NASA Archives

October 27, 2014June 5, 2022 by Ken Kremer

Orbital Antares GO to WOW US East Coast Spectators for 1st Night Launch on Oct. 27

Antares rocket stands erect, reflecting off the calm waters the night before a launch from NASA’s Wallops Flight Facility, VA, on Oct. 28, 2014. Credit: Ken Kremer/kenkremer.com

NASA WALLOPS FLIGHT FACILITY, VA – An Orbital Sciences Corp. commercial Antares rocket was given the GO for its first night launch on Oct. 27, following a launch readiness review on Sunday, Oct. 26, between managers from Orbital Sciences Corp. of Dulles, Virginia, and NASA.

The rocket was rolled to the launch pad and erected. Technicians are putting the final touches on the rocket to prepare it for flight to the International Space Station (ISS).

NASA and Orbital Sciences are targeting Antares for blastoff at 6:45 p.m. EDT on Oct. 27 from beachside Launch Pad 0A at the Mid-Atlantic Regional Spaceport (MARS) at NASA Wallops Island Flight Facility on Virginia’s eastern shore.

There is a 10 minute launch window to get Antares off the ground as the launch pad moves into the plane of the space stations orbit. The slightly longer launch window is due to the extra thrust available from using a new, more powerful ATK built upper stage engine.

Technicians processing Antares rocket on Oct 26 to prepare for first night launch from NASA’s Wallops Flight Facility, VA, on Oct. 27 at 6:45 p.m. Credit: Ken Kremer – kenkremer.com

The rare spectacle of a night launch within view of tens of millions could WOW hordes of US East Coast residents in densely populated areas up and down the Atlantic shoreline – weather permitting.

The current forecast calls for an almost unheard of 98% chance of favorable weather conditions at launch time.

Depending on local weather conditions, the Antares blastoff will be visible along much of the US eastern seaboard – stretching from Maine to South Carolina.

For precise viewing locations and sighting times, see the collection of detailed maps and trajectory graphics courtesy of Orbital Sciences and NASA in my prior story with a complete viewing guide on “How to See the Antares Launch.”

Antares is carrying Orbital’s privately developed Cygnus pressurized cargo freighter loaded with nearly 5000 pounds (2200 kg) of science experiments, research instruments, crew provisions, spare parts, spacewalk and computer equipment and gear on a critical resupply mission dubbed Orb-3 bound for the International Space Station (ISS).

Orbital Sciences Antares rocket stand erect and ready for blastoff the day before its first night launch from NASA’s Wallops Flight Facility, VA, targeted for Oct. 27 at 6:45 p.m. Credit: Ken Kremer – kenkremer.com — Orbital Sciences Antares rocket stands erect and ready for blastoff the day before its first night launch from NASA’s Wallops Flight Facility, VA, targeted for Oct. 27 at 6:45 p.m. Credit: Ken Kremer – kenkremer.com

This is the heaviest cargo load yet lofted by a Cygnus. Some 800 pounds additional cargo is loaded on board compared to earlier flights, that’s enabled by using the more powerful ATK CASTOR 30XL second stage for the first time.

Research gear and experiments account for about 1600 pounds (720 kg), or about one third of Cygnus total cargo load.

Among the items aboard are 32 cubesats and deployers, a 6000 psi high pressure replacement nitrogen tank needed for spacewalks from the Quest airlock, experiments enabling the first space-based observations of meteors entering Earth’s atmosphere, determination of how blood flows from the brain to the heart in the absence of gravity, investigations on the impact of space travel on both the human immune system and an individual’s microbiome, the collection of microbes that live in and on the human body, and student science investigations from the SSEP/NCESSE.

“There is nothing more exciting than spaceflight,” said Frank Culbertson, Orbital’s executive vice president of the advanced programs group, at a pre-launch briefing at NASA Wallops.

“It is important to inspire the next generation of scientists. We need to keep the kids inspired to study math and science and keep going back to space. If we stop going to space, it will be very hard to restart.”

On-Ramp to the Orbital Sciences Antares rocket and International Space Station - ready for blastoff the day before its first night launch from NASA’s Wallops Flight Facility, VA, targeted for Oct. 27 at 6:45 p.m. Credit: Ken Kremer – kenkremer.com — On-Ramp to the Orbital Sciences Antares rocket and International Space Station – ready for blastoff the day before its first night launch from NASA’s Wallops Flight Facility, VA, targeted for Oct. 27 at 6:45 p.m. Credit: Ken Kremer – kenkremer.com

This Cygnus resupply module, dubbed “SS Deke Slayton,” honors one of America’s original Mercury 7 astronauts, Donald “Deke” K. Slayton. He flew on the Apollo-Soyuz Test Project mission in 1975 and championed commercial space endeavors after retiring from NASA in 1982. Slayton passed away in 1993.

The Orbital-3, or Orb-3, mission is the third of eight cargo resupply missions to the ISS through 2016 under the NASA Commercial Resupply Services (CRS) contract award valued at $1.9 Billion.

Orbital Sciences is under contract to deliver 20,000 kilograms of research experiments, crew provisions, spare parts and hardware for the eight ISS flight.

NASA Television will broadcast live coverage of the launch, including pre- and post-launch briefings and arrival at the station. Launch coverage begins at 5:45 p.m. EDT.

NASA will broadcast the Antares launch live on NASA TV starting at 5:45 p.m. Monday – http://www.nasa.gov/nasatv

You can also watch the pre- and post launch briefings on Monday on NASA TV.

Of course the absolute best viewing will be locally in the mid-Atlantic region closest to Wallops Island.

Locally at Wallops you’ll get a magnificent view and hear the rockets thunder at the NASA Wallops Visitor Center or other local spots around the Chincoteague National Wildlife Refuge area.

For more information about the Wallops Visitors Center, including directions, see: http://www.nasa.gov/centers/wallops/visitorcenter

Watch here for Ken’s onsite reporting direct from NASA Wallops.

