Q & A with Mike Brown, Pluto Killer, part 1

"How I Killed Pluto" -- a new book by planet hunter (and killer) Mike Brown.

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Talk about sticking to your convictions. Astronomer Mike Brown discovered an object that, at the time, was thought to be 27% bigger than Pluto. But he really didn’t want it to be a planet — he had argued against Pluto and other objects he had discovered being planets on the basis that they are in the middle of a “swarm” of similar objects. “To me it made no sense to pull one of even a few objects out of the swarm and call them something other than part of the swarm,” he wrote in his new book, “How I Killed Pluto and Why it Had it Coming.”

Universe Today had the chance to talk with Brown about his book, his discoveries, and even the latest news that perhaps Pluto actually is the biggest dwarf planet out there that we know of. Enjoy part 1 of our Q & A with Mike Brown, with part 2 coming tomorrow.

Also read our review of “How I Killed Pluto,” and find out how you can win a copy!

Universe Today: Over the past couple of weeks, some new discoveries have come out about the size of Eris. What are your thoughts that Pluto may actually be a bit bigger than Eris?

Mike Brown. Credit: CalTech

Mike Brown: The super-cool thing there is that when we first discovered Eris, it was great. I mean, it was fascinating for everyone in the public because we thought it was bigger than Pluto. But scientifically it really didn’t add much to our understanding of the solar system. Eris was kind of just a slightly larger twin of Pluto and nothing new was going on there. That was because we assumed it was near the larger end of the ranges of uncertainty. And by assuming that, we thought Eris was on the smaller end of density, making it the same density as Pluto. When that is the case, it is just a copy. But now that we realize it is essentially the same size as Pluto, that means Eris is a good bit more dense than Pluto, and that is actually really shocking. It tells you that these two things that formed in more or less the same place in the solar system and you would have predicted to have the same composition are essentially very different in composition. I’ve been beating my head against the wall ever since those first reports that Eris was actually smaller.

UT: Your new book, “How I Killed Pluto (and why it had it coming)” is a great read – a real page turner! How long did it take you to actually write your book?

Mike Brown: It was in fits and starts. I started it before the Pluto demotion, and I started it as sort of a ‘discovery of Eris’ book and when it looked like the IAU was going to declare it a planet. And then when it wasn’t a planet and when Pluto became part of the story I restarted it as still about Eris, but also about Pluto. In the end, the sad part of it that nobody really cares about Eris, they only care about Pluto, and so it took me awhile to get back to writing it and get to the point where I could say that this was really about Pluto as well as Eris. So it was over 2-3 years in different chunks, but the final part was a 6 month push in 2009 when I sat down and wrote the whole book.

UT: At the beginning of the book, you portray yourself as sort of stumbling into the field of looking for large objects in the Kuiper Belt. And yet here you are…

Mike Brown: I don’t know if there is any way to know ahead of time how your life is going to work out. Most people don’t have a grand plan they follow and have it work out. You start working on something and sometimes these things work out spectacularly; sometimes it works out OK, and nobody hears about it and sometimes things just don’t work out.

You see people who have done big amazing things, and you wonder how they got from here to there. Usually there is drive to do something, but everybody has to have some luck. They have to have drive and ability, as nobody does it on just luck, though. But there was no requirement that there were these large things out there in the outer solar system, and then the story would have been, “wow, what an idiot. This guy spent two years doing something and nothing came of it.” I had no way of knowing ahead of time which was going to be the answer. I’m lucky, and happy that it turned out the way it did.

Artist concept of Haumea. Credit: NASA

UT: There was a dispute about the discovery of Haumea, where either it was an incredible coincidence that other astronomers may have found the object, too, or they may have stolen your data. In your book you say that you’re fine with not really knowing what happened – which to me is incredibly noble of you (and I think you were very noble about the whole episode). Why don’t you want to know?

Mike Brown: I don’t mean to say I don’t want to know; I would love to know. If you knew the answer and I knew I could ply you with whisky until you told me, I would go out and buy as much whisky as I could. I would love to know the answer. I don’t think I ever will, and so I’m maybe resigned to that. In my gut, I feel like I know what happened, but I really don’t. I could be wrong and then every once in a while I have doubts and say maybe these guys really didn’t do anything wrong and they had their lives ruined. It is very frustrating. I really would like to know the answer because somebody in this story is a bad person, and I hope it is not me. But, god, what if it is?

