An unmanned Russian space freighter hauling fresh fruit and over three tons of food, water, supplies and science experiments blasted off today, Thursday, March 31, from the Baikonur Cosmodrome in Kazakhstan, commencing a two-day orbital trek to the six person crew living aboard the International Space Station (ISS).
The successful nighttime liftoff of the Progress 63 cargo ship atop a three stage Soyuz 2.1a booster took place at 12:23 p.m. EDT (10:23 p.m. local time in Baikonur) from Site 31 at Baikonur as the orbiting outpost was flying about 251 miles (400 km) above northeast Iraq.
NASA astronaut and Expedition 47 crew member Jeff Williams captured several elegant views of the Progress launch from his heavenly perch on the station inside the Cupola.
“Fresh fruit is on the way! Here are some of the best pics taken from @Space_Station during today’s #Progress launch,” Williams said on his social media accounts from space.
“Today’s #Progress launch occurred about 5 minutes before we passed over the launch site in Baikonur.”
“Sunset occurred for us about a minute later and shortly after we caught site of the rocket ahead and below us from the Cupola. We continued to catch up to it until it was directly below. We saw the flash of 3rd stage ignition and the subsequent 3rd stage was spectacular. Here are some of the best shots taken from the International Space Station. (note the one taken just after the moment of engine cutoff!) Spectacular!” Williams elaborated.
The Progress 63 resupply ship, also known by its Russian acronym as Progress MS-02, is due to arrive at the station on April 2 for an automated docking to the aft port of the Russian Zvezda Service Module.
After a picture perfect eight and a half minute climb to its initial orbit, the Progress MS-02 separated from the Soyuz third stage and deployed its pair of solar arrays and navigational antennas as planned.
“This was a flawless ascent to orbit for the Progress 63 cargo craft carrying just over three tons of supplies,” said NASA launch commentator Rob Navius during a live launch webcast on NASA TV. “Everything was right on the money.”
“All stages of the Soyuz booster performed to perfection.”
The planned longer two-day and 34 orbit journey rather than a faster 3 or 4 orbit rendezvous and docking is designed to help engineers test out new computer software and vehicle communications gear on this new version of the Progress.
“The two-day rendezvous for the Progress is deliberately planned to enable Russian flight controllers to test new software and communications equipment for the new vehicle configuration that will be standard for future Progress and piloted Soyuz spacecraft,” according to NASA officials.
Docking to the orbiting laboratory is set for approximately 2 p.m. Saturday, April 2.
NASA TV will provide live docking coverage of the Progress 63 arrival starting at 1:15 p.m. on Saturday.
Today’s Progress launch counts as the second of a constellation of three resupply ships from the US and Russia launching to the station over a three successive weeks.
The Orbital ATK ‘SS Rick Husband’ Cygnus resupply spacecraft that launched last week on Tuesday, March 22, 2016 was at the vanguard of the cargo ship trio – as I reported here from on site at the Kennedy Space Center in Florida.
Cygnus was successfully berthed at the Earth-facing port of the Unity module this past Saturday, March 26 – as I reported here.
Following Progress is the SpaceX Return To Flight (RTF) mission dubbed SpaceX CRS-8.
It is slated to launch on April 8 and arrive at the ISS on April 10 for berthing to the Earth-facing port of the Harmony module – at the end of the station where NASA space shuttles formerly docked. It carries another 3.5 tons of supplies.
So altogether the trio of international cargo ships will supply over 12 tons of station supplies in rapid succession over the next 3 weeks.
This choreography will set up America’s Cygnus and Dragon resupply craft to simultaneously be present and reside attached at adjacent ports on the ISS for the first time in history.
Plans currently call for Cygnus to stay at station for approximately two months until May 20th., when it will be unbolted and unberthed for eventual deorbiting and reentry.
Progress 63 will remain at the station for six months.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Learn more about Orion, SLS, ISS, NASA Mars rovers, Orbital ATK, ULA, SpaceX, Boeing, Space Taxis, NASA missions and more at Ken’s upcoming outreach events:
Apr 9/10: “NASA and the Road to Mars Human Spaceflight programs” and “Curiosity explores Mars” at NEAF (NorthEast Astronomy and Space Forum), 9 AM to 5 PM, Suffern, NY, Rockland Community College and Rockland Astronomy Club – http://rocklandastronomy.com/neaf.html
Apr 12: Hosting Dr. Jim Green, NASA, Director Planetary Science, for a Planetary sciences talk about “Ceres, Pluto and Planet X” at Princeton University; 7:30 PM, Amateur Astronomers Assoc of Princeton, Peyton Hall, Princeton, NJ – http://www.princetonastronomy.org/
Apr 17: “NASA and the Road to Mars Human Spaceflight programs”- 1:30 PM at Washington Crossing State Park, Nature Center, Titusville, NJ – http://www.state.nj.us/dep/parksandforests/parks/washcros.html
KENNEDY SPACE CENTER, FL – Following a perfectly executed three day orbital rendezvous, NASA astronaut and Expedition 47 Commander Tim Kopra successfully reached out with the International Space Station’s robotic arm, Canadarm2, grabbed hold and captured Orbital ATK’s commercial Cygnus cargo freighter at 6:51 a.m. EDT, this morning, Saturday, March 26, 2016.
