Universe Today

February 22, 2013June 5, 2022 by Ken Kremer

Historic Mars Rock Drilling Sample Set for Analysis by Curiosity Robot in Search of Organics

First Curiosity Drilling Sample in the Scoop. This image shows the first sample of powdered rock extracted by the rover's drill after transfer from the drill to the rover's scoop. The sample will now be sieved and portions delivered to the Chemistry and Mineralogy instrument and the Sample Analysis at Mars instrument. The scoop is 1.8 inches (4.5 centimeters) wide. The image was taken by Curiosity's Mastcam 34 camera on Feb. 20, or Sol 193.The image has been white-balanced to show what the sample would look like if it were on Earth. Credit: NASA/JPL-Caltech/MSSS

Newly received images from the surface of Mars confirm that NASA’s Curiosity rover successfully extracted the 1st ever samples collected by drilling down inside a rock on another planet and transferred the pulverized alien powder to the robots processing scoop, thrilled mission scientists announced just hours after seeing visual corroboration.

Collecting the 1st particles bored from the interior of a rock on a planet beyond Earth marks a historic feat in humankind’s exploration of the cosmos – and is crucial for achieving Curiosity’s goal to determine whether Mars ever could have supported microbial life, past or present.

The essential next step is to feed carefully sieved portions of the precious gray colored material into the high powered duo of miniaturized analytical chemistry labs (CheMin & SAM) inside the rover, for thorough analysis and scrutiny of their mineral content and to search for signatures of organic molecules – the building blocks of life as we know it.

Curiosity is drilling into ancient bedrock and hunting for clues to the planet’s habitability over the eons and that preserve the historical record – perhaps including organics.

The rover team believes that this work area inside Gale Crater called Yellowknife Bay, experienced repeated percolation of flowing liquid water long ago when Mars was warmer and wetter – and therefore was potentially more hospitable to the possible evolution of life. See our Yellowknife Bay worksite and drill hole photo mosaics below by Ken Kremer & Marco Di Lorenzo, created from rover raw images.

Curiosity accomplished Historic 1st drilling into Martian rock at John Klein outcrop on Feb 8, 2013 (Sol 182), shown in this context mosaic view of the Yellowknife Bay basin taken on Jan. 26 (Sol 169) where the robot is currently working. The robotic arm is pressing down on the surface at John Klein outcrop of veined hydrated minerals - dramatically back dropped with her ultimate destination; Mount Sharp. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo — Curiosity accomplished Historic 1st drilling into Martian rock at John Klein outcrop on Feb 8, 2013 (Sol 182), shown in this context mosaic view of the Yellowknife Bay basin taken on Jan. 26 (Sol 169) where the robot is currently working. The robotic arm is pressing down on the surface at John Klein outcrop of veined hydrated minerals – dramatically back dropped with her ultimate destination; Mount Sharp. Credit: NASA/JPL-Caltech/Ken Kremer (kenkremer.com)/Marco Di Lorenzo

“We collected about a tablespoon of powder, which meets our expectations and is a great result,” said JPL’s Scott McCloskey, drill systems engineer for Curiosity, at a NASA media briefing on Feb. 20. “We are all very happy and relieved that the drilling was a complete success.”

The gray colored tailings from the rocky interior offer a startlingly fresh sight of Mars compared to the red-orangey veneer of rusty, oxidized dust we are so accustomed to seeing globally across what we humans have referred to for centuries as the “Red Planet”.

“For the first time we are examining ancient rocks that have not been exposed to the Martian surface environment, and weathering, and preserve the environment in which they formed,” said Joel Hurowitz, Curiosity sampling system scientist of JPL.

This is a key point because subsequent oxidation reactions can destroy organic molecules and thereby potential signs of habitability and life.

“The tailings are gray. All things being equal it’s better to have a gray color than red because oxidation is something that can destroy organic compounds,” said John Grotzinger, the Curiosity mission’s chief scientist of the California Institute of Technology.

