Saturday, December 27, 2014

The 29 Most Spectacular Space Photos Of 2014

The 29 Most Spectacular Space Photos Of 2014:



The year 2014 was a stellar one for spaceflight, what with ESA's Rosetta mission putting a robotic lander on a distant comet and NASA successfully testing its Orion spacecraft.

But 2014 was also a great year for space photography, as you can see from these remarkable 29 images (scroll down) picked for your viewing pleasure by your friends at HuffPost Science.

Join us for a trip through the cosmos--and be prepared to pick your jaw up off the floor.



  • NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
    This Hubble Space Telescope photo shows NGC 2174, the "Monkey Head Nebula," located 6,400 light-years from Earth.


  • Goddard Space Flight Center/AP
    A powerful X-class solar flare, one of three X-class flares unleashed by the sun on June 10 and 11, as seen by NASA's Solar Dynamics Observatory. X-class flares are the most powerful kind.




  • NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
    Hubble image of the barred spiral galaxy M83, the "Southern Pinwheel," which lies 15 million light-years away in the constellation Hydra. This mosaic image was released in January.


  • NASA


  • Galaxy NGC 4258, located about 23 million light-years away from Earth, as seen by NASA's Chandra X-ray Observatory.


  • ESA/NASA


  • NASA/JPL/University of Colorado


  • Reid Wiseman/NASA
    ISS astronaut Reid Wiseman tweeted this image of a sunrise on Oct. 29. Wiseman wrote, "Not every day is easy. Yesterday was a tough one. #sunrise"


  • NASA/Solar Dynamics Observatory
    This image taken by NASA's Solar Dynamics Observatory shows a profile view of coronal loops. Coronal loops are found around sunspots and in active regions.


  • NASA/JPL-Caltech/Space Science Institute




  • Rick Stevenson/Flickr
    Astrophotographer Rick Stevenson released this photo of SH2-199, also known as the "Soul Nebula," in December. This emission nebula is located about 6,500 light-years from Earth.


  • ESA/Hubble & NASA
    This Hubble image shows a portion of the Large Magellanic Cloud, a small nearby galaxy that orbits our galaxy, the Milky Way.


  • NASA/JPL-Caltech/Space Science Institute


  • X-ray: NASA/CXC/SAO/S.Mineo et al, Optical: NASA/STScI, Infr
    The photo is a composite image of the spiral galaxies NGC 2207 and IC 2163, located 130 million light years away in the constellation Canis Major. The image contains data from the Chandra X-ray Observatory in pink, optical light data from the Hubble Space Telescope in red, green, and blue, and infrared data from the Spitzer Space Telescope in red.


  • NASA/JPL
    In January and February 1979, NASA's Voyager 1 spacecraft zoomed toward Jupiter, capturing hundreds of images during its approach, including this close-up of swirling clouds around Jupiter's Great Red Spot. This image was assembled from three black and white negatives and newly released.


  • AP Photo/NASA
    An extreme ultra-violet wavelength image of a solar flare captured on Sept. 10.




  • NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
    This Hubble Space Telescope composite image shows a supernova explosion designated SN 2014J in the galaxy M82, at a distance of approximately 11.5 million light-years from Earth. It was taken on Jan. 31, as the supernova approached its peak brightness.


  • NASA, ESA, and E. Sabbi (STScI)
    An image of the Tarantula Nebula (or NGC 2070), located about 160,000 lights years away, released in January.


  • X-ray: NASA/CXC/PSU/K.Getman, E.Feigelson, M.Kuhn and the MYStIX team; Infrared: NASA/JPL-Caltech
    This composite image shows one of the clusters, NGC 2024, which is found in the center of the so-called Flame Nebula about 1,400 light years from Earth. In this image, X-rays from Chandra are seen as purple, while infrared data from NASA's Spitzer Space Telescope are colored red, green and blue.


  • NASA/JPL-Caltech/Space Science Institute
    Saturn's moon Tethys captured by the Cassini spacecraft's narrow-angle camera on July 14.


  • ESA/Rosetta/Philae/CIVA
    The Philae lander took this portrait of the Rosetta spacecraft on Sept. 7, 2014, at a distance of about 30 miles from comet 67P/Churyumov-Gerasimenko.


  • NASA/JPL-Caltech/SETI Institute
    The puzzling, fascinating surface of Jupiter's icy moon Europa looms large in this newly-reprocessed color view, made from images taken by NASA's Galileo spacecraft in the late 1990s.