The ISS and Cygnus were soaring some 250 miles (400 kilometers) over the Indian Ocean at the time of capture following the cargo crafts blastoff atop a two stage United Launch Alliance (ULA) Atlas V at 11:05 p.m. EDT on Tuesday, March 22, 2016 from Space Launch Complex 41 on Cape Canaveral Air Force Station, Fl.
Robotics officers on the ground in Houston working with the station crew high above then maneuvered Cygnus – holding over 3.5 tons of critical cargo supplies and science – into position for final installation and berthing to the orbiting laboratory’s Earth-facing port on the Unity module a few hours later. It was finally bolted fully into place at approximately 10:52 a.m. EDT.
This Cygnus is named the S.S. Rick Husband in honor of Col. Rick Husband, the late commander of Space Shuttle Columbia, which was tragically lost with its crew of seven NASA astronauts during re-entry on its final flight on Feb. 1, 2003.
The crew plans to open the hatch to the SS Rick Husband tomorrow morning on Easter Sunday, March 26.
The Orbital ATK Cygnus CRS-6 space freighter is loaded with 3513 kg (7700 pounds) of science experiments and hardware, crew supplies, spare parts, gear and station hardware for the orbital laboratory in support of over 250 research experiments being conducted on board by the Expedition 47 and 48 crews.
All of Cygnus maneuvers were “executed to perfection for a flawless approach and rendezvous” after the three day trip from Florida to the ISS, as the vehicle closed in to within a few meters for grappling, said NASA commentator Rob Navius.
NASA TV showed spectacular HD views of Cygnus and its UltraFlex solar arrays – deployed 2 hours after launch – from station and robotic arm cameras during the final approach operation, as flight controllers closely monitored all spacecraft systems.
“The crew is ready for Cygnus approach to the capture point,” radioed Kopra.
“Station you are go for capture,” Mission Control radioed back.
Cygnus was placed into free drift mode before capture to prevent any accidental perturbations in the final seconds.
From his robotics work station in the Cupola, Kopra then put the arm in motion by about 6:40 a.m. EDT, during the final phase of the final approach. He extended the 57 foot long (19 meter long) arm to reach out and grab the aft end of Cygnus cargo craft at its grappling pin by closing the snares on the end effector.
ESA astronaut Tim Peake served as backup for arm operations while NASA astronaut Jeff Williams monitored Cygnus systems.
The SS Rick Husband was rock steady during its capture as the station was flying over South Africa and the Indian Ocean.
“Capture confirmed,” reported Navius just moments before the video downlink was temporarily lost as the station communications moved between satellites.
“Excellent work gentleman. Much appreciated. Made that look easy,” radioed Jeremy Hansen, a Canadian Space Agency astronaut from Houston mission control.
“We’d also like to say we are really honored to bring aboard the SS Rick Husband to the International Space Station,” radioed Kopra. “He was a personal hero to many of us. This will be the first Cygnus honoree who was directly involved with the construction of this great station.”
It took about 9 minutes to complete the approach from the 30 meter distant hold point to the final capture point where the SS Rick Husband Cygnus arrived at about 6:37 am EDT. NASA TV showed the grapple fixture gradually coming into view.
Cygnus approached precisely within the center of the approach corridor, said Peake, during continuing updates as the ship moved closer to the targeted berthing port. It was perfectly aligned for its capture point.
Cygnus grapple fixture is located at the bottom end of the vehicles service module, beside the thruster.
Kopra and Peake are spending their 103rd day on the station today. While Williams arrived just 8 days ago.
All burns to get to the initial rendezvous point in the keep out sphere 250 meters away were “right on the money. Every burn has been on course and on target, said NASA JSC commentator Navius in Houston, as Cygnus soared some 400 km over the Pacific.
“Everything has gone off without a hitch. A rock solid approach.”
Flight controllers in Houston and Orbital ATK’s Dulles control headquarters then gave the go ahead to resume moving and approach closer to the 30 meter hold point.
The actual berthing operation took place about an hour later than expected to double check that everything was precisely aligned and communications were fully established.
Controllers used the arm to move Cygnus in for capture. They commanded four gangs of four bolts to latch Cygnus to the common berthing mechanism (CBM) on the internally positioned Unity modules nadir or Earth-facing port.
The first and second stage captures were successfully completed by 10:52 a.m. EDT this morning, marking the official hard mating of Cygnus and the station.
When the ISS Expedition 47 crew members open the hatch, they will be greeted with a sign noting the spacecraft was named SS Rick Husband in honor of the STS-107 mission commander.
The SS Rick Husband Cygnus is actually at the vanguard of a “constellation” of three resupply ships arriving at the station over a three week period of three weekends.
Next comes the Russian Progress 63 which will dock at Russia’s Zvezda module next weekend after launching this Thursday from site 31 at Kaszakhstan carrying another three tons of supplies.
