mercredi 1 juin 2016

NASA Hurricane Resources Available for 2016 Atlantic Hurricane Season














NASA & NOAA - Suomi NPP Mission logo / NASA & JAXA - GPM Mission logo.

June 1, 2016

NASA has a variety of resources for reporters covering 2016's Atlantic Ocean and Eastern and Central Pacific hurricane seasons, including scientific animations in a resource reel that look inside hurricanes and daily updates with satellite data.


Image above: NASA-NOAA's Suomi NPP satellite provided this visible look at Hurricane Alex at 9:20 a.m. EST (14:20 UTC) on Jan. 15 while it was moving over the Azores. Image Credits: NASA/NOAA/Jeff Schmaltz.

The Atlantic Ocean hurricane season begins June 1 and runs through Nov. 30. This year, activity in the Atlantic basin began unusually early, with the development in January of Hurricane Alex in the eastern Atlantic. Alex officially became a hurricane on Jan. 14, 2016 and the National Hurricane Center said it was the earliest hurricane to form in the Atlantic since 1938. Like the Atlantic, activity in the Central Pacific started early when the first tropical cyclone, Pali, developed in January and on the 11th became the earliest hurricane ever recorded. NASA satellite imagery on NASA's Hurricane page covered both storms from birth to death. The NASA Hurricane page has covered all worldwide tropical cyclones in every ocean basin since 2005.


Image above: The GPM core observatory satellite flew over Pali on Jan. 11 at 4:21 p.m. EST (21:21 UTC). GPM's Dual-Frequency Precipitation Radar (DPR) data sliced through Pali clearly showing that an eye had formed. Image Credits: NASA/JAXA/SSAI, Hal Pierce.

NASA satellites provide information such as cloud and sea-surface temperatures, rainfall locations and rates of rainfall within each storm, cloud extent, and even surface winds. All of that information is used to create daily hurricane updates and has been used in animations. The nearly hour-long online "Hurricane Resource Reel" is housed at the website for the Scientific Visualization Studio of NASA's Goddard Space Flight Center in Greenbelt, Maryland. It includes storms from various oceans around the world. There is also a gallery of hurricane and typhoon animations, and another about NASA/Japan Aerospace Exploration Agency’s Global Precipitation Measurement (GPM) mission, IMERG rainfall data and 3-D storm animations. 

Related links:

Hurricane Alex in the eastern Atlantic: http://www.nasa.gov/feature/goddard/2016/alex-atlantic-ocean

Global Precipitation Measurement (GPM): https://svs.gsfc.nasa.gov/Gallery/GPM.html and http://global.jaxa.jp/projects/sat/gpm/

NASA-NOAA's Suomi NPP: http://www.nasa.gov/mission_pages/NPP/main/index.html and http://www.jpss.noaa.gov/satellites.html

To learn more about NASA's new hurricane research mission, the Cyclone Global Navigation Satellite System, or CYGNSS mission, visit: http://www.nasa.gov/cygnss/overview

For NASA's Hurricane Resource Reel: http://svs.gsfc.nasa.gov/Gallery/HurricanesandTyphoons.html

For NASA's Hurricane page, visit: http://www.nasa.gov/hurricane

Images (mentioned), Text, Credits: NASA's Goddard Space Flight Center/Rob Gutro/Ashley Morrow.

Greetings, Orbiter.ch

Gemini IX Crew Found 'Angry Alligator' in Earth Orbit









NASA - Gemini IX Mission patch.

June 1, 2016

NASA's Gemini IX mission was another step in developing technology for future spaceflights from Apollo to the agency's Journey to Mars. But this mission included developing alternate plans when faced with the unexpected.


Image above: An Augmented Target Docking Adapter, or ATDA, launches atop an Atlas rocket from Cape Kennedy Air Force Station's Launch Complex 14 on June 1, 1966. The ATDA served as a rendezvous target for Gemini IXA. Image Credit: NASA.

Gemini IX provided NASA with crucial experience in learning how to be flexible, expanding skills in orbital rendezvous and gaining a better understanding of the challenges faced by spacewalking astronauts.

The three-day mission was designed to be similar to the previous flight in March 1966. After achieving the first orbital docking, Gemini VIII was brought home early due to a failed spacecraft thruster. The Gemini IX crew hoped to gain further experience in rendezvous, docking and working outside the capsule. Plans also called for performing a complex spacewalk using a self-contained rocket backpack, called the Astronaut Maneuvering Unit, or AMU.