  • A widefield view of the Flame (NGC2024) and Horsehead (IC434) Nebulae in Orion, captured in December by astrophotographer Roger Hutchinson . The pair are approximately 900 to 1,500 light years away.


  • AP Photo/ESA/Rosetta/MPS for OSIRIS Team
    Comet 67P/Churyumov-Gerasimenko, captured on Aug. 3, 2014 by Rosetta's OSIRIS narrow-angle camera.




  • NASA/JPL-Caltech
    The Orion Nebula, an immense stellar nursery some 1,500 light-years away. This stunning false-color view was constructed using infrared data from the Spitzer Space Telescope.


  • NASA/Reid Wiseman
    NASA astronaut Reid Wiseman captured this image from the International Space Station and tweeted it on Sept. 28, writing, "The Milky Way steals the show from Sahara sands that make the Earth glow orange."


  • NASA/ESA/Alexander Gerst
    European Space Agency astronaut Alexander Gerst tweeted this photograph taken from the International Space Station to social media on Aug. 29, 2014, writing, "words can't describe how it feels flying through an #aurora. I wouldn't even know where to begin…."


  • ESA/Hubble & NASA, Acknowledgements: D. Calzetti (UMass) and the LEGUS Team
    This view, captured by the NASA/ESA Hubble Space Telescope and released in July, shows a nearby spiral galaxy known as NGC 1433. At about 32 million light-years from Earth, it is a type of very active galaxy known as a Seyfert galaxy--with a bright, luminous center comparable in brightness to that of our entire galaxy, the Milky Way.
Photos curated by Damon Scheluer and Macrina Cooper-White.

Posted by Nelio Inacio at 12:35 PM 0 comments

Making the Trip to Mars Cheaper and Easier: The Case for Ballistic Capture

Making the Trip to Mars Cheaper and Easier: The Case for Ballistic Capture:



How long does it take to get to Mars


A new proposal for sending craft to Mars could save money and offer more flexible launch windows. Credit: NASA
When sending spacecraft to Mars, the current, preferred method involves shooting spacecraft towards Mars at full-speed, then performing a braking maneuver once the ship is close enough to slow it down and bring it into orbit.

Known as the “Hohmann Transfer” method, this type of maneuver is known to be effective. But it is also quite expensive and relies very heavily on timing. Hence why a new idea is being proposed which would involve sending the spacecraft out ahead of Mars’ orbital path and then waiting for Mars to come on by and scoop it up.

This is what is known as “Ballistic Capture”, a new technique proposed by Professor Francesco Topputo of the Polytechnic Institute of Milan and Edward Belbruno, a visiting associated researcher at Princeton University and former member of NASA’s Jet Propulsion Laboratory.

In their research paper, which was published in arXiv Astrophysics in late October, they outlined the benefits of this method versus traditional ones. In addition to cutting fuel costs, ballistic capture would also provide some flexibility when it comes to launch windows.

Currently, launches between Earth and Mars are limited to period where the rotation between the two planets is just right. Miss this window, and you have to wait another 26 months for a new one to come along.

At the same time, sending a rocket into space, through the vast gulf that separates Earth’s and Mars’ orbit, and then firing thrusters in the opposite direction to slow down, requires a great deal of fuel. This in turn means that the spacecraft responsible for transporting satellites, rovers, and (one day) astronauts need to be larger and more complicated, and hence more expensive.

As Belbruno told Universe Today via email:  “This new class of transfers is very promising for giving a new approach to future Mars missions that should lower cost and risk.  This new class of transfers should be applicable to all the planets. This should give all sorts of new possibilities for missions.”

The idea was first proposed by Belbruno while he was working for JPL, where he was trying to come up with numerical models for low-energy trajectories. “I first came up with the idea of ballistic capture in early 1986 when working on a JPL study called LGAS (Lunar Get Away Special),” he said. “This study involved putting a tiny 100 kg solar electric spacecraft in orbit around the Moon that was first ejected from a Get Away Special Canister on the Space Shuttle.”

The test of the LGAS was not a resounding success, as it would be two years before it got to the Moon. But in 1990, when Japan was looking to rescue their failed lunar orbiter, Hiten, he submitted proposals for a ballistic capture attempt that were quickly incorporated into the mission.

“The time of flight for this one was 5 months,” he said. “It was successfully used in 1991 to get Hiten to the Moon.” And since that time, the LGAS design has been used for other lunar missions, including the ESA’s SMART-1 mission in 2004 and NASA’s GRAIL mission in 2011.