UT: You certainly gave them the opportunity to tell their side of the story and I don’t know if they really have.

Mike Brown: No, they haven’t. And it is easy to take that interpretation, and if you watch enough “Law and Order” you know that people who hide what is going on are always guilty. But at the same time I try to put myself in their shoes, where they didn’t know what they were about to stumble into, and to suddenly be barraged by the media — to which they weren’t accustomed — and not knowing what to do about it, I can imagine that they wouldn’t tell their side of the story. If everything had been on the up and up, they may have behaved the same way. Deep down inside, I don’t think so, but I don’t have certainty. And I would love to have it. Someday, somewhere, someone may walk into my office and close the door and say, “OK, I know what happened and let me tell you.’ I relish that day, but I don’t know that it will ever happen.

UT: Well, again, I thought you were very nice about the whole episode.

Mike Brown: Before writing the book, I went back and looked at all the emails back and forth about this. The crazy part for me was that my daughter was 20 days old, and these guys had just potentially done something horrible. But when I started writing about it for the book, I didn’t really remember much of it because don’t think anyone remembers much from when their children are 20 days old. I could really only reconstruct it from my own emails with them. And looking back, I am kind of proud of myself. I was really very nice. I was very supportive. I made a big website proclaiming their discovery and pointing everything to them. So, wow, on lack of sleep I’m a relatively nice guy.

Perhaps it helps having a little infant that you are carrying around for perspective as far as what is important and what isn’t. As trite and cliché-ish as that is, I think it is actually true.

UT: But yet, you seem to relish the role of “Pluto Killer”…

Check back tomorrow to find out Mike Brown answers this question, and more!

Review: “How I Killed Pluto and Why it Had it Coming” — Plus win a copy!

"How I Killed Pluto" -- a new book by planet hunter (and killer) Mike Brown.

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It’s hard to imagine, but in 1992 astronomer Mike Brown didn’t know what the Kuiper Belt was. He had never heard of it. But just a few years later in 1999, he bet another scientist that within five more years he would find another planet out there at the edge of the solar system, past Pluto. It took a five-day extension of the bet, but Brown did it. And so began the death of Pluto as a planet, but the rise of a whole new class of objects called dwarf planets. Brown has written a book about his adventures as a planet hunter and eventual planet killer, called “How I Killed Pluto and Why it Had it Coming.”

(Read our exclusive Q & A with Mike Brown!)


His book is a highly readable, first person account of an astronomer who, by chance, realized he had remarkable penchant for discovering small, far away objects. The book is filled with humor, candor, geeky tendencies (he thought the first sonogram of his daughter looked like images from Venera 2 spacecraft from Venus), engaging personal anecdotes – and even romance, intrigue, mystery, fatherly love, and science.

“Discovery is exciting,” Brown writes in his book, “no matter how big or small or close or distant. But in the end, even better is discovering something that is capable of transforming our entire view of the sun and the solar system.”

And Brown’s discoveries have transformed our view of the solar system (some people have changed the world — how many can claim they have changed the solar system?!)

The discoveries of more objects in the Kuiper Belt turned on the heat of the debate of whether everyone’s favorite misfit planet, Pluto, was actually a planet or just a member of a new, quickly growing class of what are now called dwarf planets.

From this, some will claim, our planetary mnemonic went from “My Very Educated Mother Just Served Us Nine Pizzas” to “Mean Very Evil Men Just Shortened Up Nature.”

Mean and evil or educated? You decide.

Want a chance to win a copy of the book? Universe Today has 5 copies to giveaway!

UPDATE: We have winners! They are:

Gadi Eidelheit
Jason McInerney
Sten Thaning
Pam Jacobson
John Wenskovitch

Congrats!

Just send an email to [email protected] with the subject line of “Killing Pluto” by Monday, December 6 at 12 Noon Pacific Daylight Time. We’ll randomly choose 5 emails and notify the winners.