On Feb. 8, 2013 (mission Sol 182), Curiosity used the rotary-percussion drill mounted on the tool turret at the end of the 7 foot (2.1 meter) long robotic arm to bore a circular hole about 0.63 inch (16 mm) wide and about 2.5 inches (64 mm) deep into a red colored slab of flat, fine-grained, veiny sedimentary bedrock named “John Klein” that formed in water.

“Curiosity’s first drill hole at the John Klein site is a historic moment for the MSL mission, JPL, NASA and the United States. This is the first time any robot, fixed or mobile, has drilled into a rock to collect a sample on Mars,” said Louise Jandura, Curiosity’s chief engineer for the sampling system.

“In fact, this is the first time any rover has drilled into a rock to collect a sample anywhere but on Earth. In the five decade history of the space age this is indeed a rare event.”

“The rock drilling capability is a significant advancement. It allows us to go beyond the surface layer of the rock, unlocking a time capsule of evidence about the state of Mars going back 3 or 4 Billion years.”

“Using our roving geologist Curiosity, the scientists can choose the rock, get inside the rock and deliver the powdered sample to instruments on the rover for analysis.”

“We couldn’t all be happier as Curiosity drilled her first hole on Mars,” said Jandura.

Over the next few days, the powdery gray scoop material will be shaken and moved through Curiosity’s sample processing device known as CHIMRA, or Collection and Handling for In-Situ Martian Rock Analysis and sieved through ultra fine screens that filter out particles larger than 150 microns (0.006 inch) across – about the width of a human strand of hair.

Figure shows the location of CHIMRA on the turret of NASA's Curiosity rover, together with a cutaway view of the device. The CHIMRA, short for Collection and Handling for In-situ Martian Rock Analysis, processes samples from the rover's scoop or drill and delivers them to science instruments. Credit: NASA/JPL-Caltech — Figure shows the location of CHIMRA on the turret of NASA’s Curiosity rover, together with a cutaway view of the device. The CHIMRA, short for Collection and Handling for In-situ Martian Rock Analysis, processes samples from the rover’s scoop or drill and delivers them to science instruments. Credit: NASA/JPL-Caltech

Drilling goes to the heart of the mission. It is absolutely indispensable for collecting and conveying pristine portions of Martian rocks and soil to a trio of inlet ports on top of the rover deck leading into the Chemistry and Mineralogy (CheMin) instrument and Sample Analysis at Mars (SAM) instrument .

The sieving process is designed to prevent clogging downstream into the chemistry labs.

The pair of state-of-the-art instruments will then test the gray rocky powder for a variety of inorganic minerals as well as both simple and complex organic molecules.

Samples will be dropped off first to CheMin and then SAM over the next few days. Results are expected soon.

The data so far indicate the drilled rock is either siltstone or mudstone with a basaltic bulk composition, said Hurowitz. The CheMin and SAM testing will be revealing.

The high powered drill was the last of Curiosity 10 instruments still to be checked out and put into full operation and completes the robots commissioning phase.

“This is a real big turning point for us as we had a passing of the key for the rover [from the engineering team] to the science team,” said Grotzinger.

Curiosity has discovered that Yellowknife Bay is loaded with hydrated mineral veins of calcium sulfate that precipitated from interaction with aqueous environments.

I asked how was the drill target hole selected?

“We wanted to be well centered in a large plate of bedrock where we knew we could place the drill into a stable location on an interesting rock,” Hurowitz told Universe Today.

“The drill did not specifically target the veins or nodular features visible in this rock. But these rocks are so shot through with these features that it’s hard to imagine that we would have been missed them somewhere along the travel of the drill.”

“We will find out what’s in the material once we get the materials analyzed by SAM and CheMin.

“We will consider additional drill targets if we think we missed a component of the rock.”

“We believe the white vein material is calcium sulfate based on data from ChemCam and APXS but we don’t yet know the hydration state.” Hurowitz told me.

Regarding the prospects for conducting additional sample drilling and soil scooping at Yellowknife Bay, Grotzinger told me, “We have to take it one step at a time.”

“We have to see what we find in the first sample. We are discovery driven and that will determine what we do next here,” Grotzinger said. “We have no quotas.”