Following Progress is the SpaceX Return To Flight (RTF) mission dubbed SpaceX CRS-8.
It is slated to launch on April 8 and arrive at the ISS on April 10 for berthing to the Earth-facing port of the Harmony module – at the end of the station where NASA space shuttles formerly docked. It carries another 3.5 tons of supplies.
So altogether the trio of international cargo ships will supply over 12 tons of station supplies in rapid succession over the next 3 weeks.
This choreography will set up America’s Cygnus and Dragon resupply craft to simultaneously be present and reside attached at adjacent ports on the ISS for the first time in history.
Plans currently call for Cygnus to stay at station for approximately two months until May 20th, when it will be unbolted and unberthed for eventual deorbiting and reentry.
But first it will stay on orbit for about another eight days, said Orbital ATK’s Cygnus program manager Frank DeMauro in an interview with Universe Today.
After unberthing, Cygnus will be used to conduct several experiments including the Saffire-1 experiment, it will deploy nanosats from an externally mounted carrier, and the REBR experiment will monitor the burn-up of Cygnus during the fiery reentry into the Earth’s atmosphere, said DeMauro.
Orbital ATK’s attention then shifts to the next Cygnus launch on the Return to Flight, or RTF, mission of the firms Antares rocket from NASA Wallops on the eastern shore of Virginia.
OA-6 is only the second Cygnus to be launched atop a ULA Atlas V rocket, following the OA-4 mission last December.
The CRS-6/OA-6 flight is also the second flight of the enhanced Cygnus variant, that is over 1 meter longer and sports 50% more volume capability.
Thus it is capable of carrying a much heavier payload of some 3500 kg (7700 lbs) vs. a maximum of 2300 kg (5070 lbs) for the standard version.
Watch for Ken’s onsite launch reports direct from the Kennedy Space Center in Florida and continuing mission reports.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Video caption: Mobius video camera placed at Florida launch pad captures blastoff up close of Orbital ATK OA-6 (CRS-6) mission riding to orbit atop a United Launch Alliance Atlas V rocket on March 22, 2016 at 11:05 p.m. EDT from Space Launch Complex-41 on Cape Canaveral Air Force Station. Credit: Ken Kremer/kenkremer.com
KENNEDY SPACE CENTER, FL – Tuesday evening, March 22, turned into ‘streaks galore’ on Florida’s space coast, as the nighttime launch of an Orbital ATK Cygnus cargo freighter atop an Atlas V rocket was captured in unforgettable fashion by talented space photographers as it chases down the International Space Station (ISS), loaded with hundreds of science experiments.
Check out this expanding gallery of breathtaking photos and videos collected from many of my photojournalist friends and colleagues – who collectively count as the best space photographers worldwide!
We all descended on the sunshine state to record the Tuesday’s blastoff of the United Launch Alliance Atlas V rocket carrying Orbital ATK’s Cygnus CRS-6 (OA-6) spacecraft from an array of locations ringing Cape Canaveral’s seaside launch pad as well as remote cameras we all set as media directly at the launch pad.
The two stage ULA Atlas V lifted off right on time at 11:05 p.m. EDT from Space Launch Complex 41 on Cape Canaveral Air Force Station, Fl, into a picturesque moonlit sky on a resupply mission to the ISS.
One could not have asked for better weather. Conditions were near perfect at launch time with virtually no winds and clouds.
Cygnus rode to orbit on a fountain of fire. And right now she is in hot pursuit of the million pound orbiting outpost crewed by an international team of six astronauts and cosmonauts.
The streak shots vividly show how the rocket magnificently illuminated the scattered thin clouds hovering over the seaside launch pad as it ascended and arced over eastwards towards Africa.
The Orbital ATK Cygnus CRS-6 (OA-6) mission launched aboard an Atlas V Evolved Expendable Launch Vehicle (EELV) in the 401 configuration vehicle. This includes a 4-meter-diameter payload fairing in its longest, extra extended configuration to accommodate the Cygnus.
The first stage of the Atlas V booster is powered by the RD AMROSS RD-180 engine. The Centaur upper stage was powered by the Aerojet Rocketdyne RL10C-1 engine.
It was the ULA’s 62nd straight success with the Atlas V as well as the firms third launch in 2016 and the 106th launch since the company formed in 2006.
The Cygnus CRS-6 (OA-6) mission is being launched under terms of the firm’s Commercial Resupply Services (CRS) contract with NASA. It also counts as Orbital ATK’s fifth cargo delivery mission to the space station.
Watch these launch videos from remote video cameras set right at the launch pad showing the full fury of liftoff sounding off with the deafening thunder of some one million pounds of liftoff thrust.