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

Ken Kremer

…………….

Learn more about Commercial Space, Orion and NASA Human and Robotic Spaceflight at Ken’s upcoming presentations:

Oct 27/28: “Antares/Cygnus ISS Rocket Launch from Virginia”; Rodeway Inn, Chincoteague, VA

October 25, 2014June 5, 2022 by Ken Kremer

How to Watch Spectacular 1st Nighttime Antares Launch to ISS on Oct. 27 – Complete Viewing Guide

NASA WALLOPS FLIGHT FACILITY, VA – Tens of millions of US East Coast residents can expect a dinnertime spectacular for the first ever nighttime launch of the commercial Orbital Sciences Corp. Antares rocket slated to blastoff on Monday evening, October 27, from a beachside NASA launch base along the eastern shore of Virginia – if the weather holds as currently forecast.

You can watch live, below.

Antares is carrying Orbital’s private Cygnus cargo freighter loaded with a diverse array of science experiments on a critical cargo resupply mission named Orb-3, and is bound for the International Space Station (ISS).

Broadcast live streaming video on Ustream

NASA and Orbital Sciences are now targeting liftoff at 6:45 p.m. EDT on Oct. 27 from Launch Pad 0A at the Mid-Atlantic Regional Spaceport (MARS) at NASA Wallops Island Flight Facility on Virginia’s shore.

Viewing over New York City from River Road in North Bergen, New Jersey, looking south . Credit: Orbital Sciences Corp.

The launch to the ISS was delayed three days due to Hurricane Gonzalo and its direct hit on the island of Bermuda which is also home to a critical rocket tracking station – as reported here. The tracking is required to ensure public safety.

If you have never seen a rocket launch, this could be the one for you – especially since its conveniently in the early evening and you don’t have to take the long trek to the Kennedy Space Center in Florida.

Here’s our complete guide on “How to See the Antares/Cygnus Oct. 27 Blastoff” – chock full of viewing maps and trajectory graphics (above and below) from a variety of prime viewing locations, including historic and notable landmarks Washington, DC, NYC, New Jersey, Maryland, Virginia, and more.

Viewing the launch across the tidal basin from the MLK Jr. Memorial in Washington, D.C. Credit: Orbital Sciences Corp.

Depending on local weather conditions, the Antares blastoff will be visible along much of the US eastern seaboard – stretching from Maine to South Carolina.

For precise viewing locations and sighting times, see the collection of detailed maps and trajectory graphics courtesy of Orbital Sciences and NASA.

Antares first night launch will also be visible to some inland regions, including portions of New England, Pennsylvania, and West Virginia.

Of course the absolute best viewing will be locally in the mid-Atlantic region closest to Wallops Island.

Antares rocket and Cygnus spacecraft await launch on Orb 2 mission on July 13, 2014 from Launch Pad 0A at NASA Wallops Flight Facility Facility, VA. LADEE lunar mission launch pad 0B stands adjacent to right of Antares. Credit: Ken Kremer - kenkremer.com — Antares rocket and Cygnus spacecraft await launch on Orb 2 mission on July 13, 2014, from Launch Pad 0A at NASA Wallops Flight Facility Facility, VA. LADEE lunar mission launch pad 0B stands adjacent to right of Antares. Credit: Ken Kremer – kenkremer.com

Locally at Wallops you’ll get a magnificent view and hear the rockets thunder at either the NASA Wallops Visitor Center or the Chincoteague National Wildlife Refuge/Assateague National Seashore.

For more information about the Wallops Visitors Center, including directions, see: http://www.nasa.gov/centers/wallops/visitorcenter

The pressurized Cygnus cargo spacecraft is loaded with some 5,000 pounds of research experiments, top notch student science investigations from the NCESSE/SSEP, supplies, spare parts, and crew provisions on what will be the fourth Cygnus flight overall, including a demonstration flight in 2013.

Student Space Flight teams at NASA Wallops. Science experiments from these students representing 15 middle and high schools across America were selected to fly aboard the Orbital Sciences Cygnus Orb-2 spacecraft which launched to the ISS from NASA Wallops, VA, on July 13, 2014, as part of the Student Spaceflight Experiments Program (SSEP). Credit: Ken Kremer - kenkremer.com — Student Space Flight teams at NASA Wallops. Science experiments from these students representing 15 middle and high schools across America were selected to fly aboard the Orbital Sciences Cygnus Orb-2 spacecraft which launched to the ISS from NASA Wallops, VA, on July 13, 2014, as part of the Student Spaceflight Experiments Program (SSEP). Credit: Ken Kremer – kenkremer.com

This is the heaviest Cygnus cargo load to date because the Antares rocket is outfitted with a more powerful second stage from ATK – for the first time.

Altogether eight operational resupply missions will be flown for NASA under the Commercial Resupply Services (CRS) contract. That’s the same contract NASA has with SpaceX and that company’s just completed Dragon CRS-4 mission which ended with a successful Pacific Ocean splashdown on Saturday, Oct. 25 – as I reported here.

Viewing the launch from the boardwalk at Virginia Beach, VA. Credit: Orbital Sciences Corp.

It is the third of eight cargo resupply missions to the ISS under Orbital’s Commercial Resupply Services (CRS) contract with NASA through 2016.

The Orbital-3, or Orb-3, mission is the third of the eight cargo resupply missions to the ISS under the NASA CRS award valued at $1.9 Billion.

NASA Television will broadcast live coverage of the event, including pre- and post-launch briefings and arrival at the station. Launch coverage begins at 5:45 p.m. Monday – http://www.nasa.gov/nasatv

You can also watch the pre- and post launch briefing on Sunday and Monday on NASA TV.

What the Antares launch will look like from Fells Point in Baltimore, MD. Credit: Orbital Sciences Corp.