The original Gemini IX command pilot was scheduled to be Elliot See, with Charles Bassett as pilot. They were both killed on Feb. 28, 1966, when their T-38 jet crashed into the McDonnell Aircraft plant in St. Louis, where assembly of their spacecraft was being completed.

The backup crew of Tom Stafford as command pilot and Eugene Cernan as pilot then were named for the upcoming flight. A veteran of Gemini VI the previous year, Stafford would go on to command Apollo 10 in 1969 and the Apollo-Soyuz mission in 1975.


Image above: After two postponements, Gemini IXA astronauts Eugene Cernan, left, and Tom Stafford, center, arrive in the white room atop Launch Pad 19 at Cape Kennedy Air Force Station on June 3, 1966. Stafford is presenting a large match to McDonnell Aircraft Corporation's pad leader Gunter Wendt, far right. Stafford "instructed" Wendt in jest to "light the fuse today." Between Stafford and Wendt are the backup crew, Buzz Aldrin and Jim Lovell. The Gemini spacecraft did lift off later that morning atop a Titan II rocket. Image Credit: NASA.

Cernan was lunar module pilot with Stafford on Apollo 10 and commanded the final moon landing mission, Apollo 17, in December 1972.

Gemini IX's Agena target vehicle was launched by an Atlas rocket on May 17, 1966. Stafford and Cernan were already aboard their spacecraft poised to lift off 90 minutes later as the Agena competed its first orbit. However, the Atlas malfunctioned in flight, and the Agena failed to reach orbit.

Launch of Gemini IX would have to wait.

Even so, Dr. George Mueller, NASA associate administrator for Manned Space Flight, had high praise for the launch team, noting that the simultaneous countdowns at Cape Kennedy Air Force Station's Launch Complexes 14, for the Atlas-Agena, and 19, for the Gemini-Titan, had been the "smoothest yet in the Gemini Program."

While the next Agena would not be available until summer, NASA had a backup rendezvous target available, called an Augmented Target Docking Adapter, or ATDA. Additionally, the mission was redesigned Gemini IXA.

"We had a flexible flight plan allowing us to shift around items and that's exactly what happened," said Stafford.

The contingency target vehicle was developed after an Agena failed to reach orbit for the original Gemini VI mission. This spacecraft would allow Gemini flights to continue without delaying the goal of landing on the moon before the end of the decade of the 1960s.

The ATDA was built by the McDonnell Corp., prime contractor for the Gemini spacecraft. The ATDA used a Gemini spacecraft re-entry control section and other already proven equipment. Like the Agena, it was launched atop an Atlas rocket on June 1, 1966, and successfully reached an orbit 161 miles above the Earth.

However, telemetry soon indicated more unexpected news. The conical nosecone shroud at the top of the ATDA appeared not to have separated. If that was the case, docking would be impossible as the shroud covered the target vehicle's docking collar.


Image above: The Augmented Target Docking Adapter, or ATDA, as seen from the Gemini IXA spacecraft during one of their three rendezvous in Earth orbit. Failure of the docking adapter protective cover to fully separate on the ATDA prevented the docking of the two spacecraft. As a result, command pilot Tom Stafford described the ATDA as looking like an "angry alligator." Image Credit: NASA.

After a two-day delay, Stafford and Cernan were launched on June 3, and they would soon learn the condition of the shroud.

Stafford fired his thrusters 49 minutes after liftoff to begin closing in on the ATDA. Radar contact was achieved when the two space vehicles were 150 miles apart. Stafford and Cernan spotted the ATDA at three hours, 20 minutes into the mission, when they were 58 miles away.

As they closed in, Stafford began to describe what they saw.

"We've got the ATDA in reflected moonlight at about 3 1/2 miles," he said.

As they closed in at about 900 feet, Stafford reported his first good view of the ATDA.

"That's a weird looking machine," he said. "Would you believe that there's a nose cone on that rascal. The shroud is half open. It looks like an angry alligator out there rotating around."

The shroud was supposed to open in two halves and drop away during launch. It split in two, but was hung up at the base. While the rendezvous was successful, the alligator-like "jaws" would prevent docking unless there was a way to push it aside.

"You could almost knock it off," Cernan said.

Stafford suggested to spacecraft communicator Neil Armstrong in Mission Control Houston that they be allowed to extend a docking guide bar on the nose of the Gemini to gently bump the shroud in an attempt to knock it off.


Image above: Shortly after reaching orbit on June 3, 1966, Gemini IXA command pilot Tom Stafford is seen at the controls during the mission to rendezvous with an Augmented Target Docking Adapter. Image Credits: NASA/Eugene Cernan.