Video caption: Flame trench view of the Orbital/ATK OA-6 resupply module launch to the ISS on a ULA Atlas 5 rocket from Pad 41 of the CCAFS on March 22, 2016. Credit: Jeff Seibert/AmericaSpace
Video caption: Mobius video camera placed at Florida launch pad captures blastoff up close of Orbital ATK OA-6 (CRS-6) mission riding to orbit atop a United Launch Alliance Atlas V rocket on March 22, 2016 at 11:05 p.m. EDT from Space Launch Complex-41 on Cape Canaveral Air Force Station. Credit: Ken Kremer/kenkremer.com
OA-6 is loaded with 3513 kg (7700 pounds) of science experiments and hardware, crew supplies, spare parts, gear and station hardware to the orbital laboratory in support over 250 research experiments being conducted on board by the Expedition 47 and 48 crews.
Among the research highlights are experiments like Strata-1 which will evaluate how soil on airless bodies like asteroids moves about in microgravity, Gecko Gripper to test adhesives similar those found on geckos’ feet, Meteor will evaluate the chemical composition of meteors entering the Earth’s atmosphere, Saffire will purposely set a large fire inside Cygnus after it unberths from the ISS to examine how fires spread in space, and a nanosat deployer mounted externally will deploy over two dozen nanosats also after unberthing.
A new 3D printer featuring significantly upgraded capabilities is also on board.
The spacecraft will arrive at the station on Saturday, March 26, at which time Expedition 47 Commander Tim Kopra of NASA and Flight Engineer Tim Peake of ESA (European Space Agency) will grapple Cygnus, using the space station’s robotic arm, at approximately 6:40 a.m.
NASA TV coverage of rendezvous and grapple will begin at 5:30 a.m.
The Cygnus has been named the S.S. Rick Husband in honor of Col. Rick Husband, the late commander of Space Shuttle Columbia, which was tragically lost with its crew of seven NASA astronauts during re-entry on its final flight on Feb. 1, 2003.
Watch for Ken’s onsite launch reports direct from the Kennedy Space Center in Florida.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
KENNEDY SPACE CENTER, FL – A stunningly beautiful nighttime launch mesmerized delighted spectators as it roared off a Florida space coast launch pad late Tuesday night, March 22, on a mission for NASA stocked with over three tons of science and supplies bound for the multinational crews working aboard the International Space Station (ISS).
A United Launch Alliance (ULA) Atlas V rocketed raced to orbit from Cape Canaveral Air Force Station, Fl, carrying an enlarged Cygnus commercial resupply spacecraft on the Orbital ATK CRS-6 mission to the ISS.
The venerable Atlas V lifted off right on target at 11:05 p.m. EDT from Space Launch Complex 41 into a picturesque moonlit sky that magnificently illuminated the scattered thin clouds hovering over the seaside launch pad for the hordes of excited folks and families lining the beaches and lucky to witness what may be history’s last launch of a Cygnus from Florida.
Future liftoffs of the private Orbital ATK Cygnus supply truck designed to stock the station will return to their original launch site on Virginia’s eastern shore starting with the next mission for their NASA customer sometime this summer.
Cygnus launches to the ISS normally start from NASA’s Wallops Flight Facility in Virginia.
But a catastrophic failure of the Orbital ATK Antares rocket moments after liftoff on Oct. 28, 2014, forced Orbital to seek and book an alternative launch vehicle while the company redesigned and reengined Antares first stage with new powerful powerplants for the ride to orbit.
The Cygnus spacecraft will arrive at the station on Saturday, March 26, at which time Expedition 47 Commander Tim Kopra of NASA and Flight Engineer Tim Peake of ESA (European Space Agency) will grapple Cygnus, using the space station’s robotic arm, at approximately 6:40 a.m. NASA TV coverage of rendezvous and grapple will begin at 5:30 a.m.
The commercial Cygnus cargo freighter was built by Orbital ATK, based in Dulles, Virginia.
The Cygnus has been named the S.S. Rick Husband in honor of Col. Rick Husband, the late commander of Space Shuttle Columbia, which was tragically lost with its crew of seven NASA astronauts during re-entry on its final flight on Feb. 1, 2003.
This flight is also known as OA-6 and is being launched under terms of the firm’s Commercial Resupply Services (CRS) contract with NASA. It also counts as Orbital ATK’s fifth cargo delivery mission to the space station.
OA-6 is loaded with 3513 kg (7700 pounds) of science experiments and hardware, crew supplies, spare parts, gear and station hardware to the orbital laboratory in support over 250 research experiments being conducted on board by the Expedition 47 and 48 crews.
About a quarter of the cargo is devoted to science and research gear. The cargo includes 3279 kg of science investigations, 1139 kg of crew supplies, 1108 kg of vehicle hardware, 157 kg of spacewalk equipment, and 98 kg of computer resources.
Here a NASA description of a few of the scientific highlights:
– Gecko Gripper, testing a mechanism similar to the tiny hairs on geckos’ feet that lets them stick to surfaces using an adhesive that doesn’t wear off,
– Strata-1, designed to evaluate how soil on small, airless bodies such as asteroids behaves in microgravity.
– Meteor, an instrument to evaluate from space the chemical composition of meteors entering Earth’s atmosphere. The instrument is being re-flown following its loss on earlier supply missions.
