Universe Today

April 9, 2013December 23, 2015 by Elizabeth Howell

How To Crowdsource Astronomy Without People Messing It Up

A family portrait of the PH1 planetary system that was discovered in part due to crowdsourcing. Image Credit: Haven Giguere/Yale.

Maybe it’s because Jurassic Park is in theaters again, but we at Universe Today sometimes worry about how one person can mess up an otherwise technologically amazing system. It took just one nefarious employee to shut down the dinosaur park’s security fences in the movie and cause havoc. How do we ensure science can fight against that, especially when everyday citizens are getting more and more involved in the scientific process?

But perhaps, after talking to Chris Lintott, that view is too suspicious. Lintott is in charge of a collaborative astronomy and science project called the Zooniverse that uses public contributions to fuel some of the science he performs. Basically, anyone with an Internet connection and a desire to contribute can hunt for planets or examine astronomical objects, among many other projects.

Lintott, an astrophysicist at the University of Oxford, says the science requires public contributions. Moreover, he hasn’t had a problem yet despite 800,000 individual contributors to the Zooniverse. He told Universe Today about how that’s possible in an e-mail interview.

1) Zooniverse has already produced tangible scientific results in space through collaborating with ordinary folks. Can you talk about some of the papers/findings that have been produced in your various projects?

There’s a long, long list. I’m particularly excited at the minute about our work on bulgeless galaxies; most spiral galaxies have a bulge full of old stars at their centre, but we’ve found plenty that don’t. That’s exciting because we think that means that they’re guaranteed not to have had a big merger in the last 10 billion years or so, and that means we can use them to figure out just what effect mergers have on galaxies. You’ll be hearing more about them in the next year or so as we have plenty of observing time lined up.

I’m also a big fan of Planet Hunters 1b, our first confirmed planet discovery – it’s a planet in a four-star system, and thus provides a nice challenge to our understanding of how planets form. We’ve found lots of planet candidates (systems where we’re more than 90% sure there’s a planet there) but it’s nice to get one confirmed and especially nice for it to be such an interesting world.

One of Zooniverse's projects examines the nature of spiral galaxies, particularly those without central bulges at the center. Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University) — One of Zooniverse’s projects examines the nature of spiral galaxies, particularly those without central bulges at the center. Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)

2) What benefits have you received from involving the public in space projects, in terms of results as well as raising awareness?

We couldn’t do our research any other way. Astronomers have got very good in the last few decades at collecting information about the universe, but we’re not always so good at learning how to use all of that information. The Zooniverse allows us to collaborate with hundreds of thousands of people so that we can scale our efforts to deal with that flood of data, and many of those volunteers go much further than just clicking on buttons we provide. So really our research is now driven in collaboration with thousands of people, spread all around the world – that’s an inspiring thought.

3) How many people do you manage in your space projects, approximately? How do you keep track of them all?

We have more than 800,000 registered volunteers – luckily, the computer keeps track of them (when they log in!).

4) How do you ensure their results meet the standards of scientific publication?

We carefully design projects so that we’re sure they will produce scientifically useful results before they’re launched; this usually means running a test with a small amount of data and comparing work done by volunteers with that of professionals. We usually find the volunteers are better than us! It helps that we have several people complete each task, so collectively we don’t make accidental mistakes.

5) How do you guard against somebody deliberately or accidentally altering the results?

The system insists that every classification is independent, and as we have several people look at each classification finding any deliberate attack would be easy – in any case, we’ve never seen any evidence of such a thing. Despite popular reports, most people are nice!

April 9, 2013December 23, 2015 by Nancy Atkinson

Celebrate Earth Month with 2 New Videos from NASA

Nighttime photo of the Nile delta region taken from the ISS (NASA)

Enjoy some great views of our home planet from images taken from the orbiting Earth-observing satellites and taken by astronauts on the International Space Station. The satellites and scientists are cranking out data 24/7 to help us all better understand and sustain our home planet.

Above is a video created for Earth Month, and specifically Earth Day (April 22) from ISS imagery, and below is another video from satellite imagery. These are unique looks at the beauty and wonder of our home planet.