The weather prognosis is currently very favorable with a greater than a 90% chance of acceptable weather conditions at launch time.

Watch here for Ken’s onsite reporting direct from NASA Wallops.

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

Ken Kremer

…………….

Learn more about Commercial Space, Orion and NASA Human and Robotic Spaceflight at Ken’s upcoming presentations:

Oct 26/27: “Antares/Cygnus ISS Rocket Launch from Virginia”; Rodeway Inn, Chincoteague, VA

What the Antares launch will look like over the Port of Baltimore, MD. Credit: Orbital Sciences Corp.

What the Antares launch will look looking south over Heritage Commission in Dover, DE. Credit: Orbital Sciences Corp.

Viewing the launch from looking East from the University of Virginia, Charlottesville, VA. Credit: Orbital Sciences Corp.

Orbital Sciences Corporation Antares rocket and Cygnus spacecraft blasts off on July 13 2014 from Launch Pad 0A at NASA Wallops Flight Facility , VA, on the Orb-2 mission and loaded with over 3000 pounds of science experiments and supplies for the crew aboard the International Space Station. Credit: Ken Kremer - kenkremer.com — Orbital Sciences Corporation Antares rocket and Cygnus spacecraft blasts off on July 13, 2014, from Launch Pad 0A at NASA Wallops Flight Facility , VA, on the Orb-2 mission and loaded with over 3000 pounds of science experiments and supplies for the crew aboard the International Space Station. Credit: Ken Kremer – kenkremer.com

October 25, 2014June 5, 2022 by Ken Kremer

SpaceX Dragon Departs Space Station after Delivering Slew of Science and Returns with Ocean Splashdown

A space-weathered @SpaceX #Dragon looking great moments before release today. Credit: NASA/Reid Wiseman

Concluding a busy five week mission, the SpaceX Dragon CRS-4 commercial cargo ship departed the International Space Station (ISS) this morning, Oct. 25, after delivering a slew of some 2.5 tons of ground breaking science experiments and critical supplies that also inaugurated a new era in Earth science at the massive orbiting outpost following installation of the ISS-RapidScat payload.

Dragon was released from the snares of the station’s robotic arm at 9: 57 a.m. EDT while soaring some 250 mi (400 km) over the northwest coast of Australia.

It returned safely to Earth with a splashdown in the Pacific Ocean some six hours later, capping the fourth of SpaceX’s twelve contracted station resupply missions for NASA through 2016.

“The Dragon is free!” exclaimed NASA commentator Rob Navias during a live broadcast on NASA TV following the ungrappling this morning. “The release was very clean.”

Dragon released from snares of ISS robotic arm on Oct. 25, 2014 for return to Earth. Credit: NASA — Dragon released from snares of ISS robotic arm on Oct. 25, 2014, for return to Earth. Credit: NASA

The private resupply ship was loaded for return to Earth with more than 3,276 pounds of NASA cargo and science samples from the station crew’s investigations on “human research, biology and biotechnology studies, physical science investigations, and education activities sponsored by NASA and the Center for the Advancement of Science in Space, the nonprofit organization responsible for managing research aboard the U.S. national laboratory portion of the space station,” said NASA.

The release set up a quick series of three burns by the ship’s Draco thrusters designed to carry Dragon safely away from the station.

NASA astronauts Reid Wiseman and Butch Wilmore quickly retracted the arm working from their robotics workstation in the domed Cupola module.

“Thanks for the help down there,” the astronauts radioed. “It was a great day.”

Dragon moves away from ISS on Oct. 25, 2014 for return to Earth. Credit: NASA TV — Dragon moves away from ISS on Oct. 25, 2014, for return to Earth. Credit: NASA TV

The first burn took place a minute later at about 9:58 a.m. EDT and the second at about 10:00 a.m. A yaw maneuver at 10:05 a.m. set up the orientation required for the third burn at about 10:08 a.m.

Dragon moved away quickly during the nighttime release and was already outside the Keep Out Sphere (KOS), an imaginary bubble surrounding the station at a distance of 200 m. It disappeared quickly in the dark and was barely visible within minutes.

“The propulsion systems are in good shape,” said Navias. “All systems on Dragon are functioning perfectly.”

With Dragon safely gone following the trio of burns, the next major event was the deorbit burn at 2:43 p.m. EDT at a distance of about 90 statute miles from the station.

Dragon slipped out of orbit. After surviving the scorching heat of reentry through the Earth’s atmosphere, the ship sequentially deployed its drogue chutes and three main parachutes at about 3:30 p.m.

Splashdown in the Pacific Ocean occurred as expected at about 3:39 p.m., approximately 265 miles west of the Baja peninsula.

Dragon is the only vehicle that can return intact from the ISS with a substantial load of cargo and is carrying critical science samples for distribution to researchers.

Today’s Dragon departure starts a week of heavy traffic of comings and goings to the ISS involving a series of US and Russian unmanned cargo ships.

SpaceX Dragon captures view of ISS after departure on Oct. 25, 2014 for return to Earth. Credit: NASA TV — SpaceX Dragon captures view of ISS after departure on Oct. 25, 2014, for return to Earth. Credit: NASA TV

The Orbital Sciences Antares rocket with the commercial Cygnus cargo freighter is set to launch on Monday, Oct. 27, from NASA Wallops, VA. It will dock at the ISS on Nov. 2 at the Earth-facing port on the Harmony module just vacated by Dragon.

Russia’s Progress 56 unmanned cargo ship will also undock on Oct. 27. And Progress 57 will launch from Baikonur on Wednesday, Oct 29.

The SpaceX Dragon CRS-4 cargo resupply mission thundered to space on the company’s Falcon 9 rocket from Space Launch Complex-40 at Cape Canaveral Air Force Station in Florida on Sept. 21.