But it is in future missions, which involve much greater distances and expenditures of fuel, that Belbruno felt would most benefit from this method. Unfortunately, the idea met with some resistance, as no missions appeared well-suited to the technique.

“Ever since 1991 when Japan’s Hiten used the new ballistic capture transfer to the Moon, it was felt that finding a useful one for Mars was not possible due to Mars much longer distance and its high orbital velocity about the Sun. However, I was able to find one in early 2014 with my colleague Francesco Topputo.”

Granted, there are some drawbacks to the new method. For one, a spacecraft sent out ahead of Mars’ orbital path would take longer to get into orbit than one that slows itself down to establish orbit.

In addition, the Hohmann Transfer method is a time-tested and reliable one. One of the most successful applications of this maneuver took place back in September, when the Mars Orbiter Mission (MOM) made its historic orbit around the Red Planet. This not only constituted the first time an Asian nation reached Mars, it was also the first time that any space agency had achieved a Mars orbit on the first try.

Nevertheless, the possibilities for improvements over the current method of sending craft to Mars has people at NASA excited. As James Green, director of NASA’s Planetary Science Division, said in an interview with Scientific American: “It’s an eye-opener. This [ballistic capture technique] could not only apply here to the robotic end of it but also the human exploration end.”

Don’t be surprised then if upcoming missions to Mars or the outer Solar System are performed with greater flexibility, and on a tighter budget.

Further Reading: arXiv Astrophysics



About 

Author, freelance writer, educator, Taekwon-Do instructor, and loving hubby, son and Island boy!
Posted by Nelio Inacio at 6:29 AM 0 comments

Spectacular Earth Timelapse Video: Christmas Gift from Alexander Gerst’s 2014 ISS Voyage

Spectacular Earth Timelapse Video: Christmas Gift from Alexander Gerst’s 2014 ISS Voyage:



Video Caption: Watch the Earth roll by through the perspective of German astronaut Alexander Gerst in this 4K six-minute timelapse video of images taken from on board the International Space Station (ISS) during 2014. Credit: Alexander Gerst/ESA

ESA astronaut Alexander Gerst from Germany who recently returned from a six month voyage to the International Space Station (ISS) has a special Christmas gift for all – a stunning six-minute timelapse compilation of his favorite images of Earth taken during his “Blue Dot” mission in 2014.

“A 4K timelapse showing our planet in motion, from my favourite Earth images taken during the Blue Dot mission,” wrote Gerst in connection with his spectacular timelapse video released to coincide with Christmastime.

“I wish all of you a merry Christmas! It was a wild year for me, thanks for joining me on this fascinating journey!” said Gerst in English.

“Wünsche euch allen fröhliche Weihnachten! War ein wildes Jahr für mich, vielen Dank, dass ihr mit dabei wart!” said Gerst in German.

You can watch the Earth roll by through Gerst’s perspective in this six-minute timelapse video combining over 12,500 images taken during his six-month mission aboard the ISS that shows the best our beautiful planet has to offer.



Another new snapshot of Earth’s “beautiful Southern Lights” taken from the ISS on 5 July 2014. Credit: ESA/Alexander Gerst


Another new snapshot of Earth’s “beautiful Southern Lights” taken from the ISS on 5 July 2014. Credit: ESA/Alexander Gerst
“Marvel at the auroras, sunrises, clouds, stars, oceans, the Milky Way, the International Space Station, lightning, cities at night, spacecraft and the thin band of atmosphere that protects us from space,” according to the video’s description.

Gerst would often would set cameras to automatically take pictures at regular intervals while doing his science research or preparing for the docking of other spacecraft at the ISS in order to get the timelapse effect shown in the video.



“Scary. The sunlight is far from reaching down the abyss of Neoguri's 65 km-wide eye.” Taken from the ISS on 8 July 2014. Credit: ESA/NASA/Alexander Gerst


“Scary. The sunlight is far from reaching down the abyss of Neoguri’s 65 km-wide eye.” Taken from the ISS on 8 July 2014. Credit: ESA/NASA/Alexander Gerst
The robotic arm capture and berthing of the SpaceX Dragon cargo ship and the release of the Orbital Sciences Cygnus cargo freighter are particularly magnificent in given a rare seen timelapse glimpse of visiting vehicles that are absolutely essential to keeping the station afloat, stocked and humming with research activities.