– Saffire, which will set a large fire inside the Cygnus in an unprecedented study to see how large fires behave in space. The research is vital to selecting systems and designing procedures future crews of long-duration missions can use for fighting fires.
– Cygnus is carrying more than two dozen nanosatellites that will be ejected from either the spacecraft or the station at various times during the mission to evaluate a range of technology and science including Earth observations.
Here a cool video prelaunch look at Cygnus and me in the NASA Kennedy Space Center clean room discussing the Meteor experiment:
Video Credit: Thaddeus Cesari/VideoShampoo.com
When the ISS Expedition 47 crew members open the hatch, they will be greeted with a sign noting the spacecraft was named ‘SS Rick Husband’ in honor of the STS-107 mission commander.
Cygnus will spend approximately two months docked at the ISS.
OA-6 is only the second Cygnus to be launched atop a ULA Atlas V rocket, following the OA-4 mission last December.
The CRS-6/OA-6 flight is also the second flight of the enhanced Cygnus variant, that is over 1 meter longer and sports 50% more volume capability.
Thus it is capable of carrying a much heavier payload of some 3500 kg (7700 lbs) vs. a maximum of 2300 kg (5070 lbs) for the standard version.
Watch for Ken’s onsite launch reports direct from the Kennedy Space Center in Florida.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Learn more about Orbital ATK Cygnus, ISS, ULA Atlas rocket, SpaceX, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events:
Mar 21-23: “Orbital ATK Atlas/Cygnus launch to the ISS, ULA, SpaceX, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evening Mar 21 /late afternoon Mar 22/23
Volcanoes are renowned for their destructive power. In fact, there are few forces of nature that rival their sheer, awesome might, or have left as big of impact on the human psyche. Who hasn’t heard of tales of Mt. Vesuvius erupting and burying Pompeii? There’s also the Minoan Eruption, the eruption that took place in the 2nd millennium BCE on the isle of Santorini and devastated the Minoan settlement there.
In Japan, Hawaii, South American and all across the Pacific, there are countless instances of eruptions taking a terrible toll. And who can forget modern-day eruptions like Mount St. Helens? But would it surprise you to know that despite their destructive power, volcanoes actually come with their share of benefits? From enriching the soil to creating new landmasses, volcanoes are actually a productive force as well.
Soil Enrichment:
Volcanic eruptions result in ash being dispersed over wide areas around the eruption site. And depending on the chemistry of the magma from which it erupted, this ash will be contain varying amounts of soil nutrients. While the most abundant elements in magma are silica and oxygen, eruptions also result in the release of water, carbon dioxide (CO²), sulfur dioxide (SO²), hydrogen sulfide (H²S), and hydrogen chloride (HCl), amongst others.
In addition, eruptions release bits of rock such as potolivine, pyroxene, amphibole, and feldspar, which are in turn rich in iron, magnesium, and potassium. As a result, regions that have large deposits of volcanic soil (i.e. mountain slopes and valleys near eruption sites) are quite fertile. For example, most of Italy has poor soils that consist of limestone rock.
But in the regions around Naples (the site of Mt. Vesuvius), there are fertile stretches of land that were created by volcanic eruptions that took place 35,000 and 12,000 years ago. The soil in this region is rich because volcanic eruption deposit the necessary minerals, which are then weathered and broken down by rain. Once absorbed into the soil, they become a steady supply of nutrients for plant life.
Hawaii is another location where volcanism led to rich soil, which in turn allowed for the emergence of thriving agricultural communities. Between the 15th and 18th centuries on the islands of Kauai, O’ahu and Molokai, the cultivation of crops like taros and sweet potatoes allowed for the rise of powerful chiefdoms and the flowering of the culture we associate with Hawaii today.
Volcanic Land Formations:
In addition to scattering ash over large areas of land, volcanoes also push material to the surface that can result in the formation of new islands. For example, the entire Hawaiian chain of islands was created by the constant eruptions of a single volcanic hot spot. Over hundreds of thousands of years, these volcanoes breached the surface of the ocean becoming habitable islands, and rest stops during long sea journeys.
This is the case all across the Pacific, were island chains such as Micronesia, the Ryukyu Islands (between Taiwan and Japan), the Aleutian Islands (off the coast of Alaska), the Mariana Islands, and Bismark Archipelago were all formed along arcs that are parallel and close to a boundary between two converging tectonic plates.
Much the same is true of the Mediterranean. Along the Hellenic Arc (in the eastern Mediterranean), volcanic eruptions led to the creation of the Ionian Islands, Cyprus and Crete. The nearby South Aegean Arc meanwhile led to the formation of Aegina, Methana, Milos, Santorini and Kolumbo, and Kos, Nisyros and Yali. And in the Caribbean, volcanic activity led to the creation of the Antilles archipelago.
Where these islands formed, unique species of plants and animals evolved into new forms on these islands, creating balanced ecosystems and leading to new levels of biodiversity.