A SpaceX Falcon 9 rocket carrying a Dragon cargo capsule packed with science experiments and station supplies blasts off from Space Launch Complex 40 at Cape Canaveral Air Force Station, Florida, at 1:52 a.m. EDT on Sept. 21, 2014 bound for the ISS. Credit: Ken Kremer/kenkremer.com — A SpaceX Falcon 9 rocket carrying a Dragon cargo capsule packed with science experiments and station supplies blasts off from Space Launch Complex 40 at Cape Canaveral Air Force Station, Florida, at 1:52 a.m. EDT on Sept. 21, 2014, bound for the ISS. Credit: Ken Kremer/kenkremer.com

Dragon was successfully berthed at the Harmony module on Sept. 23, 2014.

Among the nearly 5000 pounds of cargo hauled up by Dragon was as an Earth observation platform named ISS-RapidScat loaded in the unpressurized trunk section.

Also loaded aboard were a slew of science experiments, spare parts, crew provisions, food, clothing and supplies to the six person crews living and working aboard the ISS soaring in low Earth orbit under NASA’s Commercial Resupply Services (CRS) contract.

It also carried the first 3-D printer to space for the first such space based studies ever attempted by the astronaut crews. The printer will remain at the station for at least the next two years.

20 mice housed in a special rodent habitat were also aboard, as well as fruit flies.

The ISS Rapid Scatterometer, or ISS-RapidScat, is NASA’s first research payload aimed at conducting near global Earth science from the station’s exterior and will be augmented with others in coming years.

ISS-RapidScat instrument, shown in this artist's rendering, was launched to the International Space Station aboard the SpaceX CRS-4 mission on Sept. 21, 2014 and attached at ESA’s Columbus module. It will measure ocean surface wind speed and direction and help improve weather forecasts, including hurricane monitoring. Credit: NASA/JPL-Caltech/Johnson Space Center. — ISS-RapidScat instrument, shown in this artist’s rendering, was launched to the International Space Station aboard the SpaceX CRS-4 mission on Sept. 21, 2014, and attached at ESA’s Columbus module. It will measure ocean surface wind speed and direction and help improve weather forecasts, including hurricane monitoring. Credit: NASA/JPL-Caltech/Johnson Space Center.

The successful installation and activation of the ISS-RapidScat science instrument on the exterior of Europe’s Columbus module in late September and early October inaugurated a new era in space station science.

RapidScat is designed to monitor ocean winds for climate research, weather predictions, and hurricane monitoring.

The 1280 pound (580 kilogram) experimental instrument is already collecting its first science data following its recent power-on and activation at the station.

SpaceX Falcon 9 erect at Cape Canaveral launch pad 40 awaiting launch on Sept 20, 2014 on the CRS-4 mission. Credit: Ken Kremer - kenkremer.com — SpaceX Falcon 9 with Dragon spaceship erect at Cape Canaveral launch pad 40 awaiting launch on Sept. 21, 2014, on the CRS-4 mission. Credit: Ken Kremer – kenkremer.com

“This mission enabled research critical to achieving NASA’s goal of long-duration human spaceflight in deep space,” said Sam Scimemi, director of the International Space Station division at NASA Headquarters.

“The delivery of the ISS RapidScatterometer advances our understanding of Earth science, and the 3-D printer will enable a critical technology demonstration. Investigations in the returned cargo could aid in the development of more efficient solar cells and semiconductor-based electronics, the development of plants better suited for space, and improvements in sustainable agriculture.”

The next SpacX cargo Dragon on the CRS-5 mission is slated for launch no earlier then Dec. 9.

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

Ken Kremer

…………….

Learn more about Commercial Space, Orion and NASA Human and Robotic Spaceflight at Ken’s upcoming presentations:

Oct 26/27: “Antares/Cygnus ISS Rocket Launch from Virginia”; Rodeway Inn, Chincoteague, VA

October 24, 2014December 23, 2015 by Tim Reyes

Making Cubesats do Astronomy

Will cubesats develop a new technological branch of astronomy? Goddard engineers are taking the necessary steps to make cubesat sized telescopes a reality. (Credit: NASA, UniverseToday/TRR)

One doesn’t take two cubesats and rub them together to make static electricity. Rather, you send them on a brief space voyage to low-earth orbit (LEO) and space them apart some distance and voilà, you have a telescope. That is the plan of NASA’s Goddard Space Flight Center engineers and also what has been imagined by several others.

Cubesats are one of the big crazes in the new space industry. But nearly all that have flown to-date are simple rudderless cubes taking photos when they are oriented correctly. The GSFC engineers are planning to give two cubes substantial control of their positions relative to each other and to the Universe surrounding them. With one holding a telescope and the other a disk to blot out the bright sun, their cubesat telescope will do what not even the Hubble Space Telescope is capable of and for far less money.

Semper (left), Calhoun, and Shah are advancing the technologies needed to create a virtual telescope that they plan to demonstrate on two CubeSats. (Image/Caption Credit: NASA/W. Hrybyk)

The 1U, the 3U, the 9U – these are all cubesats of different sizes. They all have in common the unit size of 1. A 1U cubesat is 10 x 10 x 10 centimeters cubed. A cube of this size will hold one liter of water (about one quart) which is one kilogram by weight. Or replace that water with hydrazine and you have very close to 1 kilogram of mono-propellent rocket fuel which can take a cubestat places.

GSFC aerospace engineers, led by Neerav Shah, don’t want to go far, they just want to look at things far away using two cubesats. Their design will use one as a telescope – some optics and a good detector –and the other cubesat will stand off about 20 meters, as they plan, and function as a coronagraph. The coronagraph cubesat will function as a sun mask, an occulting disk to block out the bright rays from the surface of the Sun so that the cubesat telescope can look with high resolution at the corona and the edge of the Sun. To these engineers, the challenge is keeping the two cubesats accurately aligned and pointing at their target.