Armstrong, who commanded the previous flight, relayed word that Flight Director Eugene Kranz vetoed the idea as too risky.

While the docking was ruled out, Stafford and Cernan gained valuable experience and data on different approaches to rendezvous, a maneuver that would be crucial as Apollo astronauts in a lunar module returned to the command module after exploring the moon.

Gemini IXA preformed a second rendezvous moving away from the ATDA and then successfully completed an approach from below. It also was the first pure optical rendezvous.

"Gene made all the computations and we did not use the computer," Stafford said. "We wanted to test how good man can visually judge distance."

This required learning how to best interpret visual cues.

"We had anticipated that silver paint (on the ATDA) actually would be almost equivalent to white in visual acquisition, but it certainly was not," Cernan said. "We could more easily see the white shroud in reflected moonlight."

At one point, the Gemini IXA crew used an onboard system to verify Stafford's estimation that they were about one mile from the ATDA.

"The radar said we were at 1.1 mile," he said. "It was obvious we could judge distance in close."

On flight day two, they approached the ATDA a third time, simulating a lunar module returning to the command module in lunar orbit. They learned that the rendezvous radar would be required for this approach.

Stafford then backed off from the target vehicle to prepare for the next day's ambitious spacewalk.


Image above: During his two hour, eight minute spacewalk on June 5, 1966, Gemini IXA pilot Eugene Cernan is seen outside the spacecraft. His experience during that time showed there was still much to be learned about working in microgravity. Image Credits: NASA/Tom Stafford.

During America's first spacewalk a year earlier, Gemini IV astronaut Ed White floated around for 20 minutes. Cernan planned more than two hours of task evaluations and work testing the AMU. It was equipped with propulsion, a stabilization system, oxygen and telemetry for biomedical data.

As Cernan floated through the Gemini hatch, he described what it is like being outside.

"Boy, is it beautiful out there, Tom," he said, "and what a beautiful spacecraft."

After his experience on Gemini IV, White recommended handholds to assist future spacewalkers. For Gemini IXA, Cernan tested Velcro for that purpose.

"I started using one of those Velcro pads and I lost it," Cernan said. "It came right off my hand. The Velcro's not strong enough."

Cernan then worked his way back to the aft section where the AMU was located. Once he reached the AMU in the spacecraft's adapter section, Cernan realized his spacesuit provided limited maneuverability. He was unable to gain any leverage for his planned tasks due to the lack of hand and foot holds. It also was difficult to turn valves and perform simple movements.

The extra effort caused the heat to rise in Cernan's spacesuit, and his increased respiration resulted in his helmet visor beginning to fog up.

"He's fogging real bad," said Stafford to officials in Mission Control. "The AMU controller arms presented far more difficulty to us in zero g than they did in the simulation."

With Cernan barely able to see, Stafford and mission control agreed to bring him back in after two hours and eight minutes outside the spacecraft.


Image above: "What a beautiful spacecraft," said Eugene Cernan during his spacewalk. He took this wide-angle photograph looking back at the window where Tom Stafford was watching. Image Credits: NASA/Eugene Cernan.

The next day, June 6, Stafford and Cernan fired Gemini's retro rockets on their 45th orbit of the Earth. They landed less than one mile from the prime recovery ship, the USS Wasp. It was the first time a spacecraft descending on its parachute was shown on live television.

The flight's lessons learned resulted in NASA mission planners adding even more flexibility into future flight plans. On Gemini IXA, Stafford and Cernan were able to work with flight controllers to demonstrate sophisticated rendezvous maneuvers were workable and applicable to Apollo and future space programs. Cernan's experiences on his spacewalk showed there still was much to be learned about working in microgravity outside a spacecraft.

"We came back with some data and recommendations on how to handle yourself when floating in close proximity to the spacecraft," Cernan said in the postflight news conference.


Image above: Gemini IXA splashes down in the Atlantic Ocean on June 6, 1966, less than one mile from the prime recovery ship, the aircraft carrier USS Wasp . It was the first time a spacecraft descending on its parachute was shown on live television. Image Credit: NASA.

As a result of Cernan's experience, important changes were made for planning future work outside a spacecraft, including adjustments to the workloads for future Gemini spacewalks. For Apollo moonwalks, the spacesuits were designed differently.

A Gemini spacesuit was cooled by air flow. Apollo spacesuits for moonwalkers and for those astronauts who work outside today's International Space Station would be cooled by having the astronaut wear an undergarment with small tubes circulating water near the skin.