April 8, 2013December 23, 2015 by Nancy Atkinson

Two New Online Astronomy Courses from CosmoQuest

Want to learn more about our Universe or refresh your astronomical knowledge? Cosmoquest has two new online astronomy classes, and they are a great opportunity expand your horizons! The two classes are “The Sun and Stellar Evolution” (April 15 – May 8, 2013) and “Introduction to Cosmology” (April 23 – May 16, 2013) Cosmoquest offers the convenience of an online class along with live (and lively!) interaction with your instructor and a small group astronomy enthusiasts like yourself. The lectures are held in Google+ Hangouts, with course assignments and homework assigned via Moodle.

The instructors are likely well-known to UT readers. Research assistant and blogger Ray Sanders (Dear Astronomer and UT) will be teaching the stellar evolution class and astronomer and writer Dr. Matthew Francis will be leading the cosmology course.

The cost for the class is $240, and the class is limited to 8 participants, with the possibility for an additional 5 participants. Both instructors say no prior knowledge of cosmology or astronomy is needed. There will be a little math, but it will be on the high school algebra level. Concepts will be heavily emphasized.

Here are the descriptions for each class:

Stellar Evolution:

The Sun is a fascinating topic of study, which allows solar astronomers to better understand the physical processes in other stars. During this 4-week / 8-session course, we’ll explore the Sun and Solar Evolution from an astronomer’s point of view. Our course
will begin with an overview of the Sun, and solar phenomenon. We’ll also explore how stars are formed, their lifecycles, and the
incredible events that occur when stars reach the end of their lives. The course will culminate with students doing a short presentation on a topic related to the Sun or Stellar Evolution.

Introduction to Cosmology:

Cosmology is the study of the structure, contents, and evolution of the Universe as a whole. But what do cosmologists really study? In this 8-session course, we’ll look at cosmology from an astronomy point of view: taking what seems like too big of a subject and showing how we can indeed study the Universe scientifically. The starting point is the smallest chunk of the Universe that is representative of everything we can see: the Cosmic Box.

Class level: No prior knowledge of cosmology or astronomy is needed. There will be a little math, but it will be on the high school algebra level: the manipulation of ratios and use of some important equations. The emphasis is on concepts!

More information and signup instructions can be found here at Cosmoquest.

April 8, 2013December 23, 2015 by Nancy Atkinson

A Detailed Look at the Coma of Comet PANSTARRS

Image and variations of Comet C/2011 L4 (PANSTARRS) taken on 2013, April 7, 2013 remotely from New Mexico. Credit: Ernesto Guido, Nick Howes, and Martino Nicolini.

Comet PANSTARRS has peaked, but astronomers are still keeping an eye on this comet to try and determine what its future might hold. The team from the Remanzacco Observatory has just produced some really interesting views of Comet PANSTARRS, with a little help from Martino Nicolini and his Astroart software.

Team member Nick Howes called this software “one of the best astronomical image processing and acquisition tools around,” and explained how these views can tell astronomers more about what is happening with the comet.

“The isophotes image (color coded) is a good way to see the morphology/structure of the coma,” he told Universe Today, adding that comparing the images here is “a very good way to determine any major events like a fragmentation. We’re hopeful that once PANSTARRS gets a bit higher, we’ll be able to look at it in even more detail with the 2 meter Faulkes scopes.”

And with the image processing in the image on the far right, it’s possible to see a bright shell in the coma of comet C/2011 L4 (PANSTARRS).

“The last elaboration in that image has been obtained using the M.C.M. (Median Coma Model), a filter that has the purpose of creating — from an image of a comet — a synthetic model of the ‘regular’ coma,” said Ernesto Guido, from the Remanzacco team. “That is obtained by mapping all the pixels that compose the image and averaging them together. In doing so we delete all the morphological “non-uniformity” contained in the coma itself. This regular coma will then be subtracted from the original image highlighting all the details that are normally immersed in the uniform brightness of the coma.”

Check out the Remanzacco website for more information and their continued updates.

April 8, 2013December 23, 2015 by Jason Major

More Evidence That Mars Lost Its Atmosphere

Mosaic self-portrait of Curiosity at the John Klein outcrop on Feb. 3, 2013 (NASA/JPL-Caltech/MSSS)

Although today Mars’ atmosphere is sparse and thin — barely 1% the density of Earth’s at sea level — scientists don’t believe that was always the case. The Red Planet likely had a much denser atmosphere similar to ours, long, long ago. So… what happened to it?

