particular shape. The "Sombrero" is located in the constellation Virgo (The Virgin), at a distance of about 30 million light-years.

Messier 104 is the 104th object in the famous catalogue of nebulae by French astronomer Charles Messier (1730 - 1817). It was not included in the first two editions (with 45 objects in 1774; 103 in 1781), but Messier soon thereafter added it by hand in his personal copy as a "very faint nebula". The recession velocity, about 1000 km/sec, was first measured by American astronomer Vesto M. Slipher at the Lowell Observatory in 1912; he was also the first to detect the galaxy's rotation.

This galaxy is notable for its dominant nuclear bulge, composed primarily of mature stars, and its nearly edge-on disc composed of stars, gas, and intricately structured dust. The complexity of this dust, and the high resolution of this image, is most apparent directly in front of the bright nucleus, but is also very evident as dark absorbing lanes throughout the disc. A significant fraction of the galaxy disc is even visible on the far side of the source, despite its massive bulge.

A large number of small and slightly diffuse sources can be seen as a swarm in the halo of Messier 104. Most of these are globular clusters, similar to those found in our own Galaxy.

This picture was obtained with FORS1 multi-mode instrument at VLT ANTU on January 30, 2000. It is a composite of three exposures in different wavebands. North is up and East is left.

Technical information : This composite image is based on three exposures from the FORS1 instrument at VLT ANTU. They were obtained at about 6:20 hrs UT on January 30, 2000, through V-band (central wavelength 554 nm; 112 nm Full Width Half Maximum (FWHM); exposure time 120 sec; here rendered as blue), R-band (657 nm; 150 nm FWHM; 120 sec; green) and I-band (768 nm; 138 nm FWHM, 240 sec; red). The seeing was 0.6–0.7 arcseconds.


Credit: European Southern Observatory (ESO)/P. Barthel

Acknowledgments: Mark Neeser (Kapteyn Institute, Groningen) and Richard Hook (ST/ECF, Garching, Germany)

Release Date: February 23, 2000


#NASA #ESO #Astronomy #Space #Science #Stars #Galaxy #SombreroGalaxy #Messier104 #M104 #NGC4594 #Virgo #Constellation #Cosmos #Universe #Telescopes #VLT #FORS1 #Chile #Europe #STEM #Education

Zoom into The Sombrero Galaxy | Hubble

Zoom into The Sombrero Galaxy | Hubble

The Sombrero Galaxy (also known as Messier Object 104, M104 or NGC 4594) is a peculiar galaxy in the constellation borders of Virgo and Corvus, It has a diameter of approximately 15 kiloparsecs (49,000 light-years), three-tenths the size of the Milky Way.

Distance: 30 million light years


Credit: NASA and G. Bacon (STScI)

Duration: 41 seconds

Release Date: December 31, 2014


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #Galaxy #SombreroGalaxy #Messier104 #M104 #NGC4594 #Virgo #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #AURA #UnitedStates #Europe #STEM #Education #HD #Video

The Sombrero Galaxy | Hubble

The Sombrero Galaxy | Hubble


NASA/European Space Agency Hubble Space Telescope has trained its razor-sharp eye on one of the universe's most stately and photogenic galaxies, the Sombrero galaxy, Messier 104 (M104). The galaxy's hallmark is a brilliant white, bulbous core encircled by the thick dust lanes comprising the spiral structure of the galaxy. As seen from Earth, the galaxy is tilted nearly edge-on. We view it from just six degrees north of its equatorial plane. This brilliant galaxy was named the Sombrero because of its resemblance to the broad rim and high-topped Mexican hat.

At a relatively bright magnitude of +8, M104 is just beyond the limit of naked-eye visibility and is easily seen through small telescopes. The Sombrero lies at the southern edge of the rich Virgo cluster of galaxies and is one of the most massive objects in that group, equivalent to 800 billion suns. The galaxy is 50,000 light-years across and is located 30 million light-years from Earth.


Credit: NASA/European Space Agency and The Hubble Heritage Team (STScI/AURA)

Release Date: October 2, 2004


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #Galaxy #SombreroGalaxy #Messier104 #M104 #NGC4594 #Virgo #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #AURA #UnitedStates #Europe #STEM #Education

Thursday, August 18, 2022

NASA's Mars Curiosity Rover: New August 2022 Images | JPL

NASA's Mars Curiosity Rover: New August 2022 Images | JPL


MSL - sol 3564 - Mastcam


MSL - sol 3565 - Mastcam


MSL - sol 3564 - Mastcam


MSL - sol 3565 - Mastcam


MSL - sol 3564 - MAHLI

MSL - sol 3564 - MAHLI


Mission Name: Mars Science Laboratory (MSL)

Rover Name: Curiosity

Main Job: To determine if Mars was ever habitable to microbial life. 

