Here’s Your Chance to Scream in Space

The STRaND-1 Smartphone Nanosatellite. Credit: Surry Satellite Technology

The first “Alien” movie was promoted with the celebrated tagline, “In space, no one can hear you scream.” But a group of students want to find out if this is really true, and they’re asking the public for help. Students from the University of Cambridge in the UK will be loading human screams onto a smartphone that will be launched into space in December 2012 on a nanosatellite. The screams will be played at maximum volume while the smartphone is in low Earth orbit, and at the same time as the phone will record the playback to test if it’s possible to capture the sound of screaming in space. They want the best screams possible, and so are inviting the public to submit their screams via video. There will also be public voting on the screams to determine which screams will go to space.

You know you’ve always wanted to do this…..

“Obviously, we’re not expecting to get much back, there may be some buzzing, but this is more about getting young people interested in satellites and acoustics, perhaps encouraging them to consider future study in science or engineering” said Edward Cunningham, a physics undergraduate at Churchill College and one of the members of the Cambridge University Space Flight group (CUSF).

What is actually being tested is verifying the capabilities of a smartphone to control a satellite in space. UK space company Surrey Satellite Technology and their STRaND (Surrey Training Research and Nanosatellite Demonstration) team ran a Facebook competition to find apps to go into orbit – and CUSF’s screaming app was one of the winners. STRaND-1 project is touted as the “World’s first SmartPhone Nanosatellite.”

Here’s a video showing the satellite:

The phone will run on Android’s open-source operating system, and a computer, built at the Surrey Space Centre, will test the vital statistics of the phone once in space. When all the tests are complete, the plan is to switch off the micro-computer and the smartphone will be used to operate parts of the satellite. At its lowest, the phone will orbit 400km above the Earth, roughly the same as the International Space Station.

“Modern smartphones are pretty amazing,” said Shaun Kenyon, the project manager at Surrey Satellite Technology. “We want to see if the phone works up there, and if it does, we want to see if the phone can control a satellite.”

To submit your scream, create a YouTube video and send it in at www.screaminspace.com.

Each video must be at most ten seconds long, and there will be ten winning screams which can be voted for by the public on the project’s website. Screams must be entered before midnight (UTC) on Sunday November 4, 2012. The winning videos will be announced later and loaded onto the phone for launch, which is scheduled before the end of this year.

Other winners in the STRaND-1 project were iTesa, which will record the magnitude of the magnetic field around the phone during orbit, a STRAND Data app will show satellite telemetry on the smartphone’s display which can be imaged by an additional camera on-board, and Postcards from Space and 360, a joint effort with an app that will take images using the smartphone’s camera and use the technology onboard the spacecraft to establish STRaND-1’s position.

Source: University of Cambridge
, Surrey Satellite

Cheops – A Little Satellite with Big Ideas

Caption: Artist impression of Cheops. Credit: University of Bern

Big isn’t always better. This is certainly true at ESA’s new Science Programme. They are looking to low cost, small scale missions that can be rapidly developed, in order to offer greater flexibility in response to new ideas from the scientific community, to complement the broader Medium- and Large-class missions. Back in March ESA called for ideas for dedicated, quick-turnaround missions focusing on key issues in space science. From 26 proposals submitted, ESA has now approved a new mission to be launched in 2017. Though small in scale this mission is big on ambition: to search for nearby habitable planets.

Cheops stands for CHaracterising ExOPlanets Satellite. It has a planned mission lifetime of 3.5 years during which it will operate in a Sun-synchronous low-Earth orbit at an altitude of 800 km, free from distortion by Earth’s atmosphere. It will target nearby, bright stars already known to have planets orbiting around them.

By high-precision monitoring of the star’s brightness, Cheops will search for signs of a ‘transit’ as a planet passes across the star’s face, it will also be able to look for smaller planets, impossible to see using ground based telescopes, around those stars.