Find more about the book at Amazon.com (the book will be available on Dec. 7, 2010) or at Mike Brown’s website, Mike Brown’s Planets. Here’s a link to the section on his website about the book.

Celebrate the Holidays, From Space!

Zooniverse's Advent Calendar.

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Its December, so many people are getting ready to celebrate … something, be it Hanukkah, Christmas, Winter Solstice, National Pie Day (today!), Emily Dickinson’s birthday (Dec. 10) or National Wear Plunger on Your Head Day (Dec. 18), or just being able to get together with family or having some time off work.

To help you celebrate, there are lots of online spacey goodies. The Zooniverse started the Zooniverse Advent Calendar, similar to the one-a-day-chocolate-treat calendars we all love, but this calendar includes a surprise each day such as special images, downloads and even a couple of very big pieces of news (since no one has figured out how to send chocolate over the web, yet.) Click this link, or the top image to access, as the calendar is now operational.

Emily Lakdawalla at the Planetary Society Blog has her own advent calendar with image treats, and Door Number 1 is now open! Emily’s calendar goes all the way to the New Year, which is even better for more great images.

And there’s more!

The Boston Globe’s Big Picture has their third annual Advent Calendar of Hubble Pictures.

Love Hubble, and want to send space-themed holiday cards? The folks from the Hubble Space Telescope have a great collection of beautiful cards you can download, and send. The cards are designed to be printed out at photo stores or online photo labs, though you can also use a home printer.

A Chandra e-card.

Looking for E-cards? The Chandra website has a great selection of all-occasion cards to send, and here, specifically, is a link to their winter holiday cards.

If you’d like to send an e-card specifically to the astronauts on board the International Space Station, NASA has a website just for you. NASA even encourages you to send a holiday Tweet to any of their astronauts.

SpaceWeather.com has a selection of e-cards, too.

If you are looking for holiday gift ideas with a space or astronomy theme, AmericaSpace has some ideas, Space Center Houston has an idea for that special space enthusiast on your list, The Space Store is an obvious place to look for space-related holiday gifts, and the National Geographic Store has a space section, too. Of course, just searching for “astronomy” on sites like Amazon.com will provide a boatload of ideas.

Where In The Universe #127

It’s time once again for another Where In The Universe Challenge. Name where in the Universe this image was taken and give yourself extra points if you can name the telescope or spacecraft responsible for the image. Post your guesses in the comments section, and check back on later at this same post to find the answer. To make this challenge fun for everyone, please don’t include links or extensive explanations with your answer. Good luck!

UPDATE: The answer has now been posted below:

This is Mars, as seen by the HiRISE camera on the Mars Reconnaissance Orbiter. It is sandfalls in the north polar region of the planet. This image was part of the new PDS release this week. You can see a color version and get more info on this image at this link on the HiRISE website.

And you can now find the answer to last week’s WITU challenge (which was of the image below) back at the original post (sorry for the delay in posting the answer!)

Lockheed Martin Wants to Launch Orion Spacecraft – on a Delta IV Heavy

If everything goes according to their plan - Lockheed Martin would have their Orion spacecraft launch on a Delta IV Heavy rocket. Image Credit: NASA

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After the announcement of the Vision for Space Exploration (VSE) one of the proposals to reduce the space flight ‘gap’ between the shuttle program and the Constellation Program was to attach the Crew Exploration Vehicle (CEV) to a Delta IV Heavy rocket. With all the political wrangling this simple solution appeared lost – or so it was thought. The idea of man-rating a Delta IV heavy never seemed to quite fade away and now a plan is under way to launch the Orion spacecraft on top of one of these massive launch vehicles – within the next three years.

More importantly by launching these test flights, NASA will be able to review up to three-quarters of the technical challenges involved with a flight to either the moon or to an asteroid – without risking a crew. Some of the elements that would be checked out on this unmanned test flight would be:

• Spacecraft stabilization and control.

• Parachutes used for reentry and other systems used to recover the spacecraft.

• Micrometeoroid shielding along with other systems used to protect the vehicle.

The manufacturer of the Orion spacecraft, Lockheed Martin, plans to have the first flight take place as soon as 2013. This test flight would launch from Cape Canaveral Air Force Station’s Space Launch Complex 37. If all goes well? Astronauts could be riding the Delta IV heavy to destinations such as the moon or an asteroid by 2015. For now though these plans are still in their infancy.