Only dedicated Sun observing space telescopes such as SDO, STEREO and SOHO are capable of blocking out the Sun, but their coronagraphs are limited. Separating the coronagraph farther from the optics markedly improves how closely one can look at the edge of a bright object. With the corongraph mask closer to the optics, more bright light will still reach the optics and detectors and flood out what you really want to see. The technology Shah and his colleagues develop can be a pathfinder for future space telescopes that will search for distant planets around other stars – also using a coronagraph to reveal the otherwise hidden planets.

The engineers have received a $8.6-million investment from the Defense Advanced Research Project Agency (DARPA) and are working in collaboration with the Maryland-based Emergent Space Technologies.

An example of a 3U cubesat - 3 1U cubes stacked. This cubesat size could function as the telescope of a two cubesat telescope system. It could be a simple 10 cm diameter optic system or use fancier folding optics to improve its resolving power. (Credit: LLNL) — An example of a 3U cubesat – 3 1U cubes stacked. This cubesat size could function as the telescope of a two cubesat telescope system. It could be a simple 10 cm diameter optic system or use fancier folding optics to improve its resolving power. (Credit: LLNL)

The challenge of GSFC engineers is giving two small cubesats guidance, navigation, and control (GN&C) as good as any standard spacecraft that has flown. They plan on using off-the-shelf technology and there are many small and even large companies developing and selling cubesat parts.

This is a sorting out period for the cubesat sector, if you will, of the new space industry. Sorting through the off-the-shelf components, the GSFC engineers led by Shah will pick the best in class. The parts they need are things like tiny sun sensors and star sensors, laser beams and tiny detectors of those beams, accelerometers, tiny gyroscopes or momentum wheels and also small propulsion systems. The cubesat industry is pretty close to having all these ready as standard issue. The question then is what do you do with tiny satellites in low-Earth orbit (LEO). Telescopes for earth-observing are already making headway and scopes for astronomy are next. There are also plans to venture out to interplanetary space with tiny and capable cubesat space probes.

Whether one can sustain a profit for a company built on cubesats remains a big question. Right now those building cubesats to customer specs are making a profit and those making the tiny picks and shovels for cubesats are making profits. The little industry may be overbuilt which in economic parlance might be only natural. Many small startups will fail. However, for researchers at universities and research organizations like NASA, cubesats have staying power because they reduce cost by their low mass and size, and the low cost of the components to make them function. The GSFC effort will determine how quickly cubesats begin to do real work in the field of astronomy. Controlling attitude and adding propulsion is the next big thing in cubesat development.

References:

NASA Press Release

October 23, 2014December 23, 2015 by Tim Reyes

Unusual Distributions of Organics Found in Titan’s Atmosphere

The ALMA array, as it looks now completed and standing on a Chilean high plateau at 5000 meters (16,400 ft) altitude. The first observations with ALMA of Titan have added to the Saturn moon's list of mysteries. {Credit: ALMA (ESO/NAOJ/NRAO) / L. Calçada (ESO)}

A new mystery of Titan has been uncovered by astronomers using their latest asset in the high altitude desert of Chile. Using the now fully deployed Atacama Large Millimeter Array (ALMA) telescope in Chile, astronomers moved from observing comets to Titan. A single 3 minute observation revealed organic molecules that are askew in the atmosphere of Titan. The molecules in question should be smoothly distributed across the atmosphere, but they are not.

The Cassini/Huygens spacecraft at the Saturn system has been revealing the oddities of Titan to us, with its lakes and rain clouds of methane, and an atmosphere thicker than Earth’s. But the new observations by ALMA of Titan underscore how much more can be learned about Titan and also how incredible the ALMA array is.

ALMA first obserations of the atmospher of Saturn's moon Titan. The image shows the distribution of the organic molecule HNC. Red to White representing low to high concenrations. The offset locations of the molecules relative to the poles suprised the researchers lead by NASA/GSFC astrochemist M. Cordiner.(Credit: NRAO/AUI/NSF; M. Cordiner (NASA) et at.) — ALMA’s first observations of the atmosphere of Saturn’s moon Titan. The image shows the distribution of the organic molecule HNC. Red to White representing low to high concentrations. The offset locations of the molecules relative to the poles surprised the researchers led by NASA/GSFC astrochemist M. Cordiner. (Credit: NRAO/AUI/NSF; M. Cordiner (NASA) et at.)

The ALMA astronomers called it a “brief 3 minute snapshot of Titan.” They found zones of organic molecules offset from the Titan polar regions. The molecules observed were hydrogen isocyanide (HNC) and cyanoacetylene (HC3N). It is a complete surprise to the astrochemist Martin Cordiner from NASA Goddard Space Flight Center in Greenbelt, Maryland. Cordiner is the lead author of the work published in the latest release of Astrophysical Journal Letters.

The NASA Goddard press release states, “At the highest altitudes, the gas pockets appeared to be shifted away from the poles. These off-pole locations are unexpected because the fast-moving winds in Titan’s middle atmosphere move in an east–west direction, forming zones similar to Jupiter’s bands, though much less pronounced. Within each zone, the atmospheric gases should, for the most part, be thoroughly mixed.”

When one hears there is a strange, skewed combination of organic compounds somewhere, the first thing to come to mind is life. However, the astrochemists in this study are not concluding that they found a signature of life. There are, in fact, other explanations that involve simpler forces of nature. The Sun and Saturn’s magnetic field deliver light and energized particles to Titan’s atmosphere. This energy causes the formation of complex organics in the Titan atmosphere. But how these two molecules – HNC and HC3N – came to have a skewed distribution is, as the astrochemists said, “very intriguing.” Cordiner stated, “This is an unexpected and potentially groundbreaking discovery… a fascinating new problem.”