Volcanic Minerals and Stones:
Another benefits to volcanoes are the precious gems, minerals and building materials that eruptions make available. For instance, stones like pumice volcanic ash and perlite (volcanic glass) are all mined for various commercial uses. These include acting as abrasives in soaps and household cleaners. Volcanic ash and pumice are also used as a light-weight aggregate for making cement.
The finest grades of these volcanic rocks are used in metal polishes and for woodworking. Crushed and ground pumice are also used for loose-fill insulation, filter aids, poultry litter, soil conditioner, sweeping compound, insecticide carrier, and blacktop highway dressing.
Perlite is also used as an aggregate in plaster, since it expands rapidly when heated. In precast walls, it too is used as an aggregate in concrete. Crushed basalt and diasbase are also used for road metal, railroad ballast, roofing granules, or as protective arrangements for shorelines (riprap). High-density basalt and diabase aggregate are used in the concrete shields of nuclear reactors.
Hardened volcanic ash (called tuff) makes an especially strong, lightweight building material. The ancient Romans combined tuff and lime to make a strong, lightweight concrete for walls, and buildings. The roof of the Pantheon in Rome is made of this very type of concrete because it’s so lightweight.
Precious metals that are often found in volcanoes include sulfur, zinc, silver, copper, gold, and uranium. These metals have a wide range of uses in modern economies, ranging from fine metalwork, machinery and electronics to nuclear power, research and medicine. Precious stones and minerals that are found in volcanoes include opals, obsidian, fire agate, flourite, gypsum, onyx, hematite, and others.
Global Cooling:
Volcanoes also play a vital role in periodically cooling off the planet. When volcanic ash and compounds like sulfur dioxide are released into the atmosphere, it can reflect some of the Sun’s rays back into space, thereby reducing the amount of heat energy absorbed by the atmosphere. This process, known as “global dimming”, therefore has a cooling effect on the planet.
The link between volcanic eruptions and global cooling has been the subject of scientific study for decades. In that time, several dips have been observed in global temperatures after large eruptions. And though most ash clouds dissipate quickly, the occasional prolonged period of cooler temperatures have been traced to particularly large eruptions.
Because of this well-established link, some scientists have recommended that sulfur dioxide and other be released into the atmosphere in order to combat global warming, a process which is known as ecological engineering.
Hot Springs And Geothermal Energy:
Another benefit of volcanism comes in the form of geothermal fields, which is an area of the Earth characterized by a relatively high heat flow. These fields, which are the result of present, or fairly recent magmatic activity, come in two forms. Low temperature fields (20-100°C) are due to hot rock below active faults, while high temperature fields (above 100°C) are associated with active volcanism.
Geothermal fields often create hot springs, geysers and boiling mud pools, which are often a popular destination for tourists. But they can also be harnessed for geothermal energy, a form of carbon-neutral power where pipes are placed in the Earth and channel steam upwards to turn turbines and generate electricity.
In countries like Kenya, Iceland, New Zealand, the Phillipines, Costa Rica and El Salvador, geothermal power is responsible for providing a significant portion of the country’s power supply – ranging from 14% in Costa Rica to 51% in Kenya. In all cases, this is due to the countries being in and around active volcanic regions that allow for the presence of abundant geothermal fields.
Outgassing and Atmospheric Formation:
But by far, the most beneficial aspect of volcanoes is the role they play in the formation of a planet’s atmosphere. In short, Earth’s atmosphere began to form after its formation 4.6 billion eyars ago, when volcanic outgassing led to the creation of gases stored in the Earth’s interior to collect around the surface of the planet. Initially, this atmosphere consisted of hydrogen sulfide, methane, and 10 to 200 times as much carbon dioxide as today’s atmosphere.
After about half a billion years, Earth’s surface cooled and solidified enough for water to collect on it. At this point, the atmosphere shifted to one composed of water vapor, carbon dioxide and ammonia (NH³). Much of the carbon dioxide dissolved into the oceans, where cyanobacteria developed to consume it and release oxygen as a byproduct. Meanwhile, the ammonia began to be broken down by photolysis, releasing the hydrogen into space and leaving the nitrogen behind.
Another key role played by volcanism occurred 2.5 billion years ago, during the boundary between the Archaean and Proterozoic Eras. It was at this point that oxygen began to appear in our oxygen due to photosynthesis – which is referred to asthe “Great Oxidation Event”. However, according to recent geological studies, biomarkers indicate that oxygen-producing cyanobacteria were releasing oxygen at the same levels there are today. In short, the oxygen being produced had to be going somewhere for it not to appear in the atmosphere.
The lack of terrestrial volcanoes is believed to be responsible. During the Archaean Era, there were only submarine volcanoes, which had the effect of scrubbing oxygen from the atmosphere, binding it into oxygen containing minerals. By the Archaean/Proterozoic boundary, stabilized continental land masses arose, leading to terrestrial volcanoes. From this point onward, markers show that oxygen began appearing in the atmosphere.
Volcanism also plays a vital role in the atmospheres of other planets. Mercury’s thin exosphere of hydrogen, helium, oxygen, sodium, calcium, potassium and water vapor is due in part of volcanism, which periodically replenishes it. Venus’ incredibly dense atmosphere is also believed to be periodically replenished by volcanoes on its surface.