If all does go according to how Lockheed Martin human spaceflight engineers plan – the first mission to an asteroid could beat the 2025 date that President Obama set during his April visit to Kennedy Space Center – by ten years.

Each successive flight after the first unmanned mission would shake out the technology more and more until crews fly into orbit. The first unmanned flight, as envisioned by Lockheed Martin, would emulate many of the elements of a mission to either an asteroid or to the moon.

For long-time followers of the space program, witnessing a man-rated launch of a Delta IV heavy will very much be a blast from the past. In the early days of the space program astronauts rode Atlas and Titan rockets into orbit (these rockets were actually man-rated Cold-War missiles). Attached atop the Delta IV would be the Orion capsule and on top of that would be a Launch Abort System (LAS). This last component is a small mini-rocket that would pull the capsule up and away from the Delta if there is an emergency.

Once the flight is completed, the Orion will splashdown in the same general area as Space Exploration Technology’s (SpaceX’s) Dragon Spacecraft – the Pacific Ocean off the coast of California.

The Orion Spacecraft has proved itself to be a survivor. President Obama initially promised to support NASA’s lunar ambitions on the campaign trail – a promise he went back on once elected. He then attempted to cancel all elements of the Constellation Program of which Orion was a key part. This proposal landed with a resounding thud. He then attempted to gain support for his space plan by resurrecting Orion as a stripped down lifeboat for the International Space Station (ISS) – this too met with little support. Eventually, after much Congressional wrangling, Orion emerged as the one element of Constellation – which Obama could not kill.

Congress has put some support behind his plan to have commercial space firms provide transportation to low-Earth-orbit (LEO). However, these firms have no experience whatsoever launching men and material to orbit – and Congress wanted to have a backup plan – that meant Orion. As the launch vehicle that would have hefted Orion to orbit was effectively dead another rocket was required – the best candidate was the Delta IV heavy.

Within three years a Delta IV Heavy like this one could launch the first Orion capsule. Photo Credit: Universe Today/Alan Walters - awaltersphoto.com

Carnival of Space #179

This week’s Carnival of Space is hosted by Bruce over at Weird Sciences.

Click here to read the Carnival of Space #179.

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, let Fraser know if you can be a host, and he’ll schedule you into the calendar.

First Super-Earth Atmosphere Observed

Artist’s impression of GJ 1214b
Artist’s impression of GJ 1214b

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With the recent milestone of the discovery of the 500th extra solar planet the future of planetary astronomy is promising. As the number of known planets increases so does our knowledge. With the addition of observations of atmospheres of transiting planets, astronomers are gaining a fuller picture of how planets form and live.

Thus far, the observations of atmospheres have been limited to the “Hot-Jupiter” type of planets which often puff up, extending their atmospheres and making them easier to observe. However, a recent set of observations, to be published in the December 2nd issue of Nature, have pushed the lower limit and extended observations of exoplanetary atmospheres to a super-Earth.

The planet in question, GJ 1214b passes in front of its parent star when viewed from Earth allowing for minor eclipses which help astronomers determine features of the system such as its radius and also its density. Earlier work, published in the Astrophysical Journal in August of this year, noted that the planet had an unusually low density (1.87 g/cm3). This ruled out an entirely rocky or iron based planet as well as even a giant snowball composed entirely of water ice. The conclusion was that the planet was surrounded by a thick gaseous atmosphere and the three possible atmospheres were proposed that could satisfy the observations.

The first was that the atmosphere was accreted directly from the protoplanetary nebula during formation. In this instance, the atmosphere would likely retain much of the primordial composition of hydrogen and helium since the mass would be sufficient to keep it from escaping readily. The second was that the planet itself is composed mostly of ices of water, carbon dioxide, carbon monoxide and other compounds. If such a planet formed, sublimation could result in the formation of an atmosphere that would be unable to escape. Lastly, if a strong component of rocky material formed the planet, outgassings could produce an atmosphere of water steam from geysers, as well as carbon monoxide and carbon dioxide and other gasses.