Gerst served aboard the ISS between May and November this year as a member of the Expedition 40 and 41 crews.

Gerst launched to the ISS on his rookie space flight on May 28, 2014 aboard the Russian Soyuz TMA-13M capsule along with Russian cosmonaut Maxim Suraev and NASA astronaut Reid Wiseman.

They joined the three station flyers already aboard – cosmonauts Alexander Skvortsov & Oleg Artemyev and astronaut Steve Swanson – to restore the station crew complement to six.

Gerst and Wiseman became well known and regarded for their prolific and expertly crafted photography skills.



ESA astronaut Alexander Gerst, Russian commander Maxim Suraev and NASA astronaut Reid Wiseman returned to Earth on 10 November 2014, landing in the Kazakh steppe. Credit: ESA–S. Corvaja


ESA astronaut Alexander Gerst, Russian commander Maxim Suraev and NASA astronaut Reid Wiseman returned to Earth on 10 November 2014, landing in the Kazakh steppe. Credit: ESA–S. Corvaja
They returned to Earth safely on Nov. 10, 2014 with a soft landing on the Kazakh steppes.

Alex is Germany’s third astronaut to visit the ISS. He conducted a spacewalk with Wiseman on Oct. 7 while aboard. He is trained as a geophysicist and a volcanologist.



ESA astronaut Alexander Gerst spent six hours and 13 minutes outside the International Space Station with NASA astronaut Reid Wiseman on Tuesday, 7 October 2014. This was the first spacewalk for both astronauts but they performed well in the weightlessness of orbit. Credit: NASA/ESA


ESA astronaut Alexander Gerst spent six hours and 13 minutes outside the International Space Station with NASA astronaut Reid Wiseman on Tuesday, 7 October 2014. This was the first spacewalk for both astronauts but they performed well in the weightlessness of orbit. Credit: NASA/ESA
Read my story detailing Christmas 2014 festivities with the new crews at the ISS – here.

Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.

Ken Kremer



About 

Dr. Ken Kremer is a speaker, scientist, freelance science journalist (Princeton, NJ) and photographer whose articles, space exploration images and Mars mosaics have appeared in magazines, books, websites and calanders including Astronomy Picture of the Day, NBC, BBC, SPACE.com, Spaceflight Now and the covers of Aviation Week & Space Technology, Spaceflight and the Explorers Club magazines. Ken has presented at numerous educational institutions, civic & religious organizations, museums and astronomy clubs. Ken has reported first hand from the Kennedy Space Center, Cape Canaveral and NASA Wallops on over 40 launches including 8 shuttle launches. He lectures on both Human and Robotic spaceflight - www.kenkremer.com. Follow Ken on Facebook and Twitter
Posted by Nelio Inacio at 6:28 AM 0 comments

Friday, December 26, 2014

Student Team Wants to Terraform Mars Using Cyanobacteria

Student Team Wants to Terraform Mars Using Cyanobacteria:



Living Mars. Credit: Kevin Gill


Artist concept of a ‘Living’ Mars. Credit: Kevin Gill
While scientists believe that at one time, billions of years ago, Mars had an atmosphere similar to Earth’s and was covered with flowing water, the reality today is quite different. In fact, the surface of Mars is so hostile that a vacation in Antarctica would seem pleasant by comparison.

In addition to the extreme cold, there is little atmosphere to speak of and virtually no oxygen. However, a team of students from Germany wants to change that. Their plan is to introduce cyanobacteria into the atmosphere which would convert the ample supplies of CO² into oxygen gas, thus paving the way for possible settlement someday.

The team, which is composed of students and volunteer scientists from the University of Applied Science and the Technical University in Darmstadt, Germany, call their project “Cyano Knights”. Basically, they plan to seed Mars’ atmosphere with cyanobacteria so it can convert Mars’ most abundant gas (CO2, which accounts for 96% of the Martian atmosphere) into something breathable by humans.



The Mars One University Competition poster. Credit: Mars One


Promotional image for the Mars One University Competition. Credit: Mars One
Along with teams from other universities and technical colleges taking part in the Mars One University Competition, the Cyano Knights hope that their project will be the one sent to the Red Planet in advance of the company’s proposed settlers.

This competition officially began this past summer, as part of the Mars One’s drive to enlist the support and participation of universities from all around the world. All those participating will have a chance to send their project aboard the company’s first unmanned lander, which will be sent to Mars in 2018.