EDITOR'S NOTE: This is the sixth in a series of feature articles marking the 50th anniversary of Project Gemini. The program was designed as a steppingstone toward landing on the moon. The investment also provided technology now used in NASA's work aboard the International Space Station and planning for the Journey to Mars. In July, read about an orbital rendezvous with two separate spacecraft. For more, see "On the Shoulders of Titans: A History of Project Gemini":
http://history.nasa.gov/SP-4203.pdf

For more information about Gemini Program, visit:

Gemini: https://www.nasa.gov/mission_pages/gemini/index.html

Gemini IX: https://www.nasa.gov/mission_pages/gemini/index.html

NASA History: https://www.nasa.gov/topics/history/index.html

Kennedy Space Center: https://www.nasa.gov/centers/kennedy/home/index.html

Images (mentioned), Text, Credits: NASA's Kennedy Space Center/Bob Granath.

Best regards, Orbiter.ch

Earth Monitoring CubeSats Released












ISS - Expedition 47 Mission patch.

June 1, 2016

More CubeSats are due to be deployed today contributing to humanitarian and environmental research. The crew is also continuing biomedical science to improve the health of astronauts in space and humans on Earth.

The final set of CubeSats will be released tonight from a small satellite deployer outside Japan’s Kibo laboratory module. This current fleet of 16 CubeSats, also known as Dove satellites, began deploying Monday and will monitor the Earth to help improve disaster relief and agriculture yields.


Image above: A CubeSat is deployed April 27 from a deployer on the outside of Kibo lab module. Image Credit: NASA.

The crew is exploring new space exercise techniques today to keep muscles, bones and the heart healthy during long-duration missions. The crew is also tracking its medication intake to determine the effectiveness and any side effects of using medicine in space.

BEAM, or the Bigelow Expandable Activity Module, is still undergoing temperature and pressure checks while some relief valves and ventilation valves are being swapped out. Astronaut Jeff Williams will enter BEAM for the first time next week to install sensors measuring the expandable module’s environment.

Related links:

CubeSats: http://www.nasa.gov/mission_pages/cubesats/index.html

New space exercise techniques: http://www.nasa.gov/mission_pages/station/research/experiments/972.html

Medicine in space: http://www.nasa.gov/mission_pages/station/research/experiments/1933.html

Bigelow Expandable Activity Module: http://www.nasa.gov/content/bigelow-expandable-activity-module

International Space Station (ISS): http://www.nasa.gov/mission_pages/station/main/index.html

Space Station Research and Technology: http://www.nasa.gov/mission_pages/station/research/index.html

Image (mentioned), Text, Credits: NASA/Mark Garcia.

Best regards, Orbiter.ch

Pluto’s Heart: Like a Cosmic ‘Lava Lamp’












NASA - New Horizons Mission logo.

June 1, 2016

Combining computer models with topographic and compositional data gathered by NASA’s New Horizons spacecraft last summer, New Horizons team members have determined the depth of this layer of solid nitrogen ice within Pluto's distinctive "heart" feature – a large plain informally known as Sputnik Planum – and how fast that ice is flowing. The study is published in the June 2 issue of the journal Nature.

Mission scientists used state-of-the-art computer simulations to show that the surface of Sputnik Planum is covered with icy, churning, convective "cells" 10 to 30 miles (16 to 48 kilometers) across, and less than one million years old. The findings offer additional insight into the unusual and highly active geology on Pluto and, perhaps, other bodies like it on the outskirts of the solar system.


Image above: Scientists from NASA’s New Horizons mission used state-of-the-art computer simulations to show that the surface of Pluto’s informally named Sputnik Planum is covered with churning ice "cells" that are geologically young and turning over due to a process called convection. The scene above, which is about 250 miles (400 kilometers) across, uses data from the New Horizons Ralph/Multispectral Visible Imaging Camera (MVIC), gathered July 14, 2015. Image Credits: NASA/JHUAPL/SwRI.

“For the first time, we can determine what these strange welts on the icy surface of Pluto really are,” said William B. McKinnon, from Washington University in St. Louis, who led the study and is a co-investigator on the New Horizons science team. “We found evidence that even on a distant cold planet billions of miles from Earth, there is sufficient energy for vigorous geological activity, as long as you have ‘the right stuff,’ meaning something as soft and pliable as solid nitrogen.”