While NASA’s Kepler mission has confirmed 77 planets so far, with another 2,321 candidate planets, not one is close enough to Earth to be analysed in detail. Cheops on the other hand, will be able to take accurate measurements of the radius of the planet. For those planets with a known mass, this will reveal the planet’s density and provide an indication of the internal structure. It will help scientists understand the formation of planets from ‘super-Earths’, a few times the mass of the Earth, up to Neptune-sized worlds. It will also identify planets with significant atmospheres which can then be analysed for signs of life by ground-based telescopes, and the next generation of space telescopes now being built, such as the ground-based European Extremely Large Telescope and the NASA/ESA/CSA James Webb Space Telescope.

“By concentrating on specific known exoplanet host stars, Cheops will enable scientists to conduct comparative studies of planets down to the mass of Earth with a precision that simply cannot be achieved from the ground,” said Professor Alvaro Giménez-Cañete, ESA Director of Science and Robotic Exploration.

The plan is for Cheops to be the first of a series of similar small missions, that can be rapidly developed at low cost to investigate new scientific ideas quickly. Cheops will be developed as a partnership between ESA and Switzerland, with a number of other ESA Member States delivering substantial contributions.

Find out more about Cheops here

ORBCOMM Satellite Launched by Falcon 9 Has Fallen to Earth

The OG2 satellite being prepared for testing. Credit: ORBCOMM

The satellite that was launched to orbit as a secondary payload by the SpaceX Falcon 9 rocket on October 7, 2012 has deorbited, falling back to Earth. The ORBCOMM OG2 satellite was a prototype communications satellite that was launched along with the Dragon capsule for the CRS-1 resupply mission to the International Space Station. The satellite was sent into the wrong orbit as a result of “a pre-imposed safety check required by NASA,” ORBCOMM said today in a press release, after the engine anomaly where one of the rocket’s nine Merlin engines, Engine 1, lost pressure suddenly and an engine shutdown command was issued. The rocket was prevented from performing a second burn for safety reasons and the satellite was left in a lower orbit than intended.

“The safety check was designed to protect the International Space Station and its crew,” the ORBCOMM press release said. “Had ORBCOMM been the primary payload on this mission, as planned for the upcoming launches, we believe the OG2 prototype would have reached the desired orbit.”

ORBCOMM had said earlier they were checking into the possibility of whether onboard propulsion could be used to boost the OG2 into a higher orbit, but obviously that was unsuccessful. They did say today, however that while the OG2 was in orbit for its much-shortened time frame, they were able to obtain engineering data and “made significant strides in testing various hardware components,” including an antenna that was deployed and basic functions of the satellite that were successfully turned on.

The company added that with the verifications they were able to achieve, they can now forge ahead and focus on completing and launching the more OG2 satellites, and they plan on using SpaceX to deliver them to orbit. But next time the satellites will be the primary mission payloads on two planned Falcon 9 launches, one in mid-2013 and another in 2014, putting them directly into their operational orbit.

“We appreciate the complexity and work that SpaceX put into this launch,” stated Marc Eisenberg, ORBCOMM’s CEO. “SpaceX has been a supportive partner, and we are highly confident in their team and technology.”

The OG2 satellite was supposed be in a final 750×750 km orbit, but the company didn’t verify the orbit it did end up in. According to Jonathan’s Space Report, OG2 was ejected at 0137 UTC into a 203×323 km orbit, instead of its planned 350×750 km insertion orbit. Another satellite tracker, T.S. Kelso said via Twitter that it was in a 318 x 194km orbit.

A call to ORBCOMM to verify the orbit and location of de-orbit wasn’t immediately returned.

Huge Volcano Plume Seen from Space

The Shiveluch volcano as seen by the Aqua satellite on October 6, 2012. Credit: NASA

It’s almost like this volcano has an on/off switch. The Shiveluch Volcano in the northern Russian peninsula of Kamchatka had been quiet, and an earlier image taken by NASA’s Terra satellite (below) at about noon local time (00:00 UTC) on October 6, 2012, showed a quiet volcano with no activity. But just two hours later when the Aqua satellite passed over the area, the volcano had erupted and sent a plume of ash over about 90 kilometers (55 miles). Later, a local volcanic emergency response team reported that the ash plume from Shiveluch reached an altitude of 3 kilometers (9,800 feet) above sea level, and had traveled some 220 kilometers (140 miles) from the volcano summit.