Working out of the laboratory of Cell Culture Technology of the University of Applied Science, the Cyano Knights selected cyanobacteria because of its extreme ruggedness. Here on Earth, the bacteria lives in conditions that are hostile to other life forms, hence why they seemed like the perfect candidate.

As the team leader Robert P. Schröder, said to astrowatch.net: “Cyanobacteria do live in conditions on Earth where no life would be expected. You find them everywhere on our planet! It is the first step on Mars to test microorganisms.”



Cyanobacteria Spirulina. Credit: cyanoknights.bio


Cyanobacteria Spirulina. Credit: cyanoknights.bio
The other reason for sending cyanobacteria to Mars, in advance of humans, is the biological function they perform. As an organism that produces oxygen gas through photosynthesis to obtain nutrients, cyanobacteria are thought to have played a central role in the evolution of Earth’s atmosphere.

It is estimated that 2.7 billion years ago, they were pivotal in converting it from a toxic fume to the nitrogen and oxygen-rich one that we all know and love. This, in turn, led to the formation of the ozone layer which blocks out harmful UV rays and allowed for the proliferation of life.

According to their project description, the cyanobacteria, once introduced, will “deliver oxygen made of their photosynthesis, reducing carbon dioxide and produce an environment for living organisms like us. Furthermore, they can supply food and important vitamins for a healthy nutrition.”

Of course, the team is not sure how much of the bacteria will be needed to make a dent in Mars’ carbon-rich atmosphere, nor how much of the oxygen could be retained. But much like the other teams taking part in this competition, the goal here is to find out how terrestrial organisms will fair in the Martian environment.



Artist's concept of a Martian astronaut standing outside the Mars One habitat. Credit: Bryan Versteeg/Mars One


Artist’s concept of a Martian astronaut standing outside the Mars One habitat. Credit: Bryan Versteeg/Mars One
The Cyano Knights hope that one day, manned mission will be able to take advantage of the oxygen created by these bacteria by either combining it with nitrogen to create breathable air, or recuperating it for consumption over and over again.

Not only does their project call for the use of existing technology, it also takes advantage of studies being conducted by NASA and other space agencies. As it says on their team page: “On the international space station they do experiments with cyanobacteria too. So let us take it to the next level and investigate our toughest life form on Mars finding the best survival species for mankind! We are paving the way for future Mars missions, not only to have breathable air!”

Other concepts include germinating seeds on Mars to prove that it is possible to grow plants there, building a miniature greenhouse, measuring the impact of cosmic surface and solar radiation on the surface, and processing urine into water.

All of these projects are aimed at obtaining data that will contribute to our understanding of the Martian landscape and be vital to any human settlements or manned missions there in the future.

For more information on the teams taking part in the competition, and to vote for who you would like to win, visit the Mars One University Competition page. Voting submission will be accepted until Dec. 31, 2014 and the winning university payload will be announced on Jan. 5, 2015.

Further Reading: CyanoKnights, MarsOne University Competition



About 

Author, freelance writer, educator, Taekwon-Do instructor, and loving hubby, son and Island boy!
Posted by Nelio Inacio at 10:12 AM 0 comments

Wednesday, December 24, 2014

Solved: The Mystery of Earth’s Theta Aurora

Solved: The Mystery of Earth’s Theta Aurora:



From the ground, aurora have mystified humans since we began to question the world. The space age revealed more mystery - the Theta Auroral Oval (inset) and the challenge of understanding the phenomena. (Photo Credit: NASA/APOD)


From the ground, aurora have mystified humans since we began to question the world. The space age revealed more mystery – the Theta Auroral Oval (inset) and the challenge of understanding the phenomena. (Photo Credit: NASA/APOD)
The mystery of the northern lights – aurora – spans time beyond history and to cultures of both the southern and northern hemispheres. The mystery involves the lights, fantastic patterns and mystical changes. Ancient men and women stood huddled under them wondering what it meant. Was it messages from the gods, the spirits of loved ones, warnings or messages to comfort their souls?

Aurora reside literally at the edge of space. While we know the basics and even more, we are still learning. A new published work has just added to our understanding by explaining how one type of aurora – the Theta Aurora – is created from the interaction of the charged particles, electric and magnetic fields surrounding the Earth. Their conclusions required the coordination of simultaneous observations of two missions.