The press release from the National Radio Astronomy Observatory states, “studying this complex chemistry may provide insights into the properties of Earth’s very early atmosphere.” Additionally, the new observations add to understanding Titan – a second data point (after Earth) for understanding organics of exo-planets, which may number in the hundreds of billions beyond our solar system within our Milky Way galaxy. Astronomers need more data points in order to sift through the many exo-planets that will be observed and harbor organic compounds. With Titan and Earth, astronomers will have points of comparison to determine what is happening on distant exo-planets, whether it’s life or not.

High in the atmosphere of Titan, large patches of two trace gases glow near the north pole, on the dusk side of the moon, and near the south pole, on the dawn side. Brighter colors indicate stronger signals from the two gases, HNC (left) and HC3N (right); red hues indicate less pronounced signals. Image (Credit: NRAO/AUI/NSF) — High in the atmosphere of Titan, large patches of two trace gases glow near the north pole, on the dusk side of the moon, and near the south pole, on the dawn side. Brighter colors indicate stronger signals from the two gases, HNC (left) and HC3N (right); red hues indicate less pronounced signals.
(Image Credit: NRAO/AUI/NSF)

The report of this new and brief observation also underscores the new astronomical asset in the altitudes of Chile. ALMA represents the state of the art of millimeter and sub-millimeter astronomy. This field of astronomy holds a lot of promise. Back around 1980, at the Kitt Peak National Observatory in Arizona, alongside the great visible light telescopes, there was an oddity, a millimeter wavelength dish. That dish was the beginning of radio astronomy in the 1 – 10 millimeter wavelength range. Millimeter astronomy is only about 35 years old. These wavelengths stand at the edge of the far infrared and include many light emissions and absorptions from cold objects which often include molecules and particularly organics. The ALMA array has 10 times more resolving power than the Hubble space telescope.

The Earth’s atmosphere stands in the way of observing the Universe in these wavelengths. By no coincidence our eyes evolved to see in the visible light spectrum. It is a very narrow band, and it means that there is a great, wide world of light waves to explore with different detectors than just our eyes.

The diagram shows the electromagnetic spectrum, the absorption of light by the Earth's atmosphere and illustrates the astronomical assets that focus on specific wavelengths of light. ALMA at the Chilean site and with modern solid state electronics is able to overcome the limitations placed by the Earth's atmosphere. (Credit: Wikimedia, T.Reyes) — The diagram shows the electromagnetic spectrum, the absorption of light by the Earth’s atmosphere, and illustrates the astronomical assets that focus on specific wavelengths of light. ALMA at the Chilean site, with modern solid state electronics, is able to overcome the limitations placed by the Earth’s atmosphere. (Credit: Wikimedia, T.Reyes)

In the millimeter range of wavelengths, water, oxygen, and nitrogen are big absorbers. Some wavelengths in the millimeter range are completely absorbed. So there are windows in this range. ALMA is designed to look at those wavelengths that are accessible from the ground. The Chajnantor plateau in the Atacama desert at 5000 meters (16,400 ft) provides the driest, clearest location in the world for millimeter astronomy outside of the high altitude regions of the Antarctic.

At high altitude and over this particular desert, there is very little atmospheric water. ALMA consists of 66 12 meter (39 ft) and 7 meter (23 ft) dishes. However, it wasn’t just finding a good location that made ALMA. The 35 year history of millimeter-wavelength astronomy has been a catch up game. Detecting these wavelengths required very sensitive detectors – low noise in the electronics. The steady improvement in solid-state electronics from the late 70s to today and the development of cryostats to maintain low temperatures have made the new observations of Titan possible. These are observations that Cassini at 1000 kilometers from Titan could not do but ALMA at 1.25 billion kilometers (775 million miles) away could.

The 130 ton German Antenna Dish Transporter, nicknamed Otto. The ALMA transporter vehicle carefully carries the state-of-the-art antenna, with a diameter of 12 metres and a weight of about 100 tons, on the 28 km journey to the Array Operations Site, which is at an altitude of 5000 m. The antenna is designed to withstand the harsh conditions at the high site, where the extremely dry and rarefied air is ideal for ALMA’s observations of the universe at millimetre- and sub-millimetre-wavelengths. (Credit: ESO)

The ALMA telescope array was developed by a consortium of countries led by the United States’ National Science Foundation (NSF) and countries of the European Union though ESO (European Organisation for Astronomical Research in the Southern Hemisphere). The first concepts were proposed in 1999. Japan joined the consortium in 2001.

The prototype ALMA telescope was tested at the site of the VLA in New Mexico in 2003. That prototype now stands on Kitt Peak having replaced the original millimeter wavelength dish that started this branch of astronomy in the 1980s. The first dishes arrived in 2007 followed the next year by the huge transporters for moving each dish into place at such high altitude. The German-made transporter required a cabin with an oxygen supply so that the drivers could work in the rarefied air at 5000 meters. The transporter was featured on an episode of the program Monster Moves. By 2011, test observations were taking place, and by 2013 the first science program was undertaken. This year, the full array was in place and the second science program spawned the Titan observations. Many will follow. ALMA, which can operate 24 hours per day, will remain the most powerful instrument in its class for about 10 years when another array in Africa will come on line.

References:

NASA Goddard Press Release

NRAO Press Release

ALMA Observatory Website

“Alma Measurements Of The Hnc And Hc3N Distributions In Titan’s Atmosphere“, M. A. Cordiner, et al., Astrophysical Journal Letters

October 22, 2014December 23, 2015 by Ken Kremer

Assembly Complete for NASA’s Maiden Orion Spacecraft Launching in December 2014

Technicians complete final assembly of NASA’s first Orion spacecraft with installation of the close out panels on the Launch Abort System that smooth airflow. Credit: Photo credit: Kim Shiflett

Technicians at the Kennedy Space Center have completed the final major assembly work on NASA’s maiden Orion crew module slated to launch on its first unmanned orbital test flight this December, dubbed Exploration Flight Test-1 (EFT-1)

After first attaching the Launch Abort System (LAS) to the top of the capsule, engineers carefully installed a fairing composed of a set of four ogive panels over the crew module and the abort systems lower structural framework joining them together.