The same volcano seen by the Terra satellite just two hours earlier on the same day. Credit: NASA

Shiveluch is one the biggest and most active volcanoes in this region and rises 3,283 meters (10,771 feet) above sea level. NASA’s Earth Observatory website says Shiveluch is a stratovolcano composed of alternating layers of hardened lava, compacted ash, and rocks ejected by previous eruptions. It has had numerous eruptions the past 200 years, but has been active during much of its life – estimates are the volcano is 60,000 to 70,000 years old.

The beige-colored expanse of rock on the volcano’s southern slopes (visible in both images) is due to an explosive eruption that occurred in 1964. Another eruption started in 1999 and lasted for over 10 years.

Source: NASA Earth Observatory

Surreal Photos: CubeSats Launched from the Space Station

Three small CubeSats are deployed from the International Space Station on October 4, 2012. Credit: NASA

Five tiny CubeSats were deployed from the International Space Station on Thursday and astronaut Chris Hadfield called the image above “surreal” on Twitter. And rightly so, as they look like a cross between Star Wars training droids and mini Borg Cubes from Star Trek. The Cubesats measure about 10 centimeters (4 inches) on a side and each will conduct a range of scientific missions, ranging from Earth observation and photography to technology demonstrations to sending LED pulses in Morse Code (which should be visible from Earth) to test out a potential type of optical communication system.

These are low-cost satellites that could be the wave of the future to enable students and smaller companies to send equipment into space. If you’re worried about these tiny sats creating more space junk, Hadfield assured that since they are very light and in such a low orbit, the Cubesat orbits will decay within a few months.

The Rubic-cube-sized Cubesats were deployed from the new Japanese Small Satellite Orbital Deployer that was brought to the space station in July by the Japanese HTV cargo carrier.

The Japanese FITSAT-1 will investigate the potential for new kinds of optical communication by transmitting text information to the ground via pulses of light set to Morse code. The message was originally intended to be seen just in Japan, but people around the world have asked for the satellite to communicate when it overflies them, said Takushi Tanaka, professor at The Fukuoka Institute of Technology.

Observers, ideally with binoculars, will be able to see flashes of light — green in the northern hemisphere, where people will see the “front” of the satellite, and red in the southern hemisphere, where the “back” will be visible.

The message it will send is “Hi this is Niwaka Japan.” Niwaka is the satellite’s nickname and reflects a play on words in the local dialect of southwestern Japan, according to an article on Discovery Space. To see the Morse Code message, the Cubesat will be near the ISS, so find out when you can see the ISS from NASA or Heaven’s Above. Find out more about the FITSAT at this website.

The other Cubesats include NASA’s TechEdSat which carries a ham radio transmitter and was developed by a group of student interns from San Jose State University (SJSU) in California with mentoring and support from staff at NASA’s Ames Research Center.

“TechEdSat will evaluate plug-and-play technologies, like avionics designed by commercial providers, and will allow a group of very talented aerospace engineering students from San Jose State University to experience a spaceflight project from formulation through decommission of a small spacecraft,” said Ames Director S. Pete Worden.

The other Cubesats include RAIKO, which will do photography from space, We Wish, an infrared camera for environmental studies, and and the F-1 Vietnam Student CubeSat which has an on-board camera for Earth observation.

See more cool-looking images and video of the deployement below (all images credit the Expedition 32 crew from the ISS/NASA):

Liftoff! Delta IV Launches Next Generation GPS Satellite

A Delta IV rocket launched from Florida today, sending a next-generation Global Positioning System satellite into orbit. The rocket lifted off at 12:10 UTC with the GPS IIF-3 satellite that will be part of the GPS system that is used by both civilians and the military. The new satellite will replace a 19-year-old navigation satellite in the global system that includes 31 operational satellites on-orbit which broadcast position, navigation and timing information to people around the world.