The Theta Auroral Oval as observed by the NASA IMAGE FUV camera on September 15, 2005. (Credit: NASA/SWRI)
The Theta Auroral Oval as observed by the NASA IMAGE FUV camera on September 15, 2005 and anlayzed using Cluster data in the paper by Fear et al. (Credit: NASA/SWRI)
We were not aware of Thetas until the advent of the space age and our peering back at Earth. They cannot be recognized from the ground. The auroras that bystanders see from locales such as Norway or New Zealand are just arcs and subsets of the bigger picture which is the auroral ovals atop the polar regions of the Earth. Ground based all-sky cameras and polar orbiting probes had seen what were deemed “polar cap arcs.” However, it was a spacecraft Dynamics Explorer I (DE-1) that was the first to make global images of the auroral ovals and observed the first “transpolar arcs”, that is, the Theta aurora.

They are named Theta after the Greek letter that they resemble. Thetas are uncommon and do not persist long. Early on in the exploration of this phenomenon, researchers have been aware that they occur when the Sun’s magnetic field, called the Interplanetary Magnetic Field (IMF) turns northward. Most of the time the IMF in the vicinity of the Earth points south. It is a critical aspect of the Sun-Earth interaction. The southerly pointing field is able to dovetail readily with the normal direction of the Earth’s magnetic field. The northward IMF interacting with the Earth’s field is similar to two bar magnets turned head to head, repelling each other. When the IMF flips northward locally, a convolution takes place that will, at times, but not always, produce a Theta aurora.

A group of researchers led by Dr. Robert Fear from the Department of Physics & Astronomy, University of Leicester, through analysis of simultaneous spacecraft observations, has identified how the particles and fields interact to produce Theta aurora. Their study, “Direct observation of closed magnetic flux trapped in the high-latitude magnetosphere” in the Journal Science (December 19, 2014, Vol 346) utilized a combination of data from ESA’s Cluster spacecraft mission and the IMAGE spacecraft of NASA. The specific event in the Earth’s magnetosphere on September 15, 2005 was observed simultaneously by the spacecraft of both missions.



Illustrations of the Cluster II spacecraft in orbit and formation around the Earth and the NASA IMAGE spacecraft vehicle design. The two mission's observations were combined to correlate numerous auroral and magnetospheric events. Cluster II remains in operation as of December 2014 (14 yr lifespan). (Credit: ESA, NASA)


Illustrations of the Cluster II spacecraft in orbit and formation around the Earth and the NASA IMAGE spacecraft vehicle design. The two mission’s observations were combined to correlate numerous auroral and magnetospheric events. Cluster II remains in operation as of December 2014 (14 yr lifespan). (Credit: ESA, NASA)
Due to the complexity of the Sun-Earth relationship involving neutral and charged particles and electric and magnetic fields, space scientists have long attempted to make simultaneous measurements with multiple spacecraft. ISEE-1, 2 and 3 were one early attempt. Another was the Dynamics Explorer 1 & 2 spacecraft. DE-2 was in a low orbit while DE-1 was in an elongated orbit taking it deeper into the magnetosphere. At times, the pair would align on the same magnetic field lines. The field lines are like rails that guide the charged particles from far out in the magneto-tail to all the way down to the upper atmosphere – the ionosphere. Placing two or more spacecraft on the same field lines presented the means of making coordinated observations of the same event. Dr. Fear and colleagues analyzed data when ESA’s Cluster resided in the southern lobe of the magnetotail and NASA’s IMAGE (Imager for Magnetopause-to-Aurora Global Exploration) spacecraft resided above the south polar region of the Earth.

Cluster is a set of four spacecraft, still in operation after 14 years. Together with IMAGE, five craft were observing the event. Fear, et al utilized ESA spacecraft Cluster 1 (of four) and NASA’s IMAGE. On that fateful day, the IMF turned north. As described in Dr. Fear’s paper, on that day, the north and south lobes of the magnetosphere were closed. The magnetic field lines of the lobes were separated from the Solar wind and IMF due to what is called magnetic reconnection. The following diagram shows how complex Earth’s magnetosphere is; with regions such as the bow shock, magnetopause, cusps, magnetotail, particle belts and the lobes.