“The ogive panels smooth the airflow over the conical spacecraft to limit sound and vibration, which will make for a much smoother ride for the astronauts who will ride inside Orion in the future,” according to a NASA description.

Upon finishing the panel assembly work inside the Launch Abort System Facility (LASF) at NASA’s Kennedy Space Center, the teams cleared the last major hurdle before the Orion stack is rolled out to launch pad 37 in mid-November and hoisted to the top of the Delta IV Heavy rocket.

Technicians complete final assembly of NASA’s first Orion spacecraft with installation of the last ogive close out panels on the Launch Abort System that smooth airflow. Credit: Photo credit: Kim Shiflett — Technicians complete final assembly of NASA’s first Orion spacecraft with installation of the last ogive close out panels on the Launch Abort System that smooth airflow. Photo credit: Kim Shiflett

The Orion stack is comprised of the LAS, crew module (CM) and service module (SM).

The maiden blastoff of the state-of-the-art Orion spacecraft on the EFT-1 mission is slated for December 4, 2014, from Space Launch Complex 37 (SLC-37) at Cape Canaveral Air Force Station in Florida atop the triple barreled United Launch Alliance (ULA) Delta IV Heavy booster.

Orion is NASA’s next generation human rated vehicle that will eventually carry America’s astronauts beyond Earth on voyages venturing farther into deep space than ever before – beyond the Moon to Asteroids, Mars, and other destinations in our Solar System.

NASA’s completed Orion EFT 1 crew module loaded on wheeled transporter during move to the Payload Hazardous Servicing Facility (PHFS) on Sept. 11, 2014 at the Kennedy Space Center, FL. Credit: Ken Kremer - kenkremer.com — NASA’s completed Orion EFT 1 crew module loaded on wheeled transporter during move to the Payload Hazardous Servicing Facility (PHSF) on Sept. 11, 2014, at the Kennedy Space Center, FL. Credit: Ken Kremer – kenkremer.com

The two-orbit, four and a half hour EFT-1 flight around Earth will lift the Orion spacecraft and its attached second stage to an orbital altitude of 3,600 miles, about 15 times higher than the International Space Station (ISS) – and farther than any human spacecraft has journeyed in 40 years. It will test the avionics and electronic systems inside the Orion spacecraft.

Then the spacecraft will travel back through the atmosphere at speeds approaching 20,000 mph and temperatures near 4,000 degrees Fahrenheit to test the heat shield, before splashing down for a parachute assisted landing in the Pacific Ocean.

Launch Abort System (LAS) for Orion EFT-1 on view horizontally inside the Launch Abort System Facility at the Kennedy Space Center, Florida, prior to installation atop the crew module. Credit: Ken Kremer/kenkremer.com

The LAS plays a critically important role to ensure crew safety.

In case of an emergency situation, the LAS is designed to ignite within milliseconds to rapidly propel the astronauts inside the crew module away from the rocket and save the astronauts’ lives. The quartet of LAS abort motors would generate some 500,000 pounds of thrust to pull the capsule away from the rocket.

And don’t forget that you can fly your name on Orion and also print out an elegant looking “boarding pass.”

Details below and in my article – here.

NASA announced that the public can submit their names for inclusion on a dime-sized microchip that will travel on Orion and succeeding spacecraft voyaging to destinations beyond low-Earth orbit, including Mars.

The deadline to submit your name is soon: Oct 31, 2014.

Click on this weblink posted online by NASA today: http://go.usa.gov/vcpz

NASA invites you to send your name to Mars via the first Orion test flight in December 2014. Deadline for submissions is Oct 31, 2014. Join over 170,000 others! See link below. Credit: NASA

“NASA is pushing the boundaries of exploration and working hard to send people to Mars in the future,” said Mark Geyer, Orion Program manager, in a NASA statement.

“When we set foot on the Red Planet, we’ll be exploring for all of humanity. Flying these names will enable people to be part of our journey.”

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

Ken Kremer

The United Launch Alliance Delta-IV Heavy rocket tasked with launching NASA’s Orion EFT-1 mission being hoisted vertical atop Space Launch Complex-37B at Cape Canaveral Air Force Station in Florida on the morning of Oct. 1, 2014. Photo Credit: Alan Walters / AmericaSpace

…………….

Learn more about Orion, Space Taxis, and NASA Human and Robotic Spaceflight at Ken’s upcoming presentations:

Oct 26/27: “Antares/Cygnus ISS Rocket Launch from Virginia”; Rodeway Inn, Chincoteague, VA

October 22, 2014December 23, 2015 by Jason Major

No, This Is Not a Photo of India on Diwali

Yes, it's India, but it's not a photo captured from space during Diwali night. (Credit: NASA)

Diwali, the Indian festival of lights, falls on Thursday, Oct. 23 this year and with it come celebrations, gift-giving, and brilliant lighting and firework displays all across the subcontinent of India… but this isn’t a picture of that. What is it exactly? Find out below…

Over the past several years this image has repeatedly resurfaced online, especially around the time of Diwali. And understandably so: it’s a beautiful view of India seemingly decorated for the festival… one can easily imagine the entire country awash in colorful lights from shore to shore.

But it’s not a photo at all, or even a singular image. Rather it’s a composite of many images acquired from a USAF Defense Meteorological Satellite Program (DMSP) satellite over the course of several years, and assembled by NOAA scientist Chris Elvidge to show the country’s growing population and urban areas.

In a 2012 article by Robert Johnson on Business Insider a NASA spokesperson described the colors in the image: “The white lights were the only illumination visible before 1992. The blue lights appeared in 1992. The green lights in 1998. And the red lights appeared in 2003.”

So what does India look like at night during the five-day-long Diwali festival? Click here and see.