A United Launch Alliance Delta IV stands ready for launch at Space Launch complex 37 with the GPS IIF-3 satellite. Credit: ULA

The satellite, built by Boeing, is the third of 12 planned launches to provide improved GPS signals, featuring improved anti-jam technology, more precise atomic clocks, an upgraded civilian channel for commercial aviation and on-board processors that can be reprogrammed in flight, according to CBS News.

The new satellite should be operational by November.

Manhattan-Sized Ice Island Heads Out to Sea

An “ice island” that calved from the Petermann Glacier in July is seen by NASA satellite (MODIS/Terra)

Remember that enormous slab of ice that broke off Greenland’s Petermann Glacier back in July? It’s now on its way out to sea, a little bit smaller than it was a couple of months ago — but not much. At around 10 miles long and 4.6 miles across (16.25 x 7.5 km) this ice island is actually a bit shorter than Manhattan, but is fully twice as wide.

The image above was acquired on September 14 by the Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA’s Terra satellite.

Although the calving of this particular ice island isn’t thought to be a direct result of increasing global temperatures, climate change is thought to be a major factor in this year’s drop in Arctic sea ice extent, which is now below 4.00 million square kilometers (1.54 million square miles). Compared to September conditions in the 1980s and 1990s, this represents a 45% reduction in the area of the Arctic covered by sea ice.

Arctic sea ice extent data for June-July 2012 (NSIDC)

This year sea ice in the Arctic Ocean dropped below the previous all-time record, set in 2007. 2012 also marks the first time that there has been less than 4 million square kilometers (1.54 million square miles) of sea ice since satellite observations began in 1979.

The animation below, released today by the NOAA, shows the 2012 time-series of ice extent using data from the DMSP SSMI/S satellite sensor:

Read more here.

Satellite View of Guatemalan Volcano Erupting

A natural-color image captured the eruption of Volcan de Fuego as it occurred. Credit: NASA/Moderate Resolution Imaging Spectroradiometer (MODIS) aboard the Terra satellite.

One of Central American’s most active volcanos erupted on September 13th, 2012 prompting officials to evacuate 35,000 residents in Guatemala. The Volcan de Fuego, or Fire Volcano, began belching out ash at 10 a.m. local time with ash now falling up to 40 kilometers (25 miles) from the volcano. Residents within 20 kilometers (12 miles) of the volcano were being removed from the area in buses and cars.

According to the Coordinadora Nacional para la Reducción de Desastres (CONRED), the eruption included ash emissions to the west and a 500-meter (2,000-foot) long lava flow. CONRED also warned of pyroclastic flows that could descend the mountain in any direction.

This natural-color image captured the eruption just as it occurred, NASA said. The image was acquired by the Moderate Resolution Imaging Spectroradiometer (MODIS) aboard the Terra satellite.

Thursday’s eruption was the sixth of the year for this volcano and some officials said it may be the biggest.

NASA said they would publish imagery of Guatemala two times per day on the MODIS Rapid Response web site.

Sources: NASA’s Earth Observatory, CNN

Is Triton Hiding an Underground Ocean?

Voyager 2 mosaic of Neptune’s largest moon, Triton (NASA)

At 1,680 miles (2,700 km) across, the frigid and wrinkled Triton is Neptune’s largest moon and the seventh largest in the Solar System. It orbits the planet backwards – that is, in the opposite direction that Neptune rotates – and is the only large moon to do so, leading astronomers to believe that Triton is actually a captured Kuiper Belt Object that fell into orbit around Neptune at some point in our solar system’s nearly 4.7-billion-year history.