McKinnon and colleagues believe the pattern of these cells stems from the slow thermal convection of the nitrogen-dominated ices that fill Sputnik Planum. A reservoir that’s likely several miles deep in some places, the solid nitrogen is warmed by Pluto’s modest internal heat, becomes buoyant and rises up in great blobs – like a lava lamp – before cooling off and sinking again to renew the cycle.

The computer models show that ice need only be a few miles deep for this process to occur, and that the convection cells are very broad. The models also show that these blobs of overturning solid nitrogen can slowly evolve and merge over millions of years. Ridges that mark where cooled nitrogen ice sinks back down can be pinched off and abandoned, resulting in Y- or X-shaped features in junctions where three or four convection cells once met.

“Sputnik Planum is one of the most amazing geological discoveries in 50-plus years of planetary exploration, and the finding by McKinnon and others on our science team that this vast area—bigger than Texas and Oklahoma combined – is created by current day ice convection is among the most spectacular of the New Horizons mission,” said New Horizons Principal Investigator Alan Stern, of the Southwest Research Institute, Boulder, Colorado. 

These convective surface motions average only a few centimeters a year – about as fast as your fingernails grow – which means cells recycle their surfaces every 500,000 years or so. While slow on human clocks, it’s a fast clip on geological timescales. 

“This activity probably helps support Pluto’s atmosphere by continually refreshing the surface of ‘the heart,’” McKinnon said. “It wouldn’t surprise us to see this process on other dwarf planets in the Kuiper Belt. Hopefully, we’ll get a chance to find out someday with future exploration missions there.”

New Horizons spacecraft. Image Credit: NASA

New Horizons could also potentially take a close-up look at a smaller, more ancient object much farther out in the Kuiper Belt – the disk-shaped region beyond the orbit of Neptune believed to contain comets, asteroids and other small, icy bodies. New Horizons flew through the Pluto system on July 14, 2015, making the first close observations of Pluto and its family of five moons. The spacecraft is on course for an ultra-close flyby of another Kuiper Belt object, 2014 MU69, on Jan. 1, 2019, pending NASA approval of funding for an extended mission.

For more information about New Horizons, visit: http://www.nasa.gov/mission_pages/newhorizons/main/index.html

Images (mentioned), Text, Credits: NASA/Tricia Talbert.

Greetings, Orbiter.ch

mardi 31 mai 2016

The Little Fox and the Giant Stars










NASA & ESA - Herschel Mission patch.

May 31, 2016


New stars are the lifeblood of our galaxy, and there is enough material revealed by this Herschel infrared image to build stars for millions of years to come.

Situated 8,000 light-years away in the constellation Vulpecula -- Latin for "little fox" -- the region in the image is known as Vulpecula OB1. It is a "stellar association" in which a batch of truly giant "OB" stars is being born. O and B stars are the largest stars that can form.

The giant stars at the heart of Vulpecula OB1 are some of the biggest in the galaxy. Containing dozens of times the mass of the sun, they have short lives, astronomically speaking, because they burn their fuel so quickly. At an estimated age of 2 million years, they are already well through their lifespans. When their fuel runs out, they will collapse and explode as supernovas. The shock this will send through the surrounding cloud will trigger the birth of even more stars, and the cycle will begin again.

O stars are at least 16 times more massive than the sun, and could be well over 100 times as massive. They are anywhere from 30,000 to 1 million times brighter than the sun, but they only live up to a few million years before exploding. B-stars are between two and 16 times as massive as the sun. They can range from 25 to 30,000 times brighter than the sun.

OB associations are regions with collections of O and B stars. Since OB stars have such short lives, finding them in large numbers indicates the region must be a strong site of ongoing star formation, which will include many more smaller stars that will survive far longer.

The vast quantities of ultraviolet light and other radiation emitted by these stars is compressing the surrounding cloud, causing nearby regions of dust and gas to begin the collapse into more new stars. In time, this process will "eat" its way through the cloud, transforming some of the raw material into shining new stars.

The image was obtained as part of Herschel's Hi-GAL key-project. This used the infrared space observatory's instruments to image the entire galactic plane in five different infrared wavelengths.

These wavelengths reveal cold material, most of it between -220º C and -260º C. None of it can be seen in ordinary optical wavelengths, but this infrared view shows astronomers a surprising amount of structure in the cloud's interior.

The surprise is that the Hi-GAL survey has revealed a spider's web of filaments that stretches across the star-forming regions of our galaxy. Part of this vast network can be seen in this image as a filigree of red and orange threads.