While city lighting in India is definitely visible from space, it’s not the rainbow explosion of neon colors that Internet hoaxers and uninformed online enthusiasts would eagerly have you believe. According to Adam Voiland on the NASA Earth Observatory site, “in reality, any extra light produced during Diwali is so subtle that it is likely imperceptible when observed from space.”

So this year, don’t fall for any false descriptions of this picture… and, Happy Diwali!

Sources: Business Insider, Mashable, NASA Earth Observatory, EarthSky. Read more about the 2014 celebration of Diwali here.

HT to Peter Caltner on Twitter for re-alerting me of this.

October 22, 2014December 23, 2015 by Ken Kremer

Stunning View of Solar System’s Largest Volcano and Valles Marineris Revealed by India’s Mars Orbiter Mission

Olympus Mons, Tharsis Bulge trio of volcanoes and Valles Marineris from ISRO's Mars Orbiter Mission. Note the clouds and south polar ice cap. Credit: ISRO

India’s Mars Orbiter Mission (MOM) has delivered another sweet treat – a stunning view of our Solar System’s largest volcano and the largest canyon.

Just days ago, MOM captured a new global image of the Red Planet dominated by Olympus Mons and Valles Marineris – which is the largest known volcano and the largest known canyon in the Solar System, respectively.

Situated right in between lies a vast volcanic plateau holding a trio of huge volcanoes comprising the Tharsis Bulge: Arsia Mons, Pavonis Mons, and Ascraeus Mons. All four volcanoes are shield volcanoes.

To give an idea of its enormity, Olympus Mons stands about three times taller than Mount Everest and is about the size of Arizona.

Olympus Mons from Mars orbit compared to the state of Arizona. Credit: NASA

Olympus Mons is located in Mars’ western hemisphere and measures 624 kilometers (374 miles) in diameter, 25 km (16 mi) high, and is rimmed by a 6 km (4 mi) high scarp.

Valles Marineris is often called the “Grand Canyon of Mars.” It spans about as wide as the entire United States.

The Indian Space Research Organization (ISRO), India’s space agency which designed and developed the orbiter released the image on Oct. 17, barely two days ahead of the planet’s and spacecrafts’ extremely close encounter with comet Siding Spring.

By the way, a relieved ISRO tweeted MOM’s survival of her close shave with the once-in-a-lifetime cometary passage with gusto, soon after the swingby:

“Phew! Experience of a lifetime. Watched the #MarsComet #SidingSpring whizzing past the planet. I’m in my orbit, safe and sound.”

The new global image was taken by the tri-color camera as MOM swooped around the Red Planet in a highly elliptical orbit whose nearest point to Mars (periapsis) is at 421.7 km and farthest point (apoapsis) at 76,993.6 km, according to ISRO.

To date ISRO has released four global images of the Red Planet, including a 3-D view, reported here.

Olympus Mons, the Tharsis Bulge, and Valles Marineris are near the equator.

Valles Marineris stretches over 4,000 km (2,500 mi) across the Red Planet, is as much as 600 km wide, and measures as much as 7 kilometers (4 mi) deep.

Here’s a comparison view of the region taken by NASA’s Viking 1 orbiter in the 1970s.

Global Mosaic of Mars Centered on Valles Marineris from NASA’s Viking 1 orbiter. Credit: NASA

MOM is India’s first deep space voyager to explore beyond the confines of her home planet’s influence and successfully arrived at the Red Planet only one month ago after the “history creating” orbital insertion maneuver on Sept. 23/24 following a ten month journey.

The $73 million MOM mission is expected to last at least six months.

MOM’s success follows closely on the heels of NASA’s MAVEN orbiter which also successfully achieved orbit barely two days earlier on Sept. 21 and could last 10 years or more.

With MOM’s arrival, India became the newest member of an elite club of only four entities that have launched probes that successfully investigated Mars – following the Soviet Union, the United States, and the European Space Agency (ESA).

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

Ken Kremer

ISRO's Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74500 km on Sept. 28, 2014. Credit: ISRO — ISRO’s Mars Orbiter Mission captures spectacular portrait of the Red Planet and swirling dust storms with the on-board Mars Color Camera from an altitude of 74,500 km on Sept. 28, 2014. Credit: ISRO

October 21, 2014January 15, 2019 by Matt Williams

How NASA and SpaceX are Working Together to Land on Mars

Thermal imagery of Falcon 9 rocket. Image Credit: NASA/Scifli Team/Applied Physics Laboratory Images

It is no secret that NASA is seeking out private space contractors to help bring some of its current plans to fruition. Naturally, these involve restoring indigenous launch capabilities to the US, but also include the more far-reaching goal of sending astronauts to Mars. Towards that end, NASA and SpaceX participated in an unprecedented data-sharing project that will benefit them both.

Continue reading “How NASA and SpaceX are Working Together to Land on Mars”

October 20, 2014December 15, 2018 by Matt Williams

Water On The Moon Was Blown in by Solar Wind

Near-infrared image of the Moon's surface by NASA's Moon Mineralogy Mapper on the Indian Space Research Organization's Chandrayaan-1 mission Image credit: ISRO/NASA/JPL-Caltech/Brown Univ./USGS

When they first set foot on the Moon, the Apollo 11 astronauts painted a picture of the landscape as a bone-dry desert. So astronomers were naturally surprised when in 2009, three probes showed that a lot of water is locked up in minerals in the soil. There has been some debate as to where the water came from, but now two researchers with the National Museum of Natural History in Paris, France, have determined that most of the water in the soil on the surface of the Moon was formed due to protons in the solar wind colliding with oxygen in lunar dust, rather than from comet or meteorite impacts.

The first hints that there was water on the Moon came when India’s Chandrayaan-1 found hints of water across the lunar surface when it measured a dip in reflected sunlight at a wavelength absorbed only by water and hydroxyl, a molecule that contains one atom of hydrogen and one atom of oxygen.

Continue reading “Water On The Moon Was Blown in by Solar Wind”