NASA’s Curiosity rover has now found strong evidence that Mars lost much of its atmosphere to space — just as many scientists have suspected. The findings were announced today at the EGU 2013 General Assembly in Vienna.

Curiosity's SAM instrument (NASA/JPL-Caltech) — Curiosity’s SAM instrument (NASA/JPL-Caltech)

Curiosity’s microwave oven-sized Sample Analysis at Mars (SAM) instrument analyzed an atmosphere sample last week using a process that concentrates selected gases. The results provided the most precise measurements ever made of isotopes of argon in the Martian atmosphere.

Isotopes are variants of the same element with different atomic weights.

“We found arguably the clearest and most robust signature of atmospheric loss on Mars,” said Sushil Atreya, a SAM co-investigator at the University of Michigan.

SAM found that the Martian atmosphere has about four times as much of a lighter stable isotope (argon-36) compared to a heavier one (argon-38). This ratio is much lower than the Solar System’s original ratio, as estimated from measurements of the Sun and Jupiter.

The argon isotope fractionation provides clear evidence of the loss of atmosphere from Mars. (NASA/JPL)

This also removes previous uncertainty about the ratio in the Martian atmosphere in measurements from NASA’s Viking project in 1976, as well as from small volumes of argon extracted from Martian meteorites retrieved here on Earth.

These findings point to a process that favored loss of the lighter isotope over the heavier one, likely through gas escaping from the top of the atmosphere. This appears to be in line with a previously-suggested process called sputtering, by which atoms are knocked out of the upper atmosphere by energetic particles in the solar wind.

The solar wind may have helped strip Mars of its atmosphere over the course of many hundreds of millions of years (NASA)

Lacking a strong magnetic field, Mars’ atmosphere would have been extremely susceptible to atmospheric erosion by sputtering billions of years ago, when the solar wind was an estimated 300 times the density it is today.

These findings by Curiosity and SAM will undoubtedly support those made by NASA’s upcoming MAVEN mission, which will determine how much of the Martian atmosphere has been lost over time by measuring the current rate of escape to space. Scheduled to launch in November, MAVEN will be the first mission devoted to understanding Mars’ upper atmosphere.

Find out more about MAVEN and how Mars may have lost its atmosphere in the video below, and follow the most recent discoveries of the MSL mission here.

Source: NASA/JPL

April 8, 2013December 23, 2015 by Elizabeth Howell

Want to be an Astronaut? Learn How to Speak Russian

Canadian astronaut David Saint-Jacques prepares to simulate a spacewalk in NASA's Neutral Buoyancy Laboratory. Credit: NASA

A fire breaks out on the International Space Station while the orbiting complex is over Russian mission control. How, as an English-speaking astronaut, would you keep up with instructions?

The answer is years of Russian training. In between time in simulators, jet airplanes and underwater, neophyte astronauts spend hours learning to read Cyrillic characters and pronounce consonant-heavy words. In fact, one of NASA’s requirements for its astronauts now is to learn the Russian language.

“It’s taken very seriously in the program because of the level you need to reach if, God forbid, there was an emergency on board and there was a panicky discussion going on in Russian on the radio,” Canadian astronaut and medical doctor David Saint-Jacques told Universe Today. “Ultimately, you need to be fluent to be really useful in a situation like that.”

Saint-Jacques himself is no neophyte to language learning. A native francophone, he learned English in public school and really improved it when he was 15 and moved with his family to England for a year. Today he speaks it fluently. He also has some abilities in Japanese, a language he picked up while in that country for a junior academic position at a university.

David Saint-Jacques (left) with fellow Canadian astronaut trainee Jeremy Hansen. The two men were selected as astronauts in 2009. Credit: NASA

Now approaching four years as an astronaut trainee, Saint-Jacques told us how astronauts learn Russian. It’s a process that not only includes classroom instruction, but time living with a family in Moscow to really pick up on colloquialisms. Below is an edited interview.

