In my previous post, I tried to explain how all those odd names ended up in my recently-published book and why I think it’s fun to play around with languages in the middle of a story.
So, what if you don’t really care about all that linquistic
nonsense, but just want a guide to pronouncing stuff in this particular story? In what follows, I’m going to share what I’ve
prepared for the person doing our audio book.
On the surface, it may look daunting, but, really, it all hangs together
with a few key elements:
Lots of the names end in a shortened “ay” sound I’ve tagged here as ei. It sounds almost like a long ay, but is cut short like you were going to pronounce a “y” on the end, but stopped yourself just in time, “say” without that teensy “eeya” sound that wraps up that word. Sort of like “sensei” as pronounced in Japan, or at least in anime and Japanese TV shows.
In names ending in e, the final e is always sounded–usually as that shortened “ay” sound.
The exception is “ere”, which is ayr-ee, wherever it happens to fall, so some names end with ayr-ee, while some have that in the middle or at the beginning.
Children (or adults being teased as if they are children) or intimate friends get their names shortened with a bit of a stop in the middle, so Ansegwe becomes An-s-wei, and Kantalare becomes K-a-la-rei
As an example of the “translated words” system: the “aunts” are “awnts”, Brit/Northeast/Southern style, rather than Midwestern style “ants”.
Digression: How come I like weird names? Well, jeepers, I’ve got one of my own, one
that often gets pronounced weird, though I don’t care, really, I’ve heard ’em
all. The “correct” way is
va-‘ness-uh ma-‘cla-ren-‘ray. There are
other pronunciations in use . . . but those are other Vanessas and other MacLarens.
OK, here we go. I’m not using really formal linguistic notation, but sound-shorthand that I think we all can follow. I put a single quote at the front of the stressed syllable in each word.
Our Main Characters
Varayla Ansegwe, Eskenyan Jemenga, Ensense Kantalare,
Varaylas Ansele and Adeleke, and Haillyen.
These all appear frequently, though it takes a while for Kantalare to
show up. See how what we call “last
names” (family names) come first, and “first names” (personal
names) come second.
Wary, indeed. Photo of sketch on wall, by Quinn Dombrowski, Berkeley, CA (CC BY-SA 2.0)
Varayla: Va-‘ray-la This
one’s pretty phonetic, the tricky thing, from listening to auditions for our
audio book, is that some people seem to read the “yla” as
“lya”. This reminds me of how
people read the second half of my last name as “Wary” instead of
“Wray”. Don’t let it worry
you, but if you prefer mispronouncing Varayla, just don’t go to Korlo.
In the bad old days, you could earn a set of cement overshoes for
mispronouncing that name to the wrong person.
Ansegwe: ‘ahn-seg-wei Our hero’s name is most likely to be mispronounced as on-‘seg-way, which is hilarious, as it makes me picture this enormous klutz trying to ride a Segway. The first syllable should be said relatively slowly, so the second two click together fast, so that you almost lose the sound of the “e” in the middle: ahns’gwei. It has a kind of Japanese flavor to it.
Eskenyan: ess-‘ken-yan It
sounds sort of like “a person from Kenya” (at least the way Americans
say it) plus “Ess” in front of it.
Jemenga: ja-‘meng-uh When
Jemenga is particularly pleased with himself, he really hits that middle
syllable, so it’s like Ja-MENG-ah!
The Varayla Syndicate’s above-board operations include space-based solar power satellites. (Not quite like this. This is NASA’s Solar-b satellite)
Ansele: ‘ahn-se-lei Tycoon
aunt #1.
Adeleke: a-‘del-e-kei Tycoon
aunt #2.
Haillyen: ‘hay-ul-lee-yen This is a “foreign” word to Ansegwe, so he’s basically phonetically “translated” it, the ‘y’ in the last syllable is a bridge sound you get when putting ee and en together between the ee and the en. Do ya get it? Yeah? The reader should get it about 100 pages before Ansegwe catches on.
Ensense: en-‘sens-ei You know, like, “sensei” with an “en” at the front.
Kantalare: kahn-tah-‘lahr-ei There’s a secondary stress on the first syllable. Just make it sound pretty in your head. Ansegwe is totally in love with her, so, whatever, hear her as beautiful
2. The people on the expedition
Some of these folks are only mentioned or quoted during the “expedition” chapters.