Illustration of the Earth's magnetosphere showing it complexity. The Theta Aurora are now confidently linked to magnetic reconnection events in the lobes of the magnetotail. (Credit: NASA)


Illustration of the Earth’s magnetosphere showing it complexity. The Theta Aurora are now confidently linked to magnetic reconnection events in the lobes of the magnetotail. (Credit: NASA)
The science paper explains that what was previously observed by only lower altitude spacecraft was captured by Cluster within the magnetotail lobes. The southerly lobe’s plasma – ionized particles – was very energetic. The measurements revealed that the southern lobe of the magnetotail was acting as a bottle and the particles were bouncing between two magnetic mirrors, that is, the lobes were close due to reconnection. The particles were highly energetic.

The presence of what is called a double loss cone signature in the electron energy distribution was a clear indicator that the particles were trapped and oscillating between mirror points. The consequences for the Earth’s ionosphere was that highly energetic particles flooded down the field lines from the lobes and impacted the upper atmosphere transferring their energy and causing the magnificent light show that we know as the Northern Lights (or Southern) in the form of a Theta Auroral Oval. This strong evidence supports the theory that Theta aurora are produced by energized particles from within closed field lines and not by energetic particles directly from the Solar Wind that find a path into the magnetosphere and reach the upper atmosphere of the Earth.



A video of an observed major geomagnetic storm (July 15, 2000) taken by the Far Ultraviolet Imaging System (FUV) on IMAGE. IMAGE operated from 2000 to December 2005 when communications were lost. (Credit: NASA/SWRI) [click to view the animated gif]


A video of an observed major geomagnetic storm (July 15, 2000, southward IMF) taken by the Far Ultraviolet Imaging System (FUV) on the spacecraft IMAGE. IMAGE operated from 2000 until December 2005 when communications were inexplicably lost. (Credit: NASA/SWRI) [click to view the animated gif]
Without the coordination of the observations and the collective analysis, the Theta aurora phenomenon would continue to be debated. The analysis by Dr. Fear, while not definitive, is strong proof that Theta aurora are generated from particles trapped within closed field lines.


The analysis of the Cluster mission data as well as that of many other missions takes years. Years after observations are made researchers can achieve new understanding through study of arduous details or sometimes by a ha-ha moment. Aurora represent the signature of the interaction of two magnetic fields and two populations of particles – the Sun’s field and energetic particles streaming at millions of miles per hour from its surface reaching the Earth’s magnetic field. The Earth’s field is transformed by the interaction and receives energetic particles that it bottles up and energizes further. Ultimately, the Earth’s magnetic field directs some of these particles to the topside of our atmosphere. For thousands and likely tens of thousands of years, humans have questioned what it all means. Now another piece of the puzzle has been laid down with a good degree of certainty; one that explains the Theta aurora.

Reference:

Direct observation of closed magnetic flux trapped in the high-latitude magnetosphere

Transpolar arc evolution and associated potential patterns

Transpolar aurora: time evolution, associated convection patterns, and a possible cause

Related articles at Universe Today:

Guide to Space –

Earth’s Magnetic Field,

Aurora Borealis



About 

Contributing writer Tim Reyes is a former NASA software engineer and analyst who has supported development of orbital and lander missions to the planet Mars since 1992. He has an M.S. in Space Plasma Physics from University of Alabama, Huntsville.
Posted by Nelio Inacio at 3:39 PM 0 comments

Tuesday, December 23, 2014

What is the Average Surface Temperature on Venus?

What is the Average Surface Temperature on Venus?:



False color radar topographical map of Venus provided by Magellan. Credit: Magellan Team/JPL/NASA





Venus is often referred to as our “sister planet,” due to the many geophysical similarities that exist between it Earth. For starters, our two planets are close in mass, with Venus weighing in at 4.868 x 1024 kg compared to Earth’s 5.9736×1024 kg. In terms of size, the planets are almost identical, with Venus measuring 12,100 km in diameter and Earth 12,742 km.

In terms of density and gravity, the two are neck and neck – with Venus boasting 86.6% of the former and 90.7% of the latter. Venus also has a thick atmosphere, much like our own, and it is believed that both planets share a common origin, forming at the same time out of a condensing clouds of dust particles around 4.5 billion years ago.

However, for all the characteristics these two planets have in common, average temperature is not one of them. Whereas the Earth has an average surface temperature of 14 degrees Celsius, the average temperature of Venus is 460 degrees Celsius. That is roughly 410 degrees hotter than the hottest deserts on our planet.

In fact, at a searing 750 K (477 °C), the surface of Venus is the hottest in the solar system. Venus is closer to the Sun by 108 million km, (about 30% closer than the Earth), but it is mainly due to the planet’s thick atmosphere. Unlike Earth’s, which is composed primarily of nitrogen, oxygen and ozone, Venus’ atmosphere is an incredibly dense cloud of carbon dioxide and sulfur dioxide gas.