The long term mission goal remains to drive to the lower reaches of Mount Sharp some 6 miles away and look for habitable environments in the sedimentary layers.

Curiosity executed a flawless and unprecedented nail-biting, pinpoint touchdown on Aug. 5, 2012 to begin her 2 year long primary mission inside Gale Crater. So far she has snapped over 45,000 images, traveled nearly 0.5 miles, conducted 25 analysis with the APXS spectrometer and fired over 12,000 laser shots with the ChemCam instrument.

Ken Kremer

Curiosity's First Sample Drilling hole is shown at the center of this image in a rock called "John Klein" on Feb. 8, 2013, or Sol 182 operations. The image was obtained by Curiosity’s Mars Hand Lens Imager (MAHLI). The sample-collection hole is 0.63 inch (1.6 centimeters) in diameter and 2.5 inches (6.4 centimeters) deep. The “mini drill” test hole near it is the same diameter, with a depth of 0.8 inch (2 centimeters). Credit: NASA/JPL-Caltech/MSSS — Curiosity’s First Sample Drilling hole is shown at the center of this image in a rock called “John Klein” on Feb. 8, 2013, or Sol 182 operations. The image was obtained by Curiosity’s Mars Hand Lens Imager (MAHLI). The sample-collection hole is 0.63 inch (1.6 centimeters) in diameter and 2.5 inches (6.4 centimeters) deep. The “mini drill” test hole near it is the same diameter, with a depth of 0.8 inch (2 centimeters). Credit: NASA/JPL-Caltech/MSSS

February 21, 2013December 23, 2015 by Nancy Atkinson

Scientist Who Studied Famous Martian Meteorite Passes Away

NASA scientists David. S. McKay. Credit: NASA

NASA scientist, Dr. David S. McKay has passed away. He may be best known for his paper about a Martian meteorite, ALH84001, which presented an argument that it contained evidence for life on Mars. McKay had been battling serious cardiac health problems for some time, according to an announcement from Johnson Space Center, and he died peacefully in his sleep in the early morning hours of February 20, 2013.

McKay had been the Chief Scientist For Astrobiology at NASA and searched for evidence of past life on Mars using Martian meteorites and terrestrial analogs. He performed original research on lunar soils, lunar pyroclastics, and space weathering.

McKay joined NASA in June of 1965 and participated extensively in astronaut training up until the Apollo 11 mission. He was named a Principal Investigator to study the first returned lunar samples and continued as a lunar sample PI for the next 20 years. He started many of the laboratories for the Lunar Sample Facility at Johnson Space Center and managed the NASA space resources program out of JSC during much of the 1980s.

McKay published more than 200 peer-reviewed papers on lunar samples, space resource utilization, cosmic dust, meteorites, astrobiology and Mars topics, and NASA said his “body of work includes many contributions to our understanding of the development and evolution of the lunar regolith and space weathering processes.”

Most notably, he was the lead author on the 1996 paper in Science on the ALH84001 Martian meteorite that was found in Antarctica and argued that it contains evidence for life on Mars.

“Although that claim was highly controversial, there can be no question that the appearance of that paper sparked significant changes in martian and planetary science, shaped the direction of the Mars Exploration Program to the present day, and prompted the establishment of the NASA Astrobiology Institute,” said the JSC announcement. “Whether one accepts their arguments or not, it has led, directly or indirectly, to investigations seeking and finding signs of life in the most extreme environments. History will judge the value of that rather serendipitous outcome, but it seems clear that its significance is, and will remain, great.”

Astrophoto: Giant Sunspot Group on the Sun

Sunspot 1678 in Hydrogen alpha light, taken on February 19, 2013. Credit and copyright: Paul Andrew.

On February 19 and 20, 2013, scientists watched a giant sunspot form in under 48 hours. It has grown to over six Earth diameters. This image by astrophotographer Paul Andrew shows a detailed, close-up view of this sunspot group, named AR 1678, imaged with a hydrogen alpha filter.