What language training focuses on: “The point is not to write perfectly. The point is to communicate, similar to how businessmen learn languages. The emphasis for us is understanding spoken language, but the emphasis for us, the vocabulary, is different. I know all these obscure space hardware words and these crazy Russian space acronyms, but I may not know some of the flowers, for example. I can’t know everything.”

Basic Russian training: “We have Russian classes one-on-one with a Russian instructor. We get anything between one lesson every two weeks to three, four lessons a week, depending on how you accommodate the training schedule. Most astronauts want as much training as possible. It’s part of the requirements for basic training; you have to pass a certain competency test in Russian. There is a standard test that is used by the foreign affairs department, and so we do the same test. It’s a verbal test where you call the examiner on the phone and you have a discussion with them on the phone. If you pass a certain grade on that test, you are good to go.”

NEEMO 15 crew members from right to left: Shannon Walker (NASA), Steve Squyres (Cornell University), David Saint-Jacques (Canadian Space Agency), Takuya Onishi (Japanese Space Agency). Credit: NASA

Living in Russia: “You have to go to Russia at some point to learn the Soyuz spacecraft and the Russian segment of space station. That, of course, is in all in Russian. The training is in Russian and the books are in Russian. There are translators that could be there with you, but you don’t want to rely on an interpreter for class. It really hits home; the more you know, the better. You will be living there for months, and it’s a no-brainer: you have to speak Russian when you are going to Russia.”

Immersion: “I took some holidays there [in Russia] with my family. That’s one of the great things when you speak the language of the country; you have fun there. I try to hang out with any Russian cosmonaut that comes here to Houston to keep up with them. There are two other ways we can train: you can block two to three weeks to do an intensive Russian test where all you want to do [beforehand] is study Russian. Also, when you are assigned to a spaceflight, in the year before your spaceflight, they [NASA] will try to send you for a month and a half in Moscow in a family for total immersion. That makes most people bump up their Russian level quite a lot.”

Side benefits: “It makes you realize how at the end of the day, international relations is really a form of personal relations, and speaking a language is absolutely fundamental. It makes you graduate from having a professional experience to a life experience with the other person, the other country.”

April 8, 2013December 23, 2015 by Jason Major

Cassini Says “Senkyo Very Much”

Narrow-angle camera image of Titan from Cassini (NASA/JPL-Caltech/Space Science Institute)

In this image acquired on January 5, Cassini’s near-infrared vision pierced Titan’s opaque clouds to get a glimpse of the dark dune fields across a region called Senkyo.

The vast sea of dunes is composed of solid hydrocarbon particles that have precipitated out of Titan’s atmosphere. Also visible over Titan’s southern pole are the rising clouds of the recently-formed polar vortex.

For a closer look at Titan’s dunes (and to find out what the name Senkyo means) keep reading…

In the image above north on Titan is up and rotated 18 degrees to the right. It was taken using a spectral filter sensitive to wavelengths of near-infrared light centered at 938 nanometers.

The view was obtained at a distance of approximately 750,000 miles (1.2 million kilometers) from Titan.

Titan’s hydrocarbon dunes are found across the moon in a wide swath within 30 degrees of the equator and are each about a kilometer wide and tens to hundreds of kilometers long… and in some cases stand over 100 meters tall. (Source: Astronomy Now.)

Titan dunes Jan 2007 — Radar image of Titan’s dunes acquired on Jan. 13, 2007. This view is 160 kilometers (100 miles) high by 150 kilometers (90 miles) wide. (NASA/JPL)

Observations of the dunes with Cassini and ESA’s Huygens probe during its descent onto Titan’s surface have shown that the moon experiences seasonally-shifting equatorial winds during equinoxes, similar to what occurs over the Indian Ocean between monsoon seasons.

The name Senkyo refers to the Japanese realm of serenity and freedom from wordly cares and death… in line with the IAU convention of naming albedo features on Titan after mythological enchanted places.

Click here for an earlier view of Senkyo, and follow the Cassini mission here.

Color-composite of Titan made from raw Cassini images acquired on April 13, 2013 (added 4/17) NASA/JPL/SSI. Composite by J. Major.

April 8, 2013December 29, 2015 by Carnival of Space

Carnival of Space #296

This week’s Carnival of Space is hosted by Brian Wang at the Next Big Future blog.

Click here to read Carnival of Space #296.