Launch: Nov. 6, 2011

Landing Date: Aug. 5, 2012, Gale Crater, Mars


For more information on NASA's Mars missions, visit: mars.nasa.gov


Image Credit: NASA/JPL-Caltech/MSSS/Kevin M. Gill

Image Release Dates: August 16-18, 2022


#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #MountSharp #GaleCrater #CuriosityRover #Curiosity #Rover #Robotics #Technology #Engineering #JPL #California #UnitedStates #JourneyToMars #CitizenScience #STEM #Education

View of The Running Chicken Nebula from South America | ESO

View of The Running Chicken Nebula from South America | ESO

The most obvious deep-sky objects in this image include the Carina Nebula, glowing intensely red in the middle of the image. The Carina Nebula lies in the constellation of Carina (The Keel), about 7,500 light-years from Earth. This cloud of glowing gas and dust is the brightest nebula in the sky and contains several of the brightest and most massive stars known in the Milky Way, such as Eta Carinae. The Carina Nebula is a perfect test-bed for astronomers to unveil the mysteries of the violent birth and death of massive stars. 

Below the Carina Nebula, we see the Wishing Well Cluster (NGC 3532). This open cluster of young stars was named because, through a telescope’s eyepiece, it looks like a handful of silver coins twinkling at the bottom of a wishing well. Further to the right, we find the Running Chicken Nebula (IC 2944), from a bird-like shape that some people see in its brightest region. Above this nebula and slightly to the left we find the Southern Pleiades (IC 2632), an open cluster of stars that is similar to its more familiar northern namesake.

In the foreground, we see three of the four Auxiliary Telescopes (ATs) of the Very Large Telescope Interferometer (VLTI). Using the VLTI, the ATs—or the VLT’s 8.2-meter Unit Telescopes—can be used together as a single giant telescope which can see finer details than would be possible with the individual telescopes. The VLTI has been used for a broad range of research including the study of circumstellar discs around young stellar objects and of active galactic nuclei, one of the most energetic and mysterious phenomena in the Universe.


Credit: European Southern Observatory (ESO)/B. Tafreshi

Release Date: November 12, 2012


#NASA #ESO #Astronomy #Space #Science #Stars #Nebula #EmissionNebula #IC2944 #RunningChickenNebula #Centaurus #Constellation #Cosmos #Universe #Telescopes #VLT #VLTI #Astrophotography #Chile #Europe #STEM #Education

The Running Chicken Nebula | ESO

The Running Chicken Nebula | ESO


This new image from the Wide Field Imager on the MPG/ESO 2.2-meter telescope shows the Running Chicken Nebula, a cloud of gas and newborn stars that lies around 6,500 light-years away from us in the constellation of Centaurus (The Centaur). Officially called IC 2944, or the Lambda Centauri Nebula, its strange nickname comes from the bird-like shape of its brightest region. The star Lambda Centauri itself lies just outside the field of view.


Credit: European Southern Observatory (ESO)

Release Date: September 21, 2011


#NASA #ESO #Astronomy #Space #Science #Stars #Nebula #EmissionNebula #IC2944 #RunningChickenNebula #LambdaCentauri #BokGlobules #Centaurus #Constellation #Cosmos #Universe #Telescope #Chile #Europe #STEM #Education

Thackeray's Globules in The Running Chicken Nebula | Hubble

Thackeray's Globules in The Running Chicken Nebula | Hubble


Strangely glowing dark clouds float serenely in this remarkable and beautiful image taken with the Hubble Space Telescope. These dense, opaque dust cloudsknown as 'globules'are silhouetted against nearby bright stars in the busy star-forming region, IC 2944, also known as the Running Chicken Nebula. 

Astronomer A.D. Thackeray first spied the globules in IC 2944 in 1950. Globules like these have been known since Dutch-American astronomer Bart Bok first drew attention to such objects in 1947.

However, astronomers still know very little about their origin and nature, except that they are generally associated with areas of star formation, called 'HII regions' due to the presence of hydrogen gas. IC 2944 is filled with gas and dust that is illuminated and heated by a loose cluster of massive stars. These stars are much hotter and much more massive than our Sun.


Credit: NASA/European Space Agency and The Hubble Heritage Team (STScI/AURA)

Release Date: January 3, 2002


#NASA #ESA #Hubble #Astronomy #Space #Science #Stars #Nebula #EmissionNebula #IC2944 #RunningChickenNebula #BokGlobules #ThackeraysGlobules #Centaurus #Constellation #MilkyWay #Galaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #AURA #UnitedStates #Europe #STEM #Education

A Close-up Look at The Running Chicken Nebula & Thackeray's Globules | ESO

A Close-up Look at The Running Chicken Nebula & Thackeray's Globules | ESO

This video gives us a close-up look at the spectacular stellar nursery IC 2944, also known as the Running Chicken Nebula. This image also shows a group of thick clouds of dust known as the Thackeray globules silhouetted against the pale pink glowing gas of the nebula. These globules are under fierce bombardment from the ultraviolet radiation from nearby hot young stars. They are both being eroded away and also fragmenting, rather like lumps of butter dropped onto a hot frying pan. It is likely 

Distance: 6,500 light years

This image was released to celebrate a milestone—15 years of the European Southern Observatory's VLT. 


Credit: European Southern Observatory (ESO)

Duration: 56 seconds

Release Date: May 23, 2013


#NASA #ESO #Astronomy #Space #Science #Stars #Nebula #EmissionNebula #IC2944 #RunningChickenNebula #LambdaCentauri #BokGlobules #Centaurus #Constellation #Cosmos #Universe #Telescope #VLT #ParanalObservatory #Chile #Europe #STEM #Education #HD #Video