The challenge for following astronomers would be to match the spectra of the atmosphere to one of these models, or possibly a new one. The new team is composed of Jacob Bean, Eliza Kempton, and Derek Homeier, working from the University of Göttingen and the University of California, Santa Cruz. Their spectra of the planet’s atmosphere was largely featureless, showing no strong absorption lines. This largely rules out the first of the cases in which the atmosphere is mostly hydrogen unless there is a thick layer of clouds obscuring the signal from it. However, the team notes that this finding is consistent with an atmosphere composed largely of vapors from ices. The authors are careful to note that “the planet would not harbor any liquid water due to the high temperatures present throughout its atmosphere.”

These findings don’t conclusively demonstrate that nature of the atmosphere, but narrow down the degeneracy to either a steam filled atmosphere or one with thick clouds and haze. Despite not completely narrowing down the possibilities, Bean notes that the application of transit spectroscopy to a super-Earth has “reached a real milestone on the road toward characterizing these worlds.” For further study, Bean suggests that “[f]ollow-up observations in longer wavelength infrared light are now needed to determine which of these atmospheres exists on GJ 1214b.”

Red Dwarf Discovery Changes Everything!

Artists Impression of a Red Dwarf (courtesy NASA)

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Its often said that the number of grains of sand on Earth equals the number of stars in the Universe. Well it looks like a recent study by astronomers working at the Keck Observatory in Hawaii have found that its more like three times the number of grains of sand on Earth! Working with some of the most sophisticated equipment available, astronomers from Yale University have been counting the number of dim red dwarf stars in nearby galaxies which has led to a dramatic rethink of the number of stars in the Universe.

Red dwarfs are small, faint stars compared to most others and until now, have not been detected in nearby galaxies. Pieter van Dokkum and his team from Yale University studied eight massive elliptical galaxies between 50 and 300 million lights years from us and discovered that these tiny stars are much more bountiful than first thought. “No one knew how many of these stars there were,” said Van Dokkum. “Different theoretical models predicted a wide range of possibilities, so this answers a long standing question about just how abundant these stars are.”

For years astronomers have assumed that the number of red dwarfs in any galaxy was in the same proportion that we find here in the Milky Way but surprisingly the study revealed there are about 20 times more in the target galaxies. According to Charlie Conroy of the Harvard-Smithsonian Center who also worked on the project, “not only does this affect our understanding of the number of stars in the Universe but the discovery could have a major impact on our understanding of galaxy formation and evolution.” Knowing that there are now more stars than previously thought, this lowers the amount of dark matter (a mysterious substance that cannot be directly observed but its presence inferred from its gravitational influence) needed to explain the observed gravitational influence on surrounding space.

Not only has the discovery affected the amount of dark matter we expect to find but it also changes the quantity of planets that may exist in the Universe. Planets have recently been discovered orbiting around other red dwarf stars such as the system orbiting around Gliese 581, one which may harbour life. Now that we know there are a significantly higher number of red dwarfs in the Universe, the potential number of planets in the Universe has increased too. Van Dookum explains “There are possibly trillions of Earth’s orbiting these stars, since the red dwarfs they have discovered are typically more than 10 billion years old, so have been around long enough for complex life to evolve, its one reason why people are interested in this type of star.”

It seems then that this discovery, which on the face of it seems quite humdrum, actually has far reaching consequences that not only affect our view of the number of stars in the Universe but has dramatically changed our understanding of the distribution of matter in the Universe and the number of planets that may harbour intelligent life.

The new findings appear in the Dec. 1st online issue of the journal Nature.

Source: from the Harvard Smithsonian Center for Astrophysics.

Mark Thompson is a writer and the astronomy presenter on the BBC One Show. See his website, The People’s Astronomer, and you can follow him on Twitter, @PeoplesAstro

ε Eridani’s Dust Disc

This artist's conception shows the closest known planetary system to our own, called Epsilon Eridani. Credit: NASA/JPL/Caltech

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Many stars have been discovered to have narrow discs of warm dust surrounding them. Since dynamical effects with the star’s solar winds should clear these out over long timescales, it’s presumed that these must be recently formed, likely through collisions of small rocky bodies in an asteroid or Kuiper belt. Such a disc has been detected around the nearby star ε Eridani. However, ε Eridani is also known to harbor one planet at a distance of 3.4 AU, and a second one at 40 AU is suspected. Because of this inner planet, any asteroid belt that close would be dynamically unstable as well and should have been cleared out long ago rendering the system incapable of producing dust in this region. So where did ε Eridani get this dust? A new study investigates this.