And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, sign up to be a host. Send an email to the above address.

April 8, 2013December 23, 2015 by David Dickinson

The Return of Saturn: A Guide to the 2013 Opposition

A fine recent view of Saturn as captured by Daniel Robb. (Credit & Copyright: Daniel Robb/Universe Today flickr community. All rights reserved).

A star party favorite is about to return to evening skies.

The planet Saturn can now be spied low to the southeast for northern hemisphere observers (to the northeast for folks in the southern) rising about 1-2 hours after local sunset this early April. That gap will continue to close until Saturn is opposite to the Sun in the sky later this month and rises as the Sun sets.

Opposition occurs on April 28^th at 8:00 UT/4:00AM EDT. Saturn will shine at magnitude +0.1 and appear 18.8” in diameter excluding the rings, which give it a total angular diameter of 43”.

Saturn has just passed into the faint constellation Libra for 2013, although its springtime retrograde loop will bring it back into Virgo briefly. Both the 2013 and 2014 opposition will occur in Libra. Saturn will also pass 26’ from +4.2 Kappa Virginis on July 3^rd as it moves back into Virgo while in retrograde before resuming direct motion back into Libra.

Saturn currently lies about 15° to the lower left of the +1.04 magnitude star Spica, also known as Alpha Virginis. Remember the handy saying to “Spike to Spica” from the handle of the Big Dipper asterism to locate the region. Another handy finder tip; stars twinkle, planet generally don’t. That is, unless your skies are extremely turbulent!

With an orbital period 29.46 years, Saturn moves slowly eastward year to year, taking 2-3 years to cross through each constellation along the ecliptic.

Oppositions are roughly 378 days apart and thus move forward on our calendar by about two weeks a year. Successive oppositions also move about 13° eastward per year.

Saturn as imaged by the author on June 11th, 2012.

Oppositions of the ringed planet are also currently becoming successively favorable for southern observers over the coming years. Saturn crossed into the southern celestial hemisphere some years back, and will be at its southernmost in 2018.

Saturn won’t pass north of the celestial equator again until early 2026. Saturn is 15 million kilometres farther from us than opposition last year as its moving toward aphelion in 2018.

Saturn will reach eastern quadrature this summer on July 28^th and stand its highest south at sunset northern hemisphere observers. South of the equator, it will pass directly overhead or transit to the north. Saturn will be with us for most of the remainder of 2013 in evening skies until reaching solar conjunction on November 6^th.

Looking at Saturn with binoculars, you’ll immediately note that something is amiss.

You’re getting a view similar to that of Galileo, who sketched Saturn as a sort of “double handled cup.” In fact, it wasn’t until 1655 that Christian Huygens correctly hypothesized that the rings of Saturn are a flat disk that is not physically in contact with the planet.

Huygens also discovered the large moon Titan. Shining at magnitude +8.5 and taking 16 days to orbit Saturn, Titan is the second largest moon in our solar system after Ganymede. Titan would easily be a planet in its own right if it orbited the Sun. Titan is easily picked out observing Saturn at low power through a telescope.

Saturn's system of moons visible through a small telescope. orientation is for May 9th, 2013. (Created by the author using Starry Night). — Saturn’s system of moons visible through a small telescope. orientation is for May 9th, 2013. (Created by the author using Starry Night).

Observing Saturn at slightly higher magnification, five moons interior to Titan become apparent. From outside in, they are Rhea, Dione, Tethys, Enceladus, and Mimas. Exterior to Titan is the curious moon of Iapetus. Taking 79 days to complete one orbit of Saturn, Iapetus varies in brightness from magnitude +11.9 to +10.2, or a factor of over 5 times. Arthur C. Clarke placed the final monolith in the book adaptation of 2001: A Space Odyssey on Iapetus for this reason. Close-ups from the Cassini spacecraft reveal a two-faced world covered with a dark leading hemisphere and a bright trailing side, but alas, no alien artifacts.

But the centerpiece of observing Saturn through a telescope is its brilliant and complex system of rings. The A, B, and C rings are easily apparent through a backyard telescope, as is the large spacing known as the Cassini Gap.

The rings are also currently tilted in respect to our Earthly vantage point. The rings were edge-on in 2009 and vanish when this occurs every 15-16 years.

This year, we see the rings of Saturn at a respectable 19 ° opening and widening. The rings will appear at their widest at over 25° in 2017 and then become edge-on again in 2025.

The average tilt of Saturn's ring system as seen from Earth spanning 2008-2026. (Graph created by author). — The average tilt (in degrees) of Saturn’s ring system as seen from Earth spanning 2008-2026. (Graph created by author).

The ring system of Saturn adds 0.7 magnitudes of overall brightness to the planet at opposition this year.

Another interesting optical phenomenon to watch for in the days leading up to opposition is known as the “opposition surge” in brightness, or the Seeliger effect. This is a retro-reflector effect familiar to many as high-beam headlights strike a highway sign. Think of the millions of particles making up Saturn’s rings as tiny little “retro-reflectors” focusing sunlight back directly along our line of sight. The opposition surge has been noted for other planets, but it’s most striking for Saturn when its rings are at their widest.

The disk of Saturn will cast a shadow straight back onto the rings around opposition and thus vanish from our view. The shadow across the back of the rings will then become more prominent over subsequent months, reaching its maximum angle at quadrature this northern hemisphere summer and then beginning to slowly slide back behind the planet again. A true challenge is to glimpse the disk of the through the Cassini gap in the rings… you’ll need clear steady skies and high magnification for this one!

It’s also interesting to note a very shallow partial lunar eclipse occurs with Saturn nearby just three days prior to opposition on April 25^th. Saturn will appear 4° north of the Moon and it may be just possible to image both in the same frame.

The location of Saturn and the Full Moon during the April 25th partial eclipse. (Created by the author using Starry Night).

Saturn takes about 30 years to make its way around the zodiac. I remember just beginning to observe Saturn will my new 60mm Jason refractor as a teenager in 1983 as it crossed the constellation Virgo.Hey, I’ve been into astronomy for over one “Saturnian year” now… where will the next 30 years find us?

April 7, 2013June 5, 2022 by Ken Kremer

Antares Rocket Erected at Virginia Pad for Inaugural April 17 Launch – Photo Gallery

1st fully integrated Antares rocket stands firmly erect at seaside Launch Pad 0-A at NASA’s Wallops Flight Facility during exclusive launch complex tour by Universe Today. Maiden Antares test launch is scheduled for 17 April 2013. Later operational flights are critical to resupply the ISS. Credit: Ken Kremer (kenkremer.com) See Antares rollout and erection photo gallery below

1st fully integrated Antares rocket – decaled with huge American flag – stands firmly erect at seaside Launch Pad 0-A at NASA’s Wallops Flight Facility on 6 April 2013 following night time rollout. Maiden Antares test launch is scheduled for 17 April 2013. Later operational flights are critical to resupply the ISS. Credit: Ken Kremer (kenkremer.com).
See Antares rollout and erection photo gallery below[/caption]

For the first time ever, the new and fully integrated commercial Antares rocket built by Orbital Sciences was rolled out to its oceanside launch pad on a rather chilly Saturday morning (April 6) and erected at the very edge of the Eastern Virginia shoreline in anticipation of its maiden launch slated for April 17.

The inaugural liftoff of the privately developed two stage rocket is set for 5 p.m. from the newly constructed launch pad 0-A at the Mid-Atlantic Regional Spaceport (MARS) at NASA’s Wallops Flight Facility in Virginia.

And Universe Today was there! See my photo gallery herein.

Antares is the most powerful rocket ever to ascend near major American East Coast population centers, unlike anything before. The launch is open to the public and is generating buzz.

And this is one very cool looking rocket.

Antares rocket begins 1st ever rollout from processing hanger to NASA Wallops launch pad - beneath the Moon on 6 April 2013. Credit: Ken Kremer (kenkremer.com) — Antares rocket begins 1st ever rollout from processing hanger to NASA Wallops launch pad – beneath the Moon on 6 April 2013. Credit: Ken Kremer (kenkremer.com)

The maiden April 17 launch is actually a test flight dubbed the A-One Test Launch Mission.

The goal of the A-One mission is to validate that Antares is ready to launch Orbital‘s Cygnus capsule on a crucial docking demonstration and resupply mission to the International Space Station (ISS) as soon as this summer.

The 1 mile horizontal rollout trek of the gleaming white rocket from the NASA integration hanger to the pad on a specially designed trailer began in the dead of a frosty, windy night at 4:30 a.m. – and beneath a picturesque moon.

“We are all very happy and proud to get Antares to the pad today for the test flight,” Orbital ground operations manager Mike Brainard told Universe Today in an interview at Launch Complex 0-A.

The rocket was beautifully decaled with a huge American flag as well as the Antares, Cygnus and Orbital logos.

Raising Antares at NASA Wallops. Credit: Ken Kremer (kenkremer.com)

Antares was transported aboard the Transporter/Erector/Launcher (TEL), a multifunctional, specialized vehicle that also slowly raised the rocket to a vertical position on the launch pad a few hours later, starting at about 1 p.m. under clear blue skies.

This first ever Antares erection took about 30 minutes. The lift was postponed for several hours after arriving at the pad as Orbital personal monitored the continually gusting winds approaching the 29 knot limit and checked all pad and rocket systems to insure safety.

The TEL vehicle also serves as a support interface between the 133-foot Antares and the range of launch complex systems.

Antares transported atop aboard the Transporter/Erector/Launcher (TEL) beneath the Moon on 6 April 2013. Credit: Ken Kremer (kenkremer.com

Now that Antares stands vertical, “We are on a clear path to a launch date of April 17, provided there are no significant weather disruptions or major vehicle check-out delays between now and then,” said Mr. Michael Pinkston, Orbitals Antares Program Manager.

Antares is a medium class rocket similar to the Delta II and SpaceX Falcon 9.

For this test flight Antares will boost a simulated version of the Cygnus carrier – known as a mass simulator – into a target orbit of 250 x 300 kilometers and inclined 51.6 degrees.

Antares rolls up the ramp to Launch Complex 0-A at NASA’s Wallops Flight Facility on 6 April 2013. Credit: Ken Kremer (kenkremer.com)

The Antares first stage is powered by dual liquid fueled AJ26 first stage rocket engines that generate a combined total thrust of some 680,000 lbs. The upper stage features a Castor 30 solid rocket motor with thrust vectoring. Antares can loft payloads weighing over 5000 kg to LEO.

The Antares/Cygnus system was developed by Orbital Sciences Corp under NASA’s Commercial Orbital Transportation Services (COTS) program to replace the ISS cargo resupply capability previously tasked to NASA’s now retired Space Shuttle fleet.

Up Close with Antares beautifully decaled nose NASA Wallops Pad 0-A. Credit: Ken Kremer (kenkremer.com) — Up Close with Antares beautifully decaled nose at NASA Wallops Pad 0-A. Credit: Ken Kremer (kenkremer.com)

Orbital’s Antares/Cygnus system is similar in scope to the SpaceX Falcon 9/Dragon system. Both firms won lucrative NASA contracts to deliver approximately 20,000 kilograms of supplies and equipment to the ISS.

The goal of NASA’s COTS initiative is to achieve safe, reliable and cost-effective transportation to and from the ISS and low-Earth orbit (LEO).

Orbital will launch at least eight Antares/Cygnus resupply missions to the ISS at a cost of $1.9 Billion

The maiden Antares launch has been postponed by about 2 years due to delays in laiunch pad construction and validating the rocket and engines for flight- similar in length to the start up delays experienced by SpaceX for Falcon 9 and Dragon.

Read my prior Antares story detailing my tour of the launch complex following the successful 29 sec hot-fire engine test that cleared the path for the April 17 liftoff – here & here.

Watch for my continuing reports through liftoff of the Antares A-One Test flight.

Ken Kremer

…………….

Learn more about Antares, SpaceX, Curiosity and NASA missions at Ken’s upcoming lecture presentations:

April 20/21 : “Curiosity and the Search for Life on Mars – (in 3-D)”. Plus Orion, SpaceX, Antares, the Space Shuttle and more! NEAF Astronomy Forum, Suffern, NY

April 28: “Curiosity and the Search for Life on Mars – (in 3-D)”. Plus the Space Shuttle, SpaceX, Antares, Orion and more. Washington Crossing State Park, Titusville, NJ, 130 PM