NASA said the spot quickly evolved into what’s called a delta region, which has a magnetic field that harbors energy for strong solar flares. NOAA forecasters estimate a 45% chance of M-flares and a 15% chance of X-flares during the next day.

Below is an image from the Solar Dynamics Observatory of this region on the Sun:

This image of AR 1678 combines images from two instruments on NASA's Solar Dynamics Observatory (SDO): the Helioseismic and Magnetic Imager (HMI), which takes pictures in visible light that show sunspots and the Advanced Imaging Assembly (AIA), which took an image in the 304 Angstrom wavelength showing the lower atmosphere of the sun, which is colorized in red. Credit: NASA/SDO/AIA/HMI/Goddard Space Flight Center — This image of AR 1678 combines images from two instruments on NASA’s Solar Dynamics Observatory (SDO): the Helioseismic and Magnetic Imager (HMI), which takes pictures in visible light that show sunspots and the Advanced Imaging Assembly (AIA), which took an image in the 304 Angstrom wavelength showing the lower atmosphere of the sun, which is colorized in red. Credit: NASA/SDO/AIA/HMI/Goddard Space Flight Center

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February 21, 2013December 23, 2015 by Tammy Plotner

Milky Way Leftover Shell Stars Discovered In Galactic Halo

This illustration shows the disk of our Milky Way galaxy, surrounded by a faint, extended halo of old stars. Astronomers using the Hubble Space Telescope to observe the nearby Andromeda galaxy serendipitously identified a dozen foreground stars in the Milky Way halo. They measured the first sideways motions (represented by the arrows) for such distant halo stars. The motions indicate the possible presence of a shell in the halo, which may have formed from the accretion of a dwarf galaxy. This observation supports the view that the Milky Way has undergone continuing growth and evolution over its lifetime by consuming smaller galaxies. Illustration Credit: NASA, ESA, and A. Feild (STScI)

Like tantalizing tidbits stored in the vast recesses of one’s refrigerator, astronomers using NASA’s Hubble Space Telescope have evidence of a shell of stars left over from one of the Milky Way’s meals. In a study which will appear in an upcoming issue of the Astrophysical Journal researchers have revealed a group of stars moving sideways – a motion which points to the fact our galaxy may have consumed another during its evolution.

“Hubble’s unique capabilities are allowing astronomers to uncover clues to the galaxy’s remote past. The more distant regions of the galaxy have evolved more slowly than the inner sections. Objects in the outer regions still bear the signatures of events that happened long ago,” said Roeland van der Marel of the Space Telescope Science Institute (STScI) in Baltimore, Maryland.

As curious as this shell of stars is, they offer even more information by revealing a chance to study the mysterious hidden mass of Milky Way – dark matter. With more than a hundred billion galaxies spread over the Universe, what better place to get a closer look than right here at home? The team of astronomers led by Alis Deason of the University of California, Santa Cruz, and van der Marel studied the outer halo, a region roughly 80,000 light years from our galaxy’s center, and identified 13 stars which may have come to light at the very beginning of the Milky Way’s formation.

What’s so special about this group of geriatric suns? In this case, it’s their movement. Instead of cruising along in a radial orbit, these elderly stars show tangential motion – an unexpected observation. Normally halo stars travel towards the galactic center, only to return outwards again. What could cause this double handful of stars to move differently? The research team speculates there could be an “over-density” of stars at the 80,000 light year mark.

As intriguing as these stars are, this strange shell was discovered somewhat by accident. Deason and her team winnowed out the outer halo stars from a seven year study of archival images taken by the Hubble telescope of the Andromeda galaxy. While looking some twenty times further away at our neighboring galaxy’s stars, these strange moving stars came to light as foreground objects… objects that “cluttered” the images. While these halo stars were bad for that particular study, they were very good for Deason and the team. It gave them the chance to take a really close look at the motion of the Milky Way’s halo stars.

However, seeing these stars wasn’t easy. Thanks to Hubble’s incredible resolution and light gathering power, each image contained more than 100,000 individual stars. “We had to somehow find those few stars that actually belonged to the Milky Way halo,” van der Marel said. “It was like finding needles in a haystack.”