And Io, Jupiter’s volcanically active moon, has an extremely tenuous atmosphere of sulfur dioxide (SO²), sulfur monoxide (SO), sodium chloride (NaCl), sulfur monoxide (SO), atomic sulfur (S) and oxygen (O). All of these gases are provided and replenished by the many hundreds of volcanoes situated across the moon’s surface.
As you can see, volcanoes are actually a pretty creative force when all is said and done. In fact, us terrestrial organisms depend on them for everything from the air we breathe, to the rich soil that produces our food, to the geological activity that gives rise to terrestrial renewal and biological diversity.
The early Solar System was a much different place than it is now. Chaos reigned supreme before things settled down into their present state. New research shows that the young Sun was more chaotic and expressive than it is now, and that Earth’s magnetic field was key for the development of life on Earth.
Researchers at the Harvard Smithsonian Centre for Astrophysics have been studying a star called Kappa Ceti, about 30 light years away in the Cetus constellation. Kappa Ceti is in many ways similar to our own Sun, but it’s estimated to be between 400 million to 600 million years old, about the same age as our Sun when life appeared on Earth. Studying Kappa Ceti gives scientists a good idea of the type of star that early life on Earth had to contend with.
Kappa Ceti, at its young age, is much more magnetically active than our 4.6 billion year old Sun, according to this new research. It emits a relentless solar wind, which the research team at Harvard says is 50 times as powerful as the solar wind from our Sun. It’s surface is also much more active and chaotic. Rather than the sunspots that we can see on our Sun, Kappa Ceti displays numerous starspots, the larger brother of the sunspot. And the starspots on Kappa Ceti are much more numerous than the sunspots observed on the Sun.
We’re familiar with the solar flares that come from the Sun periodically, but in the early life of the Sun, the flares were much more energetic too. Researchers have found evidence on Kappa Ceti of what are called super-flares. These monsters are similar to the flares we see today, but can release 10 to 100 million times more energy than the flares we can observe on our Sun today.
So if early life on Earth had to contend with such a noisy neighbour for a Sun, how did it cope? What prevented all that solar output from stripping away Earth’s atmosphere, and killing anything alive? Then, as now, the Earth’s electromagnetic field protected it. But in the same way that the Sun was so different long ago, so was the Earth’s protective shield. It may have been weaker than it is now.
The researchers found that if the Earth’s magnetic field was indeed weaker, then the magnetosphere may have been only 34% to 48% as large as it is now. The conclusion of the study says “… the early magnetic interaction between the stellar wind and the young Earth planetary magnetic field may well have prevented the volatile losses from the Earth exosphere and created conditions to support life.”
Or, in plain language: “The early Earth didn’t have as much protection as it does now, but it had enough,” says Do Nascimento.
On March 8, 2016 (March 9 local time) the Moon briefly blocked the light from the Sun in what was the only total solar eclipse of the year. The event was visible across portions of southeast Asia, Indonesia, and Micronesia, and was observed by both skywatchers on the ground in person and those watching live online around the world. While to most the view was of a silhouetted Moon slowly carving away the disk of the Sun before totality revealed a shimmering corona, the view from space looking back at Earth showed the Moon’s dark shadow passing over islands, clouds, and sea.
All over the Earth, there is a buried layer of sediment rich in iridium called the Cretaceous Paleogene-Boundary (K-Pg.) This sediment is the global signature of the 10-km-diameter asteroid that killed off the dinosaurs—and about 50% of all other species—66 million years ago. Now, in an effort to understand how life recovered after that event, scientists are going to drill down into the site where the asteroid struck—the Chicxulub Crater off the coast of Mexico’s Yucatan Peninsula.
The end-Cretaceous extinction was a global catastrophe, and a lot is already known about it. We’ve learned a lot about the physical effects of the strike on the impact area from oil and gas drilling in the Gulf of Mexico. According to data from that drilling, released on February 5th in the Journal of Geophysical Research: Solid Earth, the asteroid that struck Earth displaced approximately 200,000 cubic km (48,000 cubic miles) of sediment. That’s enough to fill the largest of the Great Lakes—Lake Superior—17 times.
The Chicxulub impact caused earthquakes and tsunamis that first loosened debris, then swept it from nearby areas like present-day Florida and Texas into the Gulf basin itself. This layer is hundreds of meters thick, and is hundreds of kilometers wide. It covers not only the Gulf of Mexico, but also the Caribbean and the Yucatan Peninsula.
In April, a team of scientists from the University of Texas and the National University of Mexico will spend two months drilling in the area, to gain insight into how life recovered after the impact event. Research Professor Sean Gulick of the University of Texas Institute for Geophysics told CNN in an interview that the team already has a hypothesis for what they will find. “We expect to see a period of no life initially, and then life returning and getting more diverse through time.”