The inner dust ring was first discovered by a team of astronomers working with the Spitzer Space Telescope last year. In addition to this mysterious inner ring, the system also contains an outer, cold ring of dust at distances greater than 65 AU with a more clumpy nature, possibly shepherded by the outer planet.

The authors of the new paper, led by Martin Reidemeister at Friedrich-Schiller University in Germany, propose that the inner dust ring wasn’t originally formed there. Instead, they propose it was created via collisions in the outer Kuiper belt with the outer ring, but migrated inwards due to an effect known as Poynting-Robertson drag. This effect is created when outflows from the star interact with small objects. While the outflows will ultimately be streaming perpendicular to the orbit, the motion of the orbiting particles will make them plow through this, making them appear to have a component of motion towards the particle in the particle’s reference frame. This is the same effect that makes rain seem as if it’s falling towards you as you’re driving and causes it to pile up on your windshield. Since this added component of motion is opposed to the motion of the particle, it robs the particle of angular momentum, causing it to spiral inwards. Given that ε Eridani is known to have strong winds, this effect seems primed to be an explanation.

To test this hypothesis, the team modeled the system, varying the eccentricity of the inner planet between two possible orbits for the inner planet, both with and without the outer planet, and varying compositions for the outer dust ring (more or less silicates vs. ice). The team found that they could reasonably reproduce the observed system if the dust started as a mixture of ices and silicates in which the ices underwent sublimation as they moved inwards, past the snow line. Additionally, the orbit of the inner planet, though strikingly different for the two proposed orbits, did not have a large effect on the overall distribution of dust.

In the near future, ε Eridani is slated to be the subject of further publications probing its dust discs. The author notes that other teams have already conducted observations using the James Clerk Maxwell Telescope as well as others and that, ε Eridani will likely be a prime target for the James Webb Space Telescope upon launch.

Secret Mini Space Shuttle Could Land on Friday

The X-37B spaceplane sits on a runway at Vandenberg Air Force Base during prelaunch taxi tests. Credit: U.S. Air Force

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The US Air Force announced that the X-37B Orbital Test Vehicle, a miniature, unmanned space shuttle could return to Earth as soon as this Friday, December 3. It has been in Earth orbit for about nine months on a classified mission for the military. It will land at Vandenberg Air Force Base in Los Angeles sometime between Friday and Monday, Air Force officials said in a statement. The exact time of touchdown will depend on weather conditions and technical factors.

Preparations for the landing began on Tuesday, the Air Force Space Command said. The backup landing site would be Edwards Air Force Base.

The X-37B launched from Cape Canaveral, Florida on April 22. It was built by Boeing, and the vehicle looks like a space shuttle orbiter, but is much smaller: at 9 meters long and 4.5 meter wide (29 X 15 ft), with a payload bay that is 2.1 by 1.2 meters (7 by 4 feet) the X-37B is about 1/4th the size of a shuttle.

Launch of the X37-B. Credit: Alan Walters (awaltersphoto.com) for Universe Today

The X-37B uses solar arrays and lithium ion batteries to generate power instead of fuel cells like the space shuttle, a major reason why it can stay on orbit for much longer.

Originally the vehicle was scheduled for launch in from the payload bay of the Space Shuttle, but that plan was axed following the Columbia accident.

The X-37B’s mission is to “demonstrate a reliable, reusable, unmanned space test platform for the United States Air Force,” according to a fact sheet put out by the military. “Objectives of the OTV program include space experimentation, risk reduction and concept of operations development for reusable space vehicle technologies.”

It will be interesting to see if the military will share any of the on-orbit activities of the space plane and what capabilities and uses this vehicle might have in the future.

See our previous article “What is the Air Force’s Secret X-37B Space Plane Doing in Orbit?” for more information.

Source: Air Force Space Command