In visual wavelengths, the OB association is linked to a star cluster catalogued as NGC 6823. It was discovered by William Herschel in 1785 and contains 50 to 100 stars. A nebula emitting visible light, catalogued as NGC 6820, is also part of this multi-faceted star-forming region.

Herschel Space Observatory

Herschel is a European Space Agency mission, with science instruments provided by consortia of European institutes and with important participation by NASA. While the observatory stopped making science observations in April 2013, after running out of liquid coolant as expected, scientists continue to analyze its data. NASA's Herschel Project Office is based at NASA's Jet Propulsion Laboratory, Pasadena, California. JPL contributed mission-enabling technology for two of Herschel's three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the U.S. astronomical community. Caltech manages JPL for NASA.

More information is online at http://www.herschel.caltech.edu,http://www.nasa.gov/herschel and http://www.esa.int/SPECIALS/Herschel.
Hi-GAL key-project: https://hi-gal.ifsi-roma.inaf.it/higal/

Image, Text,  Credits: ESA/Herschel/PACS, SPIRE/Hi-GAL Project/Tony Greicius.

Greetings, Orbiter.ch

In Formation












NASA - Cassini Mission to Saturn patch.

May 31, 2016


Saturn's moons Janus and Mimas coast in their silent orbits beyond the rings in this view from NASA's & ESA's Cassini spacecraft. The ansa, or outer edge of the rings, is visible at left. Janus hangs above center, while Mimas shines at right. Owing to its irregular shape, Janus’ terminator – that line which separates day from night – is jagged, while Mimas’ smooth terminator belies its round shape and larger size.

The image was taken in green light with Cassini's narrow-angle camera on Oct. 27, 2015.

The view was acquired at a distance of approximately 598,000 miles (963,000 kilometers) from Janus and at a Sun-Janus-spacecraft, or phase, angle of 86 degrees. Image scale at Janus is 3.6 miles (5.8 kilometers) per pixel. The distance to Mimas was 680,000 miles (1.1 million kilometers) for an image scale of 4.1 miles (6.6 kilometer) per pixel.

The Cassini mission is a cooperative project of NASA, ESA (the European Space Agency) and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colorado.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini. The Cassini imaging team homepage is at http://ciclops.org and ESA's website: http://www.esa.int/Our_Activities/Space_Science/Cassini-Huygens

Image, Text, Credits: NASA/JPL-Caltech/Space Science Institute/Tony Greicius.

Greetings, Orbiter.ch

lundi 30 mai 2016

Born in a golden cloak












ESA - Hubble Space Telescope patch.

May 30, 2016


This young star is breaking out. Like a hatchling pecking through its shell, this particular stellar newborn is forcing its way out into the surrounding Universe.

The golden veil of light cloaks a young stellar object known only as IRAS 14568-6304. It is ejecting gas at supersonic speeds and eventually will have cleared a hole in the cloud, allowing it to be easily visible to the outside Universe.

Stars are born deep in dense clouds of dust and gas. This particular cloud is known as the Circinus molecular cloud complex. It is 2280 light-years away and stretches across 180 light-years of space. If our eyes could register the faint infrared glow of the gas in the cloud, it would stretch across our sky more than 70 times the size of the full Moon. It contains enough gas to make 250 000 stars like the Sun.

IRAS 14568-6304 was discovered with the Infrared Astronomical Satellite, launched in 1983 as a joint project of the US, the UK and the Netherlands to make the first all-sky infrared survey from space.

This particular image was taken by the NASA/ESA Hubble Space Telescope. It is a combination of just two wavelengths: optical light (blue) and infrared (golden orange). The dark swath running across the image is the Circinus molecular cloud, which is so dense that it obscures the stars beyond.

At longer infrared wavelengths, this darkness is filled with point-like stars, all deeply embedded and which will one day break out like IRAS 14568-6304 is doing.

Hubble and the sunrise over Earth

Indeed, IRAS 14568-6304 is just one member of a nest of young stellar objects in this part of Circinus, each of which is producing jets. Put together, they make up one of the brightest, most massive and most energetic outflows that astronomers have yet observed. In years to come, they will be a beautiful, brightly visible star cloud.

For images and more information about Hubble Space Telescope, visit:

    https://www.spacetelescope.org/
    http://hubblesite.org/
    http://www.nasa.gov/hubble

Image, Video, Text, Credits: ESA/Hubble & NASA Acknowledgements: R. Sahai (Jet Propulsion Laboratory), S. Meunier.

Best regards, Orbiter.ch