Scientists have been wanting to drill in the impact region for some time, but couldn’t because of commercial drilling activity. Allowing this team to study the region directly will build on what is already known: that this enormous deposit of sediment happened over a very short period of time, possibly only a matter of days. The drilling will also help paint a picture of how life recovered by looking at the types of fossils that appear. Some scientists think that the asteroid impact would have lowered the pH of the oceans, so the fossilized remains of animals that can endure greater acidity would be of particular interest.
The Chicxulub impact was a monumental event in the history of the Earth, and it was extremely powerful. It may have been a billion times more powerful than the atomic bomb dropped on Hiroshima. Other than the layer of sediment laid down near the site of the impact itself, its global effects probably included widespread forest fires, global cooling from debris in the atmosphere, and then a period of high temperatures caused by an increase in atmospheric CO2.
We already know what will happen if an asteroid this size strikes Earth again—global devastation. But drilling in the area of the impact will tell us a lot about how geological and ecological processes respond to this type of devastation.
CAPE CANAVERAL AIR FORCE STATION, FL – After enduring four launch scrubs caused by poor weather, misguided boaters, high level winds and propellant fueling problems, SpaceX put on a stunning sky show with tonight’s sunset blastoff of their private Falcon 9 rocket boosting the high powered SES-9 commercial telecommunications satellite to orbit.
KENNEDY SPACE CENTER, FL – NASA’s first ever ‘Year in Space’ astronaut Scott Kelly was in good shape and smiling broadly for the Earth bound photographers after safely returning to Earth from his orbiting home of the past year on the International Space Station (ISS), for a smooth touchdown in the steppes of Kazakhstan late Monday evening, March 1.
He soon jetted back to the USA for a grand arrival ceremony back home in Houston in the wee hours of the morning, today, March 3, 2016.
“Great to be back on Earth, said Kelly. “There’s no place like home!”
Kelly landed on US soil at Houston’s Ellington Field early this morning at about 2:30 a.m.
Kelly was welcomed back to the USA by Second Lady of the United States Dr. Jill Biden, Assistant to the President for Science and Technology Dr. John P. Holdren, NASA Administrator and former astronaut Charles Bolden, and Kelly’s identical twin brother and former NASA astronaut Mark Kelly.
Before departing the station after a 340 day stay, Kelly said that among the things he missed most on Earth were fresh air and food and freedom of movement. And swimming in his pool.
Well he quickly made good on those wishes and after arriving back home before daylight soon took a dip in his backyard pool.
Kelly posted a video of his pleasant pool plummet in all its glory on twitter: Tweets by StationCDRKelly
“Man, that feels good!” he exclaimed.
The long trip back home began after Kelly boarded his Russian Soyuz TMA-18M return capsule along with Russian cosmonaut crewmates Mikhail Kornienko and Sergey Volkov.
Kelly and his Russian cohort Mikhail Kornienko comprised the first ever crew to live and work aboard the ISS for a record breaking year-long mission aimed at taking concrete steps towards eventually dispatching human crews for multiyear-long expeditions to the surface of Mars and back.
Volkov spent a normal six month increment aboard the station.
Expedition 46 Commander Scott Kelly of NASA is seen after returning to Ellington Field, Thursday, March 3, 2016 in Houston, Texas after his return to Earth the previous day. Credit: NASA/Joel Kowsky
The goal of the 1 year ISS mission was to collect a variety of data on the effects of long duration weightlessness on the human body that will be used to formulate a human mission to Mars.
Kelly and Kornienko originally launched to the station on March 27, 2015 along with Russian crewmate Gennady Padalka.
The trio undocked from the station inside their cramped Soyuz capsule, pulled away, fired breaking thrusters and plummeted back to Earth a few hours later, surviving scorching reentry temperatures as the passed through the Earth atmosphere.
They safely landed in Kazakhstan at 11:26 p.m. EST on Tuesday night, March 1, 2016 (10:26 a.m. March 2 Kazakhstan time), concluding Expedition 46.
Kelly set an American record for longest time in space on a single mission by living and working for 340 days straight aboard the ISS.
Kelly and Kornienko share the history making distinction of comprising the first ever ‘1 Year Crew’ to serve aboard the massive Earth orbiting science research outpost in space.
With a cumulative total of 520 days in space, Kelly has amassed the most time for an American in space. Kornienko has accumulated 516 days across two flights, and Volkov has 548 days on three flights.
During the yearlong mission 10 astronauts and cosmonauts representing six different nations including the United States, Russia, Japan, Denmark, Kazakhstan and England lived aboard the space station.
The station currently remains occupied by a three person crew hailing from the US, Russia and England. A new three person crew launches later in March.
NASA’s next commercial resupply launch to the station is slated for March 22 by a United Launch Alliance Atlas V rocket carrying an Orbital ATK Cygnus cargo freighter with over 7000 pounds of fresh science experiments and crew supplies.
Stay tuned here for Ken’s continuing Earth and planetary science and human spaceflight news.
Learn more about SpaceX Falcon 9 rocket, ULA Atlas rocket, Orbital ATK Cygnus, ISS, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events:
Mar 4: “SpaceX, ULA, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings