Moon Archives

April 5, 2013December 23, 2015 by Jason Major

Hydrogen Peroxide Could Feed Life on Europa

Reprocessed Galileo image of Europa's frozen surface by Ted Stryk (NASA/JPL/Ted Stryk)

According to research by NASA astronomers using the next-generation optics of the 10-meter Keck II telescope, Jupiter’s ice-encrusted moon Europa has hydrogen peroxide across much of the surface of its leading hemisphere, a compound that could potentially provide energy for life if it has found its way into the moon’s subsurface ocean.

“Europa has the liquid water and elements, and we think that compounds like peroxide might be an important part of the energy requirement,” said JPL scientist Kevin Hand, the paper’s lead author. “The availability of oxidants like peroxide on Earth was a critical part of the rise of complex, multicellular life.”

The paper, co-authored by Mike Brown of the California Institute of Technology in Pasadena, analyzed data in the near-infrared range of light from Europa using the Keck II Telescope on Mauna Kea, Hawaii, over four nights in September 2011. The highest concentration of peroxide found was on the side of Europa that always leads in its orbit around Jupiter, with a peroxide abundance of 0.12 percent relative to water. (For perspective, this is roughly 20 times more diluted than the hydrogen peroxide mixture available at drug stores.) The concentration of peroxide in Europa’s ice then drops off to nearly zero on the hemisphere of Europa that faces backward in its orbit.

Hydrogen peroxide was first detected on Europa by NASA’s Galileo mission, which explored the Jupiter system from 1995 to 2003, but Galileo observations were of a limited region. The new Keck data show that peroxide is widespread across much of the surface of Europa, and the highest concentrations are reached in regions where Europa’s ice is nearly pure water with very little sulfur contamination.

This color composite view combines violet, green, and infrared images of Europa acquired by Galileo in 1997 for a view of the moon in natural color (left) and in enhanced color (right). Credit: NASA/JPL/University of Arizona

The peroxide is created by the intense radiation processing of Europa’s surface ice that comes from the moon’s location within Jupiter’s strong magnetic field.

“The Galileo measurements gave us tantalizing hints of what might be happening all over the surface of Europa, and we’ve now been able to quantify that with our Keck telescope observations,” Brown said. “What we still don’t know is how the surface and the ocean mix, which would provide a mechanism for any life to use the peroxide.”

The scientists think hydrogen peroxide is an important factor for the habitability of the global liquid water ocean under Europa’s icy crust because hydrogen peroxide decays to oxygen when mixed into liquid water. “At Europa, abundant compounds like peroxide could help to satisfy the chemical energy requirement needed for life within the ocean, if the peroxide is mixed into the ocean,” said Hand.

(Source: NASA)

What’s notable to add, on March 26, 2013, the U.S. President signed a bill that would increase the budget for NASA’s planetary science program as well as provide $75 million for the exploration of Europa. Exactly how the funds will be used isn’t clear — perhaps for components on the proposed Europa Clipper mission? — but it’s a step in the right direction for learning more about this increasingly intriguing world. Read more on SETI’s Destination: Europa blog.

April 2, 2013December 23, 2015 by Elizabeth Howell

The Man Who Sold The Moon … And Other ‘Lunarcy’

One man claims to own the moon. Another promises to create effective lunar habitats. And yet another, a former astronaut, paints pictures of its surface.

Lunarcy! is a movie that chronicles our obsession with the Moon. It’s currently making the rounds at independent theatres, but before long it will be easy to watch it on cable, or even Netflix and Amazon.

The film chronicles the efforts of half a dozen people working, in their own way, to bring the notion of regular Moon exploration closer to reality. There’s Alan Bean, the Apollo 12 moonwalker who now paints scenes of lunar exploration. Or Dennis Hope, who has staked a claim on the entire Moon and has sold plots to interested homesteaders.

At the story’s center, however, is an ordinary man called Christopher Carson who is convinced he could be the first person to colonize the Moon — if he could only obtain enough money. Director Simon Ennis follows his efforts to get funds and awareness, sprinkling the rest of the movie with other lunar-loving people.

Universe Today caught up with Ennis, who answered our questions by e-mail.

1) What was your aim with filming/presenting Lunarcy?

As with any film, the aim is to make something that is entertaining, informative and moving. Something that can capture people’s imagination in some way.

2) Why is the moon so attractive to the people in you interviewed?

They all had different reasons. Some want to live there, some are inspired by it, for Dennis Hope (the man who owns it), he saw a business opportunity. Others are interested in space exploration in general and the Moon seems the most practical first step. Apollo astronaut Alan Bean has been there, so his attraction should be obvious.

3) One of your greatest challenges must have been trying to present some of the characters — people such as Christopher Carson, who has been ignored in his belief that living on the moon is possible — in a way that helps the audience feel understanding for their cause. How did you try to do that?

I don’t think that was much of a challenge actually. I only included subjects in the film who I felt a very strong affinity for, whose goals, quests or projects were ones that caught my imagination and that I could get behind myself. Considering that I felt understanding for the “cause”, I figured that would naturally come through to the audience.

4) A minor theme in Lunarcy! is presenting the moon as a viable place to do business — selling plots of land or colonizing it, for example. We also have companies that are looking to mine asteroids. But often, these plans meet with ridicule, as Newt Gingrich discovered when he promised a moon base. What, in your view, will it take for off-earth private ventures such as these to succeed?

I think they will ultimately succeed when they become financially viable industries. For that to happen, I suspect that some of the billionaire space enthusiasts (e.g. [SpaceX‘s Elon] Musk, [Virgin Galactic’s Richard Branson, etc) will have to invest their own funds to get various projects going and to show that they’re not only possible but viable. So far SpaceX seems to be doing just this.

5) What else would you like to add?

Lunarcy! will premiere on EPIX on April 3 and will be available on Netflix and Amazon at the beginning of July.

March 19, 2013December 23, 2015 by Jason Major

Enceladus’ Jets Reach All the Way to its Sea

Saturn's moon Enceladus sprays its salty sea out into space. Those plumes are rich in phosphates. (NASA/JPL/SSI/J. Major)

Thanks to the Cassini mission we’ve known about the jets of icy brine spraying from the south pole of Saturn’s moon Enceladus for about 8 years now, but this week it was revealed at the 44th Lunar and Planetary Science Conference outside Houston, Texas that Enceladus’ jets very likely reach all the way down to the sea — a salty subsurface sea of liquid water that’s thought to lie beneath nearly 10 kilometers of ice.

Enceladus’ jets were first observed by the Cassini spacecraft in 2005. The jets constantly spray fine particles of ice into space which enter orbit around Saturn, creating the hazy, diffuse E ring in which Enceladus resides.

Emanating from deep fissures nicknamed “tiger stripes” that gouge the 512-km (318-mile) -wide moon’s south pole the icy jets — and the stripes — have been repeatedly investigated by Cassini, which has discovered that not only do the ice particles contain salts and organic compounds but also that the stripes are surprisingly warm, measuring at 180 Kelvin (minus 135 degrees Fahrenheit) — over twice as warm as most other regions of the moon.

Where the jets are getting their supply of liquid water has been a question scientists have puzzled over for years. Is friction caused by tidal stresses heating the insides of the stripes, which melts the ice and shoots it upwards? Or do the fissures actually extend all the way down through Enceladus’ crust to a subsurface ocean of liquid water, and through tidal pressure pull vapor and ice up to the surface?

"Baghdad Sulcus," one of many tiger stripe fissures on Enceladus (NASA/JPL/SSI) — “Baghdad Sulcus,” one of many tiger stripe fissures on Enceladus (NASA/JPL/SSI)

Researchers are now confident that the latter is the case.

In a presentation at the Lunar and Planetary Science Conference titled “How the Jets, Heat and Tidal Stresses across the South Polar Terrain of Enceladus Are Related” (see the PDF here) Cassini scientists note that the amount of heating due to tidal stress seen along Enceladus’ tiger stripes isn’t nearly enough to cause the full spectrum of heating observed, and the “hot spots” that have been seen don’t correlate with the type of heating caused by shear friction.

Instead, the researchers believe that heat energy is being carried upwards along with the pressurized water vapor from the subsurface sea, warming the areas around individual vents as well as serving to keep their channels open.

With 98 individual jets observed so far on Enceladus’ south polar terrain and surface heating corresponding to each one, this scenario, for lack of a better term… seems legit.

What this means is that not only does a moon of Saturn have a considerable subsurface ocean of liquid water with a heat source and Earthlike salinity (and also a bit of fizz) but also that it’s spraying that ocean, that potentially habitable environment, out into local space where it can be studied relatively easily — making Enceladus a very intriguing target for future exploration.

“To touch the jets of Enceladus is to touch the most accessible salty, organic-rich, extraterrestrial body of water and, hence, habitable zone, in our solar system.”

– Cassini imaging team leader Carolyn Porco et al.

Enceladus is actively spraying its habitable zone out into space (NASA/JPL/SSI)

Research notes via C. Porco, D. DiNino, F. Nimmo, CICLOPS, Space Science Institute at Boulder, CO, and Earth and Planetary Sciences at UC Santa Cruz, CA.

Top image: color-composite of Enceladus made from raw Cassini images acquired in 2010. The moon is lit by reflected light from Saturn while the jets are backlit by the Sun.

March 19, 2013December 23, 2015 by Nancy Atkinson

Remains of GRAIL Spacecraft Found on Lunar Surface

Before and after the GRAIL twins impacts on the Moon December 17, 2012. The LROC Narrow Angle Camera (NAC) directors were able to resolve the impact sites on February 28, 2013, revealing both to be about 5 meters in diameter. Upper panels show the area before the impact; lower panels after the impact. Arrows point to crater locations. LROC NAC observations M186085512R, M186078336L, M1116736474R and M1116736474L. Credit: NASA/GSFC/Arizona State University.

On December 17, 2012, the GRAIL mission came to an end, and the two washing machine-sized spacecraft performed a flying finale with a planned formation-flying double impact into the southern face of 2.5-kilometer- (1.5-mile-) tall mountain on a crater rim near the Moon’s north pole. The Lunar Reconnaissance Orbiter has now imaged the impact sites, which show evidence of the crashes.

But surprisingly, these impacts were not what was expected, says the LRO and GRAIL teams. The ejecta around both craters is dark. Usually, ejecta from craters is lighter in color – with a higher reflectance – than the regolith on surface.

“I expected the ejecta to be bright,” said LROC PI Mark Robinson at a press conference from the Lunar and Planetary Science Conference today, “because everybody knows impact rays on the Moon are bright. We are speculating it could be from hydrocarbons from the spacecraft.”

GRAIL A site seen before and after the impact event. Crater center is located at 75.609°N, 333.407°E/ Credit: NASA/GSFC/Arizona State University.

Typically ejecta from craters is brighter, since subsurface regolith tends to have a higher reflectance. The lunar regolith on the surface tends to be darker because of its exposure to the vacuum of space, cosmic radiation, solar wind bombardment, and micrometeorite impacts. Slowly over time, these processes tend to darken the surface soil.

Robinson said the hydrocarbons could have come from fuel left in the fuel lines (JPL estimated a quarter to half a kilogram of fuel may have remained in the spacecraft – so, not very much) or from the spacecraft itself, which is made out of carbon material.

GRAIL B site seen before and after impact event. Crater center is located at 75.651°N, 333.168°E. Credit: NASA/GSFC/Arizona State University.

Additionally, the impact craters’ shapes were not as expected. The impacts formed craters about 5 m (15 ft) in diameter, and there is little ejecta to the south – the direction from which the spacecraft were traveling. “The spacecraft came in at a 1 or 2 degree impact angle,” said Robinson, “so this not a normal impact, as all the ejecta went upstream in the direction of travel.”

“I was expecting to see skid marks, myself,” said GRAIL principal investigator Maria Zuber. She added that she was committed to using every bit of fuel to mapping the gravity field at as low an altitude as possible. “I was determined that we would not end the mission with unused fuel because that would have meant we could mapped it even lower.

The spacecraft did end up being able to map the Moon from 2 km above the surface, the lowest altitude from which any planetary surface has ever been mapped, creating an extremely high resolution map.

LRO Wide Angle Camera (WAC) image of the GRAIL impact area on the south side of the unnamed massif. Credit: NASA/GSFC/ASU.

Robinson said he was skeptical that they could find the impact craters, since the team has yet to find the impact sites of the Apollo ascent stages, which should be much bigger than the GRAIL impacts.

“Finding the impact crater was like finding a needle in haystack,” Robinson said, “as the images are looking at an area that is about 8 km wide and 30 to 40 km tall, and we were looking for something that is a couple of pixels wide.”

Robinson said he spent hours looking for it with no luck, only to see it later when he was on a conference call and was just looking at it out of the corner of his eye.

“It was really fun to find the craters,” he said. LRO did take images in early January, but better images were taken on February 28, 2013.

While LRO’s camera was not able to image the actual impact since it occurred on the night-side of the Moon, the LAMP instrument (Lyman Alpha Mapping Project) on LRO was able to detect the plumes of the impacts.

Kurt Retherford, PI of LAMP said the UV spectrograph was pointed towards the limb of the Moon — and actually looking in the direction of the constellation Orion at the time of the GRAIL impact — to observe the gases coming out of the plumes. They did detect the two impact plumes which clearly showed an excess of emissions from hydrogen atoms. “We were excited to see this detection of atomic hydrogen coming from the impact sites,” Retherford said. “This is our first detection of native hydrogen atoms from the lunar environment.”

This video shows LRO as it flies over the north pole of the Moon, where it has a very good view of the GRAIL impact. The second part is the view from LRO through LAMP’s slit, showing the impact and the resulting plume. The orbits, impact locations, terrain, LAMP field of view, and starfield are accurately rendered.

Retherford said further studies from this will help in determining the processes of how the implantation of solar wind protons on the lunar surface could create the water and hydroxyl that has been recently detected on the lunar surface by other spacecraft and in studies of lunar rocks returned by the Apollo missions.

You can see more images from LRO on the LROC website. Additionally, NASA has now issued a press release about this, too.

March 7, 2013December 23, 2015 by Ray Sanders

Join the Golden Spike Video Contest

If you’ve been following Golden Spike Company, you know that the company is planning to launch commercial Lunar exploration missions by 2020.

Last month, Golden Spike announced their Indiegogo crowdfunding campaign to raise funds to help generate public interest in their mission. So far people from around the world have contributed to the Golden Spike Indiegogo campaign.

Today, Golden Spike has announced a video submission contest for their supporters. Keep reading to learn how you can participate!

The video competition is open to anyone who contributes to the Indiegogo crowdfunding campaign at: http://www.indiegogo.com/projects/golden-spike-is-sending-nations-and-people-to-the-moon-join-in

To enter, simply submit your video on why you believe Lunar exploration is important. Golden Spike will accept entries for the first round of the competition until Friday, March 15. All appropriate videos will be uploaded to the Golden Spike Youtube Channel where the public can vote for their favorite via the comments section. The prize for the first round of videos is a lunar rover model (at left).

Email your video submission to: [email protected]

Learn more about Golden Spike Company at: www.goldenspikecompany.com

March 7, 2013December 23, 2015 by Nancy Atkinson

Looking Into the Moon’s Permanently Shadowed Craters

This shaded relief image shows the Moon's Shackleton Crater, a 21-km-wide crater permanently shadowed crater near the lunar south pole. The crater’s interior structure is shown in false color based on data from NASA's LRO probe. Scientists suspect that there's a lot of water ice hidden in the crater's shadow. Credit: NASA

There are some craters on the Moon that never see the light of day. But that doesn’t stop the Lunar Reconnaissance Orbiter from shedding new light on some the darkest mysteries on the lunar surface. With its battery of instruments, LRO has been collecting data so that we can learn more about what we can’t see with our eyes or with optical telescopes. The video provides more details, but by studing the Moon, we’ll improve our understanding of the solar system, bringing new discoveries to light.

For more info, see the LRO website.

February 26, 2013December 23, 2015 by Nancy Atkinson

Astrophotos: The Full Snow Moon

Fishing for walleye on the Bay of Quinte (Lake Ontario) near Belleville, Ontario, when the full Moon appeared through the clouds on the horizon. Credit and copyright: Rick Stankiewicz.

In Native American lore, the full Moon in February is called the Snow Moon, as this time of year usually signals the deepest snows of winter in the now cold northern latitudes in the Northern Hemisphere. This year, the full moon fell on February 25th and here are a few images shared by our readers. Above is a classic view of a winter evening in the north — especially where I used to live in Minnesota, but also where Rick Stankiewicz lives in Ontario, Canada.

“I was fishing for walleye with some friends on the Bay of Quinte (Lake Ontario) near Belleville, Ontario,” Rick wrote, “and I was fortunate to be in an opportune location to see the Moon rising in the eastern sky. “A pale pastel pink disc appeared initially, but as the minutes wore on and the lunar disk rose higher above the horizon it grew brighter and transformed from pink, then red, then orange as it evaded more and more of the earth’s atmosphere along the horizon. What a wonderful sight and this made the whole trip worth the effort. Our fishing party caught one nice fish this trip but the rising of the Snow Moon was the ‘icing on the cake’ for me.”

A beautiful shot too!

See more below:

Planet Moon? A panoramic view from Östersund, Sweden. Credit and copyright: Göran Strand

Here’s a fun panoramic view of the full Moon, which seemingly creates a little snow covered planet with the full Moon in the sky. This was sent in by Göran Strand from Sweden: “I wanted to catch the Moon in a snowy environment,” Göran wrote, “so me and my friend went out on Storsjöns snow-covered ice here in Östersund, Sweden….As a bonus, a light mist came in over the lake just as we arrived.”

The full Snow Moon on 02-25-2013 as seen from Dayton, Ohio USA. Credit and copyright: John Chumack. — The full Snow Moon on 02-25-2013 as seen from
Dayton, Ohio USA. Credit and copyright: John Chumack.

Our pal John Chumack can always be counted on for a great view of the full Moon! You can see more of his images at his Flickr page or his website, Galactic Images.

The Moon partially hidden by tree branches, taken on February 25, 2013. Credit and copyright: Carolyn Postelwait.

The February 2013 full Moon as seen in Michigan, USA. Credit and copyright: Kevin (Kevin's Stuff on Flickr.) — The February 2013 full Moon as seen in Michigan, USA. Credit and copyright: Kevin (Kevin’s Stuff on Flickr.)
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[caption id="attachment_100297" align="aligncenter" width="580"] The full Moon as seen in Japan on Feb. 25, 2013. Credit and copyright: Masashi Ito.

The February 2013 full Moon as seen in Michigan, USA. Credit and copyright: Kevin (Kevin’s Stuff on Flickr.)
[caption]

[caption id="attachment_100297" align="aligncenter" width="580"] The full Moon as seen in Japan on Feb. 25, 2013. Credit and copyright: Masashi Ito.

Want to get your astrophoto featured on Universe Today? Join our Flickr group or send us your images by email (this means you’re giving us permission to post them). Please explain what’s in the picture, when you took it, the equipment you used, etc.

February 19, 2013December 23, 2015 by Nancy Atkinson

Luckiest Photo Ever: The Moon, Jupiter … and More

'Fly Me to the Moons' -- a view of the Moon with Jupiter and the four Galilean moons, along with a passing airplane. Credit and copyright: Greg Gibbs.

“No matter how much you plan and prepare,” said photographer Greg Gibbs, “sometimes you just have to be very lucky.”