So how did the astronomers separate the shell stars from those that belonged to the outer fringes of the Andromeda? The initial observations picked the stars out based on their color, brightness and sideways motion. Thanks to parallax, our halo stars seem to move far faster simply because they are closer. Through the work of team member Tony Sohn of STSci, these revolutionary stars were identified and measured. Their tangential motion was observed and recorded with five percent precision. Not a speedy process when you consider these shell stars only move across the sky at a rate of about one milliarcsecond per year!

“Measurements of this accuracy are enabled by a combination of Hubble’s sharp view, the many years’ worth of observations, and the telescope’s stability. Hubble is located in the space environment, and it’s free of gravity, wind, atmosphere, and seismic perturbations,” van der Marel said.

What makes the team so confident in their findings? As we know, stars at home in our galaxy’s inner halo have highly radial orbits. When a comparison was made between the sideways motion of the outer halo stars with the inner motions, the researchers found equality. According to computer simulations of galaxy formation, outer stars should continue to have radial motion as they move outward into the halo, but these new findings prove opposite. What could cause it? A natural explanation would be an accretion event involving a satellite galaxy.

To further substantiate their findings, the team compared their results with data taken by the Sloan Digital Sky Survey involving halo stars. It was a eureka moment. The observations taken by the SDSS revealed a higher density of stars at roughly the same distance as the shell-shocked travelers. And the Milky Way isn’t alone. Other studies of halo stars involved in both the Triangulum and Andromeda show a large number of halo stars existing to a certain point – only to drop off. Deason realized this wasn’t just a weird coincidence. “What may be happening is that the stars are moving quite slowly because they are at the apocenter, the farthest point in their orbit about the hub of our Milky Way,” Deason explained. “The slowdown creates a pileup of stars as they loop around in their path and travel back towards the galaxy. So their in and out or radial motion decreases compared with their sideways or tangential motion.”

As exciting as these findings are, they aren’t news. Shell stars have been observed in the halos of other galaxies and were predicted to be part of the Milky Way. By nature, they should have been there – but they were simply to dim and too far-flung to make astronomers positive of their presence. Not any more. Now that astronomers know what to look for, they are even more anxious to dig into Hubble’s archives. “These unexpected results fuel our interest in looking for more stars to confirm that this is really happening,” Deason said. “At the moment we have quite a small sample. So we really can make it a lot more robust with getting more fields with Hubble.” The Andromeda observations only cover a very small “keyhole view” of the sky.

So what’s next? Now the team can paint an even more fine portrait of the Milky Way’s evolutionary history. By understanding the motions and orbits of the “shell” of stars in the halo, they might even by able to give us a accurate mass. “Until now, what we have been missing is the stars’ tangential motion, which is a key component. The tangential motion will allow us to better measure the total mass distribution of the galaxy, which is dominated by dark matter. By studying the mass distribution, we can see whether it follows the same distribution as predicted in theories of structure formation,” Deason said.

Until then we’ll enjoy the “leftovers”…

Original Story Source: HubbleSite News Release.

February 21, 2013December 23, 2015 by Nancy Atkinson

As Seen From Space: Mt. Etna Boils Over

Lava flows on Mt. Etna visible from the The Advanced Land Imager (ALI) on the Earth Observing-1 (EO-1) satellite captured Etna on February 19, 2013. Credit: NASA

Italy’s Mount Etna has turned on again, spewing lava and gas in its first big eruption in 2013. The volcano is one of the most active in the world, and is Europe’s tallest active volcano, currently standing about 3,329 m (10,922 ft) high.

The volcano has been “simmering” for 10 months, but on February 19 and 20, the famous volcano came to life, providing dramatic visuals from the ground (see the video below) as well as from space, with three outbursts in less than 36 hours. This image from the Advanced Land Imager (ALI) on the Earth Observing-1 (EO-1) satellite captured Etna on February 19 at 9:59 a.m. Central European Time, about 3 hours after the end of the first outbursts.