The combination of these gases in high concentrations causes a catastrophic greenhouse effect that traps incident sunlight and prevents it from radiating into space. This results in an estimated surface temperature boost of 475 K (196.85 °C), leaving the surface a molten, charred mess that nothing (that we know of) can live on. Atmospheric pressure also plays a role, being 91 times that of what it is here on Earth; and clouds of toxic vapor constantly rain sulfuric acid on the surface.



False color radar topographical map of Venus provided by Magellan. Credit: Magellan Team/JPL/NASA


False-color radar topographical map of Venus produced by the Magellan spacecraft’s radar system. Credit: Magellan Team/JPL/NASA
In addition, the surface temperature on Venus does not vary like it does here on Earth. On our planet, temperatures vary wildly due to the time of year and even more so based on the location on our planet. The hottest temperature ever recorded on Earth was 70.7°C in the Lut Desert of Iran in 2005. On the other end of the spectrum, the coldest temperature ever recorded on Earth was in Vostok, Antarctica at -89.2 C.

But on Venus, the surface temperature is 460 degrees Celsius, day or night, at the poles or at the equator. Beyond its thick atmosphere, Venus’ axial tilt (aka. obliquity) plays a role in this temperature consistency. Earth’s axis is tilted 23.4 ° in relation to the Sun, whereas Venus’ is only tilted by 3 °.

The only respite from the heat on Venus is to be found around 50 km into the atmosphere. It is at that point that temperatures and atmospheric pressure are equal to that of Earth’s. It is for this reason that some scientists believe that floating habitats could be constructed here, using Venus’ thick clouds to buoy the habitats high above the surface. Additionally, in 2014, a group of mission planners from NASA Langely came up with a mission to Venus’ atmosphere using airships.

These habitats could play an important role in the terraforming of Venus as well, acting as scientific research stations that could either fire off the excess atmosphere off into space, or introduce bacteria or chemicals that could convert all the CO2 and SO2 into a hospitable, breathable atmosphere.

Beyond the fact that it is a hot and hellish landscape, very little is known about Venus’ surface environment. This is due to the thick atmosphere, which has made visual observation impossible. The sulfuric acid is also problematic since clouds composed of it are highly reflective of visible light, which prevents optical observation. Probes have been sent to the surface in the past, but the volatile and corrosive environment means that anything that lands there can only survive for a few hours.



3-D perspective of the Venusian volcano, Maat Mons generated from radar data from NASA’s Magellan mission.


3-D perspective of the Venusian volcano, Maat Mons generated from radar data from NASA’s Magellan mission. Credit: Magellan Team/NASA/JPL
What little we know about the planet’s surface has come from years worth of radar imaging, the most recent of which was conducted by NASA’s Magellan spacecraft (aka. the Venus Radar Mapper). Using synthetic aperture radar, the robotic space probe spent four years (1990-1994) mapping the surface of Venus and measuring its gravitational field before its orbit decayed and it was “disposed of” in the planet’s atmosphere.

The images provided by this and other missions revealed a surface dominated by volcanoes. There are at least 1,000 volcanoes or volcanic centers larger than 20 km in diameter on Venus’ harsh landscape. Many scientists believe Venus was resurfaced by volcanic activity 300 to 500 million years ago. Lava flows are a testament to this, which appear to have produced channels of hardened magma that extend for hundreds of km in all directions. The mixture of volcanic ash and the sulfuric acid clouds is also known to produce intense lightning and thunder storms.

The temperature of Venus is not the only extreme on the planet. The atmosphere is constantly churned by hurricane force winds reaching 360 kph. Add to that the crushing air pressure and rainstorms of sulfuric acid, and it becomes easy to see why Venus is such a barren, lifeless rock that has been hard to explore.

We have written many articles about Venus for Universe Today. Here are some interesting facts about Venus, and here’s an article about Venus Greenhouse Effect. And here is an article about the many interesting pictures taken of Venus over the past few decades.

If you’d like more information on Venus, check out Hubblesite’s News Releases about Venus, and here’s a link to NASA’s Solar System Exploration Guide on Venus.

We’ve also recorded an entire episode of Astronomy Cast all about Venus. Listen here, Episode 50: Venus.

Reference:
NASA



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Posted by Nelio Inacio at 2:48 PM 0 comments
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