As we mentioned last week, Jupiter and the Moon were going to have a close encounter in the sky on February 18, with an occultation visible in some areas. And so Gibbs was preparing to get shots of the occultation through his telescope from his location in Victoria, Australia, and was using an automated timer to get shots at about 10 second intervals But then he noticed lights from a plane coming close to the Moon.

“I realised that there was a chance that it would pass in front of the Moon,” he said, “so I quickly canceled the remote timer I was using to take the shots and instead started shooting high speed continuous frames. I managed to get this plane crossing the moon in five individual frames just as Jupiter was about to be occulted by The Moon.”

This final product, as Gibbs notes on his Facebook page, is a two image composite. The Moon, Jupiter and the plane are all one single image. Then he took an overexposed image to bring up the Galilean Moons of (from left to right) Io, Callisto and Europa. At the time of this shot, Ganymede had already been occulted by The Moon.

There’s the old saying, “If you can’t be good, be lucky…”

This shot may have been lucky, but it sure is good, too!

See more of Gibbs astrophotography at his website, Capturing the Night.

Additionally, Peter Lake from Australia put together this video from last night’s occultation:

February 17, 2013December 23, 2015 by Elizabeth Howell

The Astronomy of Shakespeare

A portrait of William Shakespeare on the cover of the first Folio of his plays. Credit: Elizabethan Club of Yale University

With all this talk lately of rocks whizzing by Earth (or crashing through the atmosphere), it’s remarkable that we didn’t even know of space rocks a few centuries ago. The first asteroid, 1 Ceres, was discovered in 1801.

Dial back a few centuries, and we were still in the realm of a perfect universe with the Earth at the center. William Shakespeare’s (1564-1616) plays are full of these references. Universe Today recently stumbled across a 1964 Irish Astronomical Journal paper replete with examples.

Shakespeare was born about 20 years after Nicolaus Copernicus, whose book De revolutionibus orbium coelestium (On the Revolutions of the Celestial Spheres) laid out the case for the Sun-centered solar system. It took a while for Copernicus’ theories to take hold, however.

While bearing in mind that Shakespeare often wrote about historical personages, one passage from Troilus and Cressida demonstrates an example of the characters speaking of the Sun following the other planets in circles around the Earth.

The heavens themselves, the planets, and this centre,
Observe degree, priority and place.
Insisture, course, proportion, season, form,
Office, and custom, in all line of order:
And therefore is the glorious planet Sol
In noble eminence enthroned and sphered
Amidst the other …

An Earth-centered solar system had its problems when predicting the paths of the planets. Astronomers couldn’t figure out why Mars reversed in its path in the sky, for example.

The real explanation is the Earth “catching up” and passing Mars in its orbit, but astronomers in Shakespeare’s time commonly used “epicycles” (small circles in a planet’s orbit) to explain what was going on. Shakespeare wrote about this problem in Henry VI:

Mars his true moving, even as in the heavens,
So in the earth, to this day is not known.

However, the Bard displayed a more modern understanding of the Moon’s movement around the Earth, the paper points out. The Moon’s distance varies in its orbit, a fact spoken about in Othello, although note that Shakespeare attributes madness to the moon’s movements:

It is the very error of the moon;
She comes more near the earth than she was wont
And makes men mad.

For more examples — including what Shakespeare thought about astrology — you can check out the paper here.

February 12, 2013December 23, 2015 by Ken Kremer

45 meter Asteroid to Skirt Very Near Earth on Feb 15

Asteroid 2012 DA14 Zooms just 17,200 miles above Earth on Feb. 13 in this artist’s concept. Credit; NASA

Our home planet is due for a record setting space encounter on Friday (Feb. 15) of this week, when a space rock roughly half a football field wide skirts very close by Earth at break neck speed and well inside the plethora of hugely expensive communications and weather satellites that ring around us in geosynchronous orbit.

“There is no possibility of an Earth impact” by the Near Earth Asteroid (NEO) known as 2012 DA 14, said Don Yeomans, NASA’s foremost asteroid expert at a media briefing. Well that’s good news for us – but a little late for the dinosaurs.

At its closest approach in less than 4 days, the 45 meter (150 feet) wide Asteroid 2012 DA14 will zoom by within an altitude of 27,700 kilometers (17,200 miles). That is some 8000 km (5000 miles) inside the ring of geosynchronous satellites, but far above most Earth orbiting satellites, including the 6 person crew currently working aboard the International Space Station.

Although the likelihood of a satellite collision is extremely remote, NASA is actively working with satellite providers to inform them of the space rocks path.

The razor thin close shave takes place at about 2:24 p.m. EST (11:24 a.m. PST and 1924 UTC) as the asteroid passes swiftly by at a speed of about 7.8 kilometers per second (17,400 MPH)- or about 8 times the speed of a rifle bullet. For some perspective, it will be only about 1/13th of the distance to the moon at its closest.

“Asteroid 2012 DA14 will make a very close Earth approach, traveling rapidly from South to North and be moving at about two full moons per minute,” said Yeomans, who manages NASA’s Near-Earth Object Program Office at the Jet Propulsion Laboratory in Pasadena, Calif. “That’s very fast for a celestial object.”

Diagram depicting the passage of asteroid 2012 DA14 through the Earth-moon system on Feb. 15, 2013. Credit: NASA/JPL-Caltech

No known asteroid has ever passed so near to Earth.

“This is a record predicted close approach for a known object this size,” stated Yeomans. “Such close flybys happen every 40 years on average. An actual Earth collision would happen about every 1200 years.”

Yeomans said that if an asteroid the size of 2012 DA14 fell to Earth, the impact effect would be similar to the 1908 Tunguska event in Siberia. That was an air blast event that leveled trees over an area greater than about 800 square miles.

So the local effect on human cities for example of a 50 meter wide asteroid impact would be deadly and utterly devastating. But it would not be catastrophic to all life on Earth. Nevertheless, at this moment, Earth has no defenses against asteroids other than talk.

By comparison, the K-T event that caused the mass extinction of the dinosaurs some 65 million years ago was caused by an asteroid about 10 km (6 mi) in diameter. About 2/3 of all species went extinct. If 2012 DA14 impacted Earth the force would be equivalent to about 2.4 megatons of energy (2.4 million tons of TNT), said Yeomans.

Artists concept of meteoroide impact event

There is no danger to the ISS crew and apparently they won’t have any chance to observe it.

“The ISS is not positioned right for observations,” Lindley Johnson, program executive, Near Earth Object Observations Program, NASA Headquarters, Washington, told Universe Today.

“No NASA space-based assets will be making measurements,” Lindley told me. “The asteroid is moving to fast.”

However, radar astronomers do plan to take images around eight hours after the flyby using the Goldstone antenna in California’s Mojave Desert, which is part of NASA’s Deep Space Network.

Some skilful and knowledgeable Earthlings might have a chance to see the asteroid hurtling by with binoculars or a small telescope.

“The asteroid will be observable in the dark sky in Eastern Europe, Asia and Australia, achieving about 7.5 magnitude, somewhat fainter than naked eye visibility,” explained Yeomans. “Closest approach will be over Indonesia.”

Astronomers at the La Sagra Sky Survey program in southern Spain discovered the asteroid in February 2012 just after its last Earth flyby, at a fairly distant 7 Earth-Moon distances. They reported the finding to the Minor Planet Center.

NASA’s NEO group and collaborators in Pisa, Italy then use such data to predict future flight paths and look into past trajectories as well.

Yeomans said that the Feb 15 flyby will be the closest for the next 100 years and its orbit will be perturbed so that it comes back less frequently – changing its orbital class from Apollo to Aten.

Due to its small size and recent discovery, not much is known about the composition of 2012 DA14. It might be silicate rock.

Small space rocks hit Earth on a daily basis amounting to about 100 tons. Car sized rocks hit weekly.

Stay Alert !

Ken Kremer