The false-color image combines shortwave infrared, near infrared, and green light in the red, green, and blue channels of an RGB picture. This combination differentiates the appearance of fresh lava, snow, clouds, and forest.

Fresh lava is bright red—the hot surface emits enough energy to saturate the instrument’s shortwave infrared detectors, but is dark in near infrared and green light. Snow is blue-green, because it absorbs shortwave infrared light, but reflects near infrared and green light. Clouds made of water droplets (not ice crystals) reflect all three wavelengths of light similarly, and are white. Forests and other vegetation reflect near infrared more strongly than shortwave infrared and green light, and appear green. Dark gray areas are lightly vegetated lava flows, 30 to 350 years old.

The video from the ground was captured by Klaus Dorschfeldt, a videographer and webmaster at Italy’s National Institute of Geophysics and Volcanology.

In an update today on the Italian National Institute of Geophysics and Vocanology website, a fourth episode of lava fountains was reported. “Like the previous paroxysms, this event produced fountains and lava and an ash cloud that has shifted to the northern sector of the volcano.”

If you want to keep updated on what Mt. Etna is doing, there’s a webcam where you can watch the eruptions live.

Source: NASA’s Earth Observatory

February 21, 2013December 23, 2015 by Elizabeth Howell

What are the Most Memorable NASA Spacewalks?

Bruce McCandless testing out the ultimate jetpack during STS-41B in February 1984. Credit: NASA

The official name is “extra-vehicular activity,” (EVA) but most of us like to call it a spacewalk. However, when you think about it, you don’t really walk in space. You float.

Or more properly speaking, clutch on to handlebars as you make your way from spot to spot on your spacecraft as you race against the clock to finish your repair or whatever outdoor tasks you were assigned. But hey, the view more than makes up for the hard work.

Some astronauts actually got to fly during their time “outside.” During STS-41B 29 years ago this month, Bruce McCandless was the first one to strap on a jetpack and, in science fiction style, float a little distance away from the shuttle.

He called his test of the manned maneuvering unit “a heck of a big leap”. Nearly 30 years after the fact, it still looks like a gutsy move.

What other memorable floating NASA spacewalks have we seen during the space age? Here are some examples:

The first American one

Ed White did the first American spacewalk in 1965. Credit: NASA

The pictures for Ed White’s spacewalk on Gemini 4 still look amazing, nearly 48 years after the fact. The astronaut tumbled and spun during his 23-minute walk in space, and even tested out a small rocket gun until the gas ran out. When commander Jim McDivitt ordered him back inside, the astronaut said it was the saddest moment in his life.

The dancing-with-exhaustion one

Eugene Cernan during his spacewalk on Gemini 9. Credit: NASA

On Gemini 9, which took place the year after Gemini 4, Eugene Cernan was tasked with a spacewalk that was supposed to test out a backpack to let him move independently of the spacecraft.

Cernan, however, faced a lack of handholds and physical supports as he clambered outside towards the backpack. Putting it on took almost all the strength out of him, as he had nowhere to hold on to counterbalance himself.

“Lord, I was tired. My heart was motoring at about 155 beats per minute, I was sweating like a pig, the pickle was a pest, and I had yet to begin any real work,” Cernan wrote in his memoir, Last Man on the Moon, about the experience.

The situation worsened as his visor fogged up and Cernan struggled unsuccessfully to use the backpack. Cernan was so exhausted that he could barely get inside the spacecraft. “I was as weary as I had ever been in my life,” he wrote.

The three-astronauts-outside one

Three astronauts grab the Intelsat VI satellite during the STS-49 mission. Credit: NASA

Spacewalks traditionally (at least, in the shuttle and station era) happen in pairs, so that if one person runs into trouble there’s another to help him or her out. However, two astronauts working outside during STS-49 couldn’t get enough of a grip on the free-flying Intelsat VI satellite they were trying to fix. So NASA elected to do another spacewalk with a third man.

Pierre Thuot hung on the Canadarm while Richard Hieb and Thomas Akers attached their bodies to the payload bay. Having three men hanging on to the satellite provided enough purchase for the astronauts inside the shuttle to maneuver Endeavour to a spot where Intelsat VI could be attached to the payload bay.

The facing-electrical-shock one

scott parazynski space station — Scott Parazynski repaired a damaged solar panel on the space station. Credit: NASA

In 2007, the astronauts of STS-120 unfolded a solar array on the International Space Station and saw — to everyone’s horror — that some panels were torn. Veteran spacewalker Scott Parazynski was dispatched to the rescue. He rode on the end of the Canadarm2, dangling above a live set of electrified panels, and carefully threaded in a repair.

In an interview with Parazynski that I did several years ago, I asked how he used his medical training while doing the repair. Parazynski quipped something along the lines of, “Well, the top thing in my mind was ‘First do no harm.’ ”

The International Space Station construction ones

Sunita Williams appears to touch the sun during this spacewalk on Expedition 35 on the completed International Space Station. Credit: NASA — Sunita Williams appears to touch the sun during this spacewalk on Expedition 35, which took place on the completed International Space Station. Credit: NASA

Spacewalks used to be something extra-special, something that only happened every missions or, on long-duration ones, maybe once. Building the International Space Station was different. The astronauts brought the pieces up in the shuttle and installed them themselves.

The station made spacewalking routine, or as routine such a dangerous endeavour can be. For that reason, an honorary mention goes to every mission that built the ISS.

What are your favorite EVAs? Feel free to add yours to the comments.

February 21, 2013December 23, 2015 by Nancy Atkinson

Dennis Tito Wants to Send Human Mission to Mars in 2018

Image of Mars from Mars Express. Credit: ESA

According to a press release posted on SpaceRef and NASAWatch, Dennis Tito — the first-ever space tourist — is planning to send a human mission to Mars in January 2018 on a round-trip journey lasting 501 days. The trip would be timed to take advantage of the launch ‘window’ when Mars and Earth reach a position in their respective orbits that offers the best trajectory between the two planets.

Reportedly, Tito has created a new nonprofit company called the Inspiration Mars Foundation to facilitate the mission. The mission is intended to “generate new knowledge, experience and momentum for the next great era of space exploration.”

(2/21/13 13:00 UTC) We have an update on this news below:

Tito, along with several other notable people from the space community will provide more information in a press conference set for Wednesday, February 27th. Also at the press conference will be Taber MacCallum and Jane Poynter who were members of the Biosphere-2 project, and who are with the Paragon Space Development Corporation, which creates life-support systems, and Jonathan Clark, a medical researcher at the National Space Biomedical Research Institute, who may discuss the dangers from radiation to humans in deep space. The press conference will be moderated by journalist Miles O’Brien.

Tito paid about $20 million to visit the International Space Station in 2001.

Another endeavor, the Mars One project, wants to create a human settlement on Mars by 2023.

UPDATE: Spaceflight expert Jeff Foust did a some digging, and posted some insights about this story in his NewSpace Journal. Foust obtained a copy of a paper Tito plans to present at the IEEE Aerospace Conference in March, which discusses conference, a crewed free-return Mars mission that would fly by Mars – no going into orbit or landing. Such a 501-day mission would launch in January 2018, “using a modified SpaceX Dragon spacecraft launched on a Falcon Heavy rocket,” Foust writes. “According to the paper, existing environmental control and life support system (ECLSS) technologies would allow such a spacecraft to support two people for the mission, although in Spartan condition. ‘Crew comfort is limited to survival needs only. For example, sponge baths are acceptable, with no need for showers,’ the paper states.”

One of the paper’s co-authors is NASA Ames director Pete Worden, the paper outlines how NASA would also have a role in this mission in terms of supporting key life support and thermal protection systems, even though this is a private-sector effort. No estimates of what such a mission would cost are included in the paper, but it does say it would be financed privately. The paper adds that if they miss this favorable 2018 opportunity, the next chance to take advantage of this lower energy trajectory would be in 2031.

Read more in Foust’s NewSpace Journal.

We’ll provide more information when it becomes available.

February 20, 2013December 23, 2015 by Fraser Cain

Adaptive Optics Explained! In Comic Form

Emily Coren is an accomplished illustrator and scientist, and she’s figured out how to bring those two skills together to make science easier to understand: science illustrations.

On her blog, Emily regularly illustrates complex scientific topics, creating beautiful images which are half-art/half-educational resource. She illustrates the landscapes out her window on plane flights, jellyfish in the aquarium, and sexy ferns.

Emily completed a series last year on how adaptive optics works. This is the technology that increases the resolution of both telescopes and microscopes, and she gave us permission to reprint the series here on Universe Today.

February 20, 2013December 23, 2015 by Nancy Atkinson

No Glory: NASA Releases Findings from Taurus XL Rocket Failure

Artist concept of the Glory spacecraft in Earth orbit. Credit: NASA Goddard Space Flight Center

NASA has released the findings from a panel that investigated the 2011 crash of the Glory spacecraft after it failed to reach orbit on board an Orbital Sciences Taurus XL rocket, falling into the Pacific Ocean. Early on, the problem was traced to the fairing – the clamshell nosecone that encapsulates the satellite as it travels through the atmosphere — which did not separate from the rocket, weighing the satellite down, preventing its flight toward orbit.

However, the mishap investigation board was not able to identify the definitive cause for the fairing system failure. The rocket and satellite weren’t recovered, so there was no physical evidence to examine. In short, the board confirmed the Taurus launch vehicle’s fairing system failed to open fully and caused the mishap. And the board’s report does recommend ways to prevent future problems associated with the joint system that makes up the fairing.

But the board’s complete report is not available for public release because it contains information restricted by U.S. International Traffic in Arms Regulations (ITAR) and information proprietary to the companies involved.

A similar technical glitch occurred during the 2009 launch of the Orbiting Carbon Observatory (OCO). A replacement, OCO-2 is scheduled to launch in 2014. NASA had originally planned to fly OCO-2 on a Taurus rocket, but changed its plans after the loss of Glory. OCO-2 will now launch on a United Launch Alliance Delta-II. But NASA and Orbital are continuing to investigate the fairing system.

Glory was going to be a three-year mission designed to improve our understanding of Earth’s climate by collecting data on the properties of natural and human-caused aerosols in Earth’s atmosphere and how they might affect climate change, as well as determining the Sun’s affect on climate by measuring the total solar energy entering Earth’s atmosphere.

You can read the summary here. (pdf file).

February 20, 2013December 23, 2015 by Nancy Atkinson

New Video Shows Fire and ‘Rain’ on the Sun

Screenshot of a dazzling magnetic display on the Sun, a phenomenon known as coronal rain. Credit: NASA/SDO

This footage was obtained by the AIA instrument on the Solar Dynamics Observatory on July 19, 2012. It provides a stunning display of solar activity and shows how wildly different events on the Sun can be. Some come just with a solar flare, some with an additional ejection of solar material called a coronal mass ejection (CME), and some with complex moving structures in association with changes in magnetic field lines that loop up into the Sun’s atmosphere, the corona.

This eruption produced all three.

A moderately powerful solar flare exploded on the Sun’s lower right hand limb, sending out light and radiation. Next came a CME, which shot off to the right out into space. And then, the Sun treated viewers to one of its dazzling magnetic displays — a phenomenon known as coronal rain.

Over the course of the next day, hot plasma in the corona cooled and condensed along strong magnetic fields in the region. Magnetic fields, themselves, are invisible, but the charged plasma is forced to move along the lines, showing up brightly in the extreme ultraviolet wavelength of 304 Angstroms, which highlights material at a temperature of about 50,000 Kelvin. This plasma acts as a tracer, helping scientists watch the dance of magnetic fields on the Sun, outlining the fields as it slowly falls back to the solar surface.

SDO collected one frame every 12 seconds, and the movie plays at 30 frames per second, so each second in this video corresponds to 6 minutes of real time. The video covers 12:30 a.m. EDT to 10:00 p.m. EDT on July 19, 2012.