Briefly visited by Voyager 2 in late August 1989, Triton was found to have a curiously mottled and rather reflective surface nearly half-covered with a bumpy “cantaloupe terrain” and a crust made up of mostly water ice, wrapped around a dense core of metallic rock. But researchers from the University of Maryland are suggesting that between the ice and rock may lie a hidden ocean of water, kept liquid despite estimated temperatures of  -97°C (-143°F), making Triton yet another moon that could have a subsurface sea.

How could such a chilly world maintain an ocean of liquid water for any length of time? For one thing, the presence of ammonia inside Triton would help to significantly lower the freezing point of water, making for a very cold — not to mention nasty-tasting — subsurface ocean that refrains from freezing solid.

In addition to this, Triton may have a source of internal heat — if not several. When Triton was first captured by Neptune’s gravity its orbit would have initially been highly elliptical, subjecting the new moon to intense tidal flexing that would have generated quite a bit of heat due to friction (not unlike what happens on Jupiter’s volcanic moon Io.) Although over time Triton’s orbit has become very nearly circular around Neptune due to the energy loss caused by such tidal forces, the heat could have been enough to melt a considerable amount of water ice trapped beneath Triton’s crust.

Related: Titan’s Tides Suggest a Subsurface Sea

Another possible source of heat is the decay of radioactive isotopes, an ongoing process which can heat a planet internally for billions of years. Although not alone enough to defrost an entire ocean, combine this radiogenic heating with tidal heating and Triton could very well have enough warmth to harbor a thin, ammonia-rich ocean beneath an insulating “blanket” of frozen crust for a very long time — although eventually it too will cool and freeze solid like the rest of the moon. Whether this has already happened or still has yet to happen remains to be seen, as several unknowns are still part of the equation.

“I think it is extremely likely that a subsurface ammonia-rich ocean exists in Triton,” said Saswata Hier-Majumder at the University of Maryland’s Department of Geology, whose team’s paper was recently published in the August edition of the journal Icarus. “[Yet] there are a number of uncertainties in our knowledge of Triton’s interior and past which makes it difficult to predict with absolute certainty.”

Still, any promise of liquid water existing elsewhere in large amounts should make us take notice, as it’s within such environments that scientists believe lie our best chances of locating any extraterrestrial life. Even in the farthest reaches of the Solar System, from the planets to their moons, into the Kuiper Belt and even beyond, if there’s heat, liquid water and the right elements — all of which seem to be popping up in the most surprising of places — the stage can be set for life to take hold.

Read more about this here on Astrobiology.net.

Inset image: Voyager 2 portrait of Neptune and Triton taken on August 28, 1989. (NASA)

Satellites Keep Track of Hurricane Isaac

This visible image of Tropical Storm Isaac taken from NOAA’s GOES-13 satellite shows the huge extent of the storm, where the eastern-most clouds lie over the Carolinas and the western-most clouds are brushing east Texas. The image was captured on Tuesday, Aug. 28, 2012 at 10:25 a.m. EDT. Image Credit: NASA GOES Project

As expected Tropical Storm Isaac has now become a full-fledged hurricane, after being fed by the warm waters in the Gulf of Mexico. The slow moving storm is now closing in on the Louisiana-Mississippi coast and could make landfall in the region seven years to the day after Hurricane Katrina devastated the same area. It is not expected to be another Katrina, but with the slowness of the storm — about 16 km/h (10 mph) — forecasters are predicting 7-14 inches of rainfall across the coast as well as inland regions, and some places could even see 20 inches. Flooding from rainfall and storm surges are expected, according to NOAA. Satellites have been keeping an eye on the storm, and above is an image from one of the GOES satellites taken on Tuesday, August 28. Below are more satellite views.

The Proba-2 satellite’s X-Cam – Exploration Camera – acquired this image at 11:38:33 GMT on August 27, 2012. Credit: ESA

The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite captured this natural-color image of Isaac over the Gulf of Mexico at 2:00 p.m. CDT on August 27, 2012. Credit: NASA

Here’s a screenshot of Weather.com’s Hurricane Tracker for Isaac. Click here to see up-to-the-minute details on Isaac.

Sources: NOAA, NASA, ESA