Tkonle: t-‘kawn-lei
Kulandere: koo-lahn-‘dayr-ee
Tekere: ta-‘kayr-ee
Tereinse: ‘tayr-ee-in-sei
Alekwa: ah-‘leek-wah
Nara: ‘nah-rah
Ensargen: en-‘sahr-gen It’s
a hard g, as in “gun”, not a soft one as in “generation”.
They don’t really use hard “g”
Korton: ‘kor-tun
Alawere: ah-la-‘wayr-ee
Tasegion: tah-‘seg-ee-on
Turame: too-‘rah-mei
3. People at home
Kateseo: ka-‘tay-see-oh
Kinshada: kin-‘shah-dah
Tumbal: ‘toom-bal
Erekulu: ayr-ee-‘koo-loo OK,
this one isn’t a person, he’s a domesticated animal, so his name is a little
goofy, meant to sound cute.
Tokal: toh-‘kahl
Ans’we: ‘ahn-se-wei This is
a nickname for Ansegwe, used mostly by Kantalare, but also used by his
expedition “friends” when they want to get on his case.
K’alare-: kah-‘lahr-ei This
is a nickname for Kantalare, used by Ansegwe.
Az-dyel: ahz-dee-‘ell Note
that this is another “foreign” word that Ansegwe has transcribed this
way, so it’s pretty phonetic, the three syllables have almost equal stress, I
hear just a little more on the last one, but you can feel more free to mess
around with this one–it’s the ONLY word in this language that appears at all.
Eskewere: ess-ke-wayr-ee
Ensense Halense: en-‘sen-sei hah-‘len-sei This is a member of Kantalare’s extended family that they happen to run into at some point.
4. List of authors.
About two-thirds of the way through, someone gives Ansegwe a
reading list, and the authors of the books are a mix of people from his world,
one from outside his culture, and one (the last) he’s going to spend a lot of
time with. I wouldn’t worry about these too much, but have fun with them. Yeah, uh-huh, that’s intentional.
Asvelan Kulumbu: ‘ahs-veh-lahn koo-‘loom-boo
Palawan Vejr: ‘pah-lah-wahn vee-‘yay-zher
Trjia Qwijlian: ‘trr-zhee-ah ‘kwizh-lee-ahn
Tsulander Tkonle: ‘Tzoo-lahn-der T’kawn-lei
5. People in quotes.
Yeah, this is one of those books where each chapter opens
with a quote from someone. I picture
these as remarks that people who know Ansegwe have made when interviewed about
the events in the story. Picture them
sitting across the desk on their version of The Daily Show, chatting with their
Trevor Noah. Most of the quoted
individuals made it into the final. A
few only get mentioned in these quotes.
These ones are mostly government officials. Make them sound stuffy, self-important, and
less-than-competent.
Insake Hailaware: ‘in-sah-kei hai-uh-la-‘wahr-ei (For fussiness, there’s
a secondary stress on first syllable in Hailaware. He will get all huffy if you
miss that and maybe will find some minor infraction to write you up for.)
Elesennen Haileski:
el-es-‘sen-en hai-uh-‘les-kee
Kinsala Tkerelon: kin-‘sah-lah T-‘kayr-ee-lon
6. Other words and place names.
The story takes place in a fairly limited set of
“alien” geographic locations.
But I do have some place names included and there are a few other
“thing” words that appear more than once.
The Kalinidor is something like this. Alexander Fleming’s Nobel Prize (1945) (Jemenga would discover penicillin if someone else hadn’t already.) Source: Science and Society Picture Library, London Museum of Science (CC BY-SA 2.0)
Korlo: ‘kor-low It simply
sounds like “core” “low”.
This is Ansegwe’s country.
Kalinidor: ka-‘lin-ee-dor This
is a person’s name that’s become an object name–sort of like the Nobel Prize, well,
actually, exactly like the Nobel prize.
Jemenga really really wants one of these.
Quazwallade: kwaz-‘wall-ah-dei This is a place name, just a foreign country,
one with some technological and cultural differences from Korlo.
Cignali: sig-‘nah-lee Let’s
say that probably this was originally a person’s name, but now it’s the name of
a famous university, think “Stanford”.
Utumwe: oo-‘tum-wei I told
you there were academics in this story.
This is another university, a medical school actually, one that Jemenga
lectures at, when they can get him.
Terende: ta-‘ren-dei Another place name.
Tule: ‘too-lei Yep, place
name. Doesn’t get much play, but even minor places count, says the writer who
lives in a town that isn’t a proper town, just a collection of farms, houses,
shops, and a gas station, that gets its own post office.
When I post on the front page of my site, it has to be temporary, but it’s often goodies that I don’t want to trash, so I’m beginning a little practice of shifting the “old” content to a NEW blog post, maybe with a little bit of extra commentary. Skip it if you want, or not, whatever. This is the blog part of this page, it’s my playground and as long as I’m not hurting anybody, I can do whatever I want, right?
Like, right now, I’m listening to Travis music videos on YouTube. There are official ones and unofficial ones, and these guys are so menschy, they don’t worry about the unofficial ones, because fans love them, right? Besides, what does it make me want to do? It makes me want to go see if there’s an album of theirs I maybe don’t have yet. Marketing, kids.
The funniest one is a concert video where whoever has the camera skips real fast past the audience members closer to the band’s age and lingers on the fresh-faced youngsters. Well, it’s nice that younger people have discovered them, isn’t it?
hehehe
A few of my Travis CD’s. And yeah one’s a (legit) digital download that was a gift with Keane music on it, too.
All right then, here’s a nostalgic look at the front page that’s going away today:
Greetings, fellow star travellers! Big news!
Paper Angel Press has launched a new imprint devoted to science fiction and fantasy.
I’ve been waiting for months to say: you’ll now find my book at Water Dragon Publishing. Click the dragon and explore their new site.
Meanwhile … my newsletter launched successfully last month! Thanks to all who signed up here and through StoryOrigin. The newsletter comes out mid-month, with science news, story previews, writer-life chat, and just a little gaming stuff.
Learning by doing! I ran an experiment: subscriber pop-up vs static subscribe-here form. The pop-up wins, hands, down. Apparently, it’s just way more convenient. However, I can flip a switch so it only asks every so often. And I’m keeping the static forms on the contact and blog pages, for those who prefer that. Remember, if you’re on gmail, Google will tend to pipeline emails from new people into preset folders like “Promotions,” until you tell it not to.
What would you say if someone said, “Will you take this alien creature home and be responsible for it.”? Ansegwe says, “Yes.” Get the story in digital, audio, softcover, or hardback!
This first-contact story explores the challenges of communication between species–when neither side has a universal translator to rely on, when the alien in question is so odd most people would consider it an animal–not a person, and when accidents and misunderstandings get in the way.
Ansegwe’s a tagalong, a wannabe poet, and the pampered offspring of a rich, powerful family. When faced with the choice of leaving an injured alien creature to fend for itself in the wilds of a strange world, he makes decisions that force him to contend with his own failings–but also help him discover his mission in life.
Official Safety Notice for Poetry-Averse Readers: There are no actual poems in this book.
Before launching (pun intended) into this installment, I have to note some disappointing news from the European Space Agencyâs ATV-5 mission. Due to a power issue, they decided not to do the shallow-angle reentry, which would require the vehicle to be in flight for an extra week or more after deploying from the ISS. Instead, it completed its mission in a more typical reentry maneuver, earlier today (Sunday, Feb. 15th ). Oh, well, the astronauts saved the new NASA monitoring instrument aboard the ISS for use in a future mission. But it was not like we had anticipated. To cope with the loss, enjoy some NASA imagery from the reentry of Japanâs Hayabusa spacecraft.
Terry Fong with NASA Social Team:Â Blue Skies Over the Roverscape
Once weâre done with the agency-wide event of the morning, we find our way to the dazzling outdoors and distribute ourselves between a shuttle van and a minivan with our NASA team and a service-dog-in-training, and weâre off to the Roverscape.
Welcome to the Roverscape
Iâm figuring weâll get a few canned presentations about the rovers that roam that dirt lot, climbing its artificial hills and avoiding its alignements of obstacle-rocks. And Iâm psyched for that. At Amesâ 75th-anniversary Open House, it was a crowd-fighting challenge to catch a glimpse of the rover patrolling on the other side of the barbed-wire-topped fence, subject to remote-control by a NASA roboteer hiding in plain sight under a pop-up tent in the parking lot.
But no. Itâs not a presentation in the parking lot.
On arrival, our NASA Social Team quickly demonstrates thinking, writing, photographing, and connecting.
Now, presentations are nice. But the thing is, if youâre at a NASA Social, you feel like you have to be tweeting and posting the whole time and itâs been pretty thoroughly proven that there is no such thing as multi-tasking. Which means while youâre tweeting and posting youâre missing stuff. Some folks handle that by simply recording presentationsâyou know, like the Real Media do. My strategy is to free-type notes, but thatâs pretty dependent on having mad touch-typing skills. In any case, you donât actually get much chance to interact with the people youâre there to learn from. Plus, for the presenters, gawd, there is nothing more tedious than being dragged away from your work to give a presentation to a bunch of people who seem to be playing video games and are not prepared to ask you questions.
So today the Ames Media Relations Gang are trying out a new idea.
The Elevator Pitch for The Elevator Pitch System, Featuring Today’s Reverse Photo Op
They have rounded up a bevy of NASA engineers & scientists associated with seven different project groups. Each group has chosen a representative to give a three-minute âelevator pitchâ. That would be either a) the one person who wasnât there when the rep was chosen or b) a team leader who actually likes talking to groups. Then the social-media herd will be set free to scatter among the projects that have sparked their interest.
This is an experiment that works well on several levels. First, the quick-posting tweeters get snippets of video of the pitch presentations & those are up on YouTube in nanosecs. Second, at first, the attendees naturally focus on projects that interest them the most. Third, because everyoneâs free to wander, attendees also wander over to chat with folks whose topics werenât as appealing at first. That means people discover new things. And theyâre more likely to get excited about new discoveries. Fourth, because it becomes nearly a one-to-one discussion format, questions are livelier, connections are made, and, fundamentally, everyone has a better time.
The sole downside is, for an old-school note-taker like me, itâs tough to shoot photos & video, listen, ask sensible questions, and get notes written down. Gives you some respect for the professional media, eh, what? I’m envying that old-style team of reporter + photographer.
I tried to chat with every group. Very nearly made it, too. So, with rough notes supported by follow-up research, my photos, and the power of memoryâŚ
Target #1: Big Giant Roverbots!
First off, I headed right for Terry Fong and the K-REX robot that was actively surveying the Roverscape. Strangely, no one else was chatting with him yet. Maybe they were scared off by his position as Director of the Intelligent Robotics Group, aka King of the Roverscape. But, seriously, Terry Fong is one the most personable robotics experts you can talk to, and others quickly joined me. It was quickly evident that what people wanted were photos of the rover, so he suggested good shooting angles, led small groups close enough for the rover to demonstrate its detection-and-avoidance behavior, and (near the end of the event) asked his crew to go to RC mode for a bit so the rover wouldnât trundle away so determinedly.
Howdy, Prospector Bot K-REX
Where Be the Water?
The current design mission for the K-REX (which is the upsized younger sibling of the workhorse K-10 robot platform) is developing prospecting tools and algorithms. For survey missions, the rover can use a variety of tools from ground-penetrating radar to its 3-D GigaPan camera. But the hot topic of the moment is seeking water ice under the surface, for Lunar and Mars missions. But how do you âseeâ underground water? Robots, not being prone to faith-based data acquisition (or confidence tricks), arenât good at dowsing. But water contains hydrogen, and each hydrogen nucleus (i.e., a single proton) is just the right size for interacting with a neutron in a measurable way. If you fire neutrons into the ground, theyâll penetrate about a meter, while bouncing around among the component atoms. Eventually, some will bounce back out of the surface. Ones that have only hit large, heavy atoms will be flying at close to their original velocity. But the neutrons that have struck hydrogen atoms will be slowed down significantly. The HYDRA neutron spectroscope detects the relative fraction of slowed-down neutrons and reports high hydrogen concentrations. Lots of hydrogen almost certainly means H2O. The team recently took their rover on a practice mission to search for water in the Mohave desert.
Will K-REX find water under the pebble patch?
One factor they are teaching the robots to work around is the varied character of the surface of the ground, so at the Roverscape, there are test patches of gravel, smooth pebbles, sand, and even shale rocks with smooth surfaces and jagged edges.
Couldn’t resist snagging some video of the rover at work:
Target #2: Makers of the Three (or More) Rules of Flying Robots
At the far end of the row of tents were a couple of guys with, sadly, no active robots to play with. And no one hanging around asking them questions. So, ever happy to avoid a crowd, I left Terry and made a bee line for their display. And discovered the team working to protect us all from wild mobs of flying robots clogging our skies. No, seriously, have you not worried whatâs up with drones these days? Anyone can pick one up on Amazon and start zooming about. There have already been legal cases with âpeeping tomâ drones. And towns arguing about whether or not to legalize shooting down drones above, say, your ranch property. More prosaically, but even more seriously, a drone wandering into airspace populated with passenger airplanes poses serious safety issues. Back in the early days of airplanes, there were similar issues of privacy, rights of transit, and safety.
In his State of NASA address, Charles Bolden trotted out the NASA aero mantra, âNASA is with you when you flyâ. Did you know that on top of cool aero hardware, NASA has been involved in air traffic control & collision avoidance? Now itâs time for UAV traffic controls. In big words, weâre talking: Unmanned Aerial System (UAS) Traffic Management (UTM). This mission involves devising both regulations and technology, because UAVâs need to be smart enough to “know” the rules and to recognize and avoid âforbiddenâ space.
The timeline is short, as the drones are already out thereâwith lots of useful and fun applications but just as many problematic situationsâso the plan is to have essential systems for safe airspace in place within five years. The proposed solution space incorporates static elements (âgeofencingâ to tag keep-out zones) and drone smarts (to detect geofences and manage routing) to build, by stages, a comprehensive system allowing for autonomous operations which maintain secure areas and safe travel.
I only wish theyâd been able to have a live drone to play with and illustrate their points. Because, you know, objects in flight.
Target #3:Â The One I Missed, But Oh, Well, Didya Know…?
The guys next door had a huge UAV on their table, but, well, it was popular. I never did get to talk to them about it. Luckily Tokiwa Smith (@Tokiwana–follow her on Twitter, ok?) tweeted a good photo, so I was able to ID that fierce flyer as FrankenEye, a hybrid creation built largely by a group of student interns using parts from the NASA Dragon Eye UAVâs and their own 3-D printed parts.
It’s FrankenEye: A project student interns got to work on! (Courtesy of NASA)
So, this is a good place to mention that NASA has a tremendous internship program. The robotics programs alone at Ames pull in a dozen or more interns every summer. There are openings for liberal-arts students as well as engineers & scientists. And there are year-round internships as well. The best place to get connected with NASA internships all around the country is a single website, OSSI. There are spots for high-schoolers, undergraduates, grad students, and postdocs, all with one application. However, if you (or a student you know) are in commute distance of any NASA site, check their website for a local internship. For example, at Ames there is the Education Associates Program (supported by funding from USRA)
Target #4:Â Innovative Bots Based On Baby Toys. Seriously.
Next up: the tensegrity bots, a NASA research project which has involved university students and professors from Ghent University to UC-Berkeley to Case Western Reserve. We got our introduction from Vitas SunSpiral, a Stanford-trained innovator whose company is a contractor for the IRG. Yes–one way to work “for NASA” is to work for a company that works with NASA.
Meet the Tensegrity Team
These folks are thinking so far outside the box that there isnât any box left. Theyâre most fascinated by designing structures with great flexibility, analogous to our own flexible spines and spring-loaded tendons and joints. For their inspiration, theyâve turned to the toy universe: remember those springy rattles or balls made of sticks and elastics? At the Open House, Iâd seen the large prototype that theyâre sharing at this event as well as a prototype Berkeley students had built using LEGO Mindstorms. (SunSpiral told me that excited kids at the Open House partly disassembled the LEGO version.) Theyâve even dubbed this design a âSuper Ball Botâ, reflecting the nature of the device is to be âbouncyâ in a flexibility sense (and it also works as a pun on the robotics event âBot Ballâ, though I’m not sure that’s intentional). The Ball Bot moves by adjusting tension in cables connecting the rods in response to dynamic pressure signals transmitted through this physical network. The result is a slow rolling peregrination. Theoretically, this device is its own safety net: it could roll to the edge of a cliff, drop down, and land safely. Eventually, a payload can be added, suspended in the middle of the âballâ and protected by the springy structure of its un-legs.
Hereâs a fun video the team posted a while back of their Super Ball Bot in development, concluding with a demo run right here at the Roverscape:
Target #5:Â Making Robots Take Charge of Their Own Health
OK, there were people nearby showing off tiny satellites, but I needed a big-robot fix again. The guys from the âHealth and Prognosticsâ group were displaying an older-style roverbot with a laptop perched on top of it.
“Health and Prognostics for Optimal Mission Success”  What? Huh?
Whatâs this all about? Health? Is this a bot that helps keep people healthy? I can tell from some of my fellow NASA Socialistas that this is the first-line guess, because that’s how they tag the first photos they tweet.
But, well, no. The âHealthâ under consideration here is the deviceâs own health. For this prototype, the robot assesses the status of its battery packs and then has to decide if itâs up to completing the mission itâs been assigned: driving an assigned path and returning to base. It may need to eliminate some waypoints to safely complete at least the most critical stops on its route and skip the lower-priority stops. Consider that an autonomous survey rover on the Moon or Mars must be able to get itself back to its charging station and still make the cost of its construction and deployment worth the investment.  The laptop on this robot is displaying its “thoughts” as it assesses its assigned route and redesigns that route in response to having one of its battery units disconnected in a recent experimental expedition around the streets right near the Roverscape.
But, wait, thereâs more! To do this job well takes more than an instantaneous measure of how the batteries are doing. This crew has tested batteries to build a system which predicts battery status in the course of the missionâthatâs the âPrognosticsâ in the heading. And that’s also information that is already set to be applied in batteries for electric cars–because this robot uses the same batteries.
It’s unfortunate that the nomenclature leads to a natural confusion here. This is a new field in systems engineering, one that truly sounds like something to do with medicine: Integrated Systems Health Management, or ISHM. I’d’ve picked a different word than “health”, but systems engineers have used that term for so long, it would have been hard to change. In any case, what’s important (and, analogous to biological health) is that it’s all about maintaining systems, and in this context a âdiagnosisâ isnât determining the cause of a rash but more like asking a smart device, like, say, the starship Enterprise, to give itself a check-up, that is: ârun diagnostics.â This has applications in any area with multiple components with failure potential. Here, weâre seeing it applied to an exploration rover system.
Target #6: Synchronized Position Hold, Engage, Reorient, Experimental Satellites
OK, as I plunge over the 2,000-word line, check out those little cubes that Astronaut Scott Kelly is playing with here. I only got to look around the shoulders of others talking to the SPHERES crew, but I got the gist just fine.
Astronaut Kelly juggles SPHERES (Courtesy of NASA)
First of all, theyâre not cubes, theyâre SPHERES. Yes, clearly the acronym was assembled to be cute. But the job of these babies is cool: they are flying ISS helper bots designed to be used as test beds for small satellite designs which include satellites which can work together to perform tasks in space. Theyâve been under constant development since their first flight in 2006. The original-style SPHERES in this photo aren’t really being juggled, they’re navigating within the ISS using echolocation, using fixed-position ultrasound transmitters in the ISS to establish their location and relative positions. The most recent versions are âSmartSPHERESâ equipped with smartphones to communicate rapidly and enable image-taking and provide potential for vision-based navigation.
The resemblance of the SPHERES bots to the âremoteâ droids in the Start Wars franchise is no accident: the original SPHERES were designed by MIT students in response to a challenge from their professor to build him one of those droids. Since then, the SPHERES have continued to be influenced by students, as students have been able to âflyâ by writing programs for SPHERES to execute.
An interesting recent series of experiments involved using a pair of SPHERES to cooperatively rotate a canister of fluid to study the way fluids slosh in microgravity. This is not just an academic exercise. Sloshing behavior affects the way fuel behaves during spacecraft maneuvers. Hereâs a little NASA video of one sloshing experiment (And YouTube will happily point you to more like this.):Â Â
Target #7: Teeny-Tiny Satellites
I could see others moving towards the exit (and some groups packing up their displays), but I squeezed in a quick conversation with one of the CubeSat team members. What the heckâs a CubeSat, did I hear you say? Well, CubeSat is a modular design for a nanosatellite (i.e., a really small satellite). Each CubeSat is composed of a specific number of same-sized cubical “units”. Oh, and though the SPHERES bots look like cubes, a CubeSat âunitâ is actually meant to be cubical: nominally 10x10x10 cm (though if you nit-pick, the specs come out closer to 10x10x11cm).  A CubeSat is assembled as 1 or 2 or 3 such âunitsâ, with 6-unit and 12-unit cubesats in the works. Look at it this way: a 3U CubeSat is a bit smaller than a 12-pack of soda…roughly the size of a standard roll of paper towels. The beauty of the small and modular design is that it opens up satellite-building to students, small businesses, and even hobbyists(though not everyone will score a launch ride with NASA).
You donât launch a CubeSat from Earth. You launch it from space, by hitching a ride up to the ISS (or further) and having it slung from there to its desired orbit. When Orion runs its test flight to the Moon and back in 2017, itâs hoped that a few CubeSats will be able to hitch a ride and be launched from the orbit of the moon, for placement further from Earth. For instance, solar physicists would love to see an array of little satellites spread out around the sun, so they could see the activity over the entire solar surface at one time.
My captive researcher was was happy to talk but eager to get going as well, because she’s involved in an important test scheduled for “very soon”.
TechEdSat-3 (a 3U CubeSat) was the first test of an Exo-Brake.                          TES-4 is coming down in February 2015
Weâd like to be able to send small payloads to Earth. So far, the final parachute drop has been tested. The ability to communicate with the microsat during transit, using the the Iridium satellite network (yep, the smartphone network) for rapid interactive data handling has had testing, and we know how to pop the device out from the ISS. The exo-brake is a parachute designed for use in the low-density upper reaches of the atmosphere to steer the payload on the right course until regular parachutes can be deployed. The upcoming test is the deployment and descent of TES-4, a CubeSat project involving San Jose State University students. They’ll be testing the latest exo-brake and applying the Iridium communications system.
And then, finally, the call came for us all to exit the Roverscape. I walked backward and took the time for one last photo of K-REX before scrambling back aboard our vans for the ride back to the Exploration Center.
In this activity, the most importantidea is to explore and experiment with models and games to understand how a cometâs tail behaves as the comet hurtles around the sun. The key concept is that the cometâs tail is being pushed away from the sun by the ionizing radiation, solar wind and even the light itself blasting out of the sun. This means that when the comet is inbound, approaching the sun, its tail streams behind it, like a horseâs tail. But on the outbound journey, as the comet leaves the sun behind, its tail flies out in front of it. What we hope the participants will take away from these activities is a picture of what a comet looks like as it moves and the knowledge of why it looks that way.
Comet-tail behavior simply makes sense when âexperiencedâ from the cometâs point of view. If by any chance some of these facts are a discovery for you, too, donât feel like you have to keep it a secret that you are learning–have fun with it. A key ingredient in the formula for growing a scientist is that finding out how the universe works is fun. Or, in the words of one physicist profiled in the film Particle Fever: The real answer to âwhy do we do this is . . . because itâs cool.â)
Keep in mind the constraints of your particular situation when assembling your materials and pre-planning the project. For instance, if there arenât enough classroom scissors or if session time is tightly constrained, you can pre-cut the ribbon for the individual comet models into 3-foot lengths. Be aware of opportunities for participants with special needsâfor instance, the comet-running activity does require at least one person to be standing still. In return, that one who just canât stand still could be a pinch-runner. If the group as a whole isnât particularly fast-moving, the ârunningâ game can be done at whatever pace suits the team.  (One can be a âstudentâ at any ageâmost of us middle-aged folks are not exactly speed-demons.) If you’re planning this as a home-schooling project, this is one you’ll want to save for a get-together with other home-schoolers–you need at least three players and it is ever so much more fun with a group.
Stage 1: The Small-Scale Experiment
This description may look long, but that’s just to let you walk through it easily and to share some photos to help. This whole Stage 1 should take about fifteen minutes, tops.  I’ll spare your weary eyes and park the “Stage 2” and “Stage 3” activities in the next posting–but don’t worry, the entire activity fits into a single science session if you can claim an hour’s time to play with.
Before distributing materials, bring out one individual model comet, the sample to be used for the models everyone will take home. Itâs simply an ordinary badminton birdie with long streamers of ribbon tied to it. For now, keep the ribbons bunched up inside the net of the birdie. Explain that the ball at the end of the birdie is the cometâs nucleus, the frilly part can be its atmosphere, or coma, which begins to form as the gas and dust which jets away from the outer layers comet as it warms up.
One Small Comet
Notes: Iâd suggest that you relax and let your sample comet be imperfectâcomets are messy creatures by nature and you donât need that one super-meticulous individual slowing down the whole event by striving to exactly matching a perfect sample. If you have an older, more experienced group of comet enthusiasts to work with, you can interject the extra information about the distinction between the ion and dust tailsâperhaps even represent them by different ribbon colors.On the other hand, if youâre working with anyone between the ages of 5 and 15, and you donât want to deal with distracting snickers and giggles erupting through the group, simply refrain from using the technical term for a birdie. Oh, come on, you know why.
OK, back to it. The ribbon represents those gases and dust particles that make up the cometâs tail(s). Now, if we toss our model across the room, what happens to the streamers tied to it? Right . . . they float out behind. They donât stretch out in front or clump in a bunch around the head of the âbirdieâ. You can demonstrate by trying to throw your comet backwards: hold the tail in front and toss, but the tail will just fall back to the head andâif your throw is a mighty oneâend up in back again..
Now, invite answers to a key question: why does the ribbon float behind? What pushes the tail behind the cone as it flies through the room? With a little nudging, you should get general agreement that it is the air pushing on the lightweight streamers, shoving them behind the âheadâ of our comet.
But now we must turn to a more difficult line of questioning. Pull out playground or soccer ball (a handy model for the sun), and ask one student to stand and hold up your Sun so everyone can see the next portion. Bunch up the cometâs tail in the back of the shuttlecock again, and carry the comet in a âflightâ around the âSunâ. As you move, ask the students to think hard about what happens to the cometâs tail as it whips around the sun.
Start easy. Shake out the streamers, and stretch them out with your free hand. Move the comet towards the sun. Which way should I point the streamers? Everyone will be quick to tell you to pull them backwards, away from the sun. Now, place the comet at its closest approach to the sun, just before it curves back to head into deep space again. âIâm at the Sun now,â you can say, âzooming around the back of it. And moving as fast as Iâll go in this journey. Which way should the streamers point?â
Usually this question generates some disagreement. A reasonable argument would be that you should hold the streamers behind the comet, as it moves, which would mean the cometâs tail would point along a tangent to its orbit around the Sun. (Even if the students are covering tangents in math, please donât interrupt yourself to pause and discuss tangents right now! Use this lesson later to enliven the math session.)
Tail Behind?
Tail In Front?
Tail Sideways?
Some students may suggestâquite logically–that when you are that close, the Sunâs gravity should pull the tail towards it. If the group is large enough, you should also get someone who can argue that the tail should point away from the sunâfor now, it doesnât matter if this is a knowledge-based claim or just a contrarian viewpoint from snarkiest person in the room. Whatever hypotheses are offered, just accept them as proposed solutions and demonstrate what each would look like.
Finally, move to the âoutboundâ portion of your cometâs orbit. âOur comet now flies on away from the sun, perhaps to return in another century or two. Now, which way should the cometâs tail point?â Again, if you have managed to keep a poker face so far, the most popular answer is likely have the tail streaming behind the comet. As before, accept and demonstrate each of the guesses. If students have reasons for their theories, let everyone hear them. Discussing and justifying hypotheses is an integral part of the real scientific process.
If you have access to a blackboard (oh, well, itâs modern times, so, okayokayokay, you can use your smelly whiteboard or that fancy tablet-linked projector), now is the moment to leave off demonstrating with the model and sketch the competing hypotheses for everyone to see. Your picture will look kind of like this. Please remember to Keep It Messy.
Discussing Possible Tail Directions
Have you ever read one of those annoying mystery stories in which the author leaves you in the dark about a critical fact that solves the entire case? Well, here too, we have denied our puzzle-solvers an important clue. So, tell the group itâs time for a change of topic. But actually what weâre doing is rolling out the narrative twist that makes the whole thing so cool.
Here on Earth, it is air that pushes the streamers on our comet model. But how much air is there out in space? (So little that you might as well say âzeroâ!) But without air, why should any comet have a tail at all?
What comes out of the sun? You should hear the following answers: heat, light, maybe even radiation. But has anyone heard of the solar wind? The sun blasts out particles, too? The sun is shooting out plasma, protons and electrons flying through the solar system at thousands of miles per hour. This is the solar wind, which blows through the solar system all the time, at thousands of miles per hour. The particles are tiny, not even as big as atoms, so it is an invisible wind. And like wind, itâs not perfectly even, it gusts and changes from moment to moment as the Sun itself changes.
All of those things we named help to make our comets look the way they do. Consider your audienceâŚ
Explanation #1: You are all correct. All of that stuff blasting out of the sun–light, radiation, heat, and the solar wind–shove all that stuff leaking out of the comet into a tail. And since all that stuff is coming from the sun, the only way the tail can point is away from the sun.
Explanation #2: All of those answers are correct . . . and they all combine to make a cometâs tail. The heat of the sun warms the comet to free the gases and dust. The solar wind blasts the gasesâand the particles in the solar wind also interact with those gases, stripping some of their electrons to make that part of the tail a glowing stream of ionized gas. The radiation from the sun actually can push things, and that pressure is just strong enough to shove those tiny dust particles enough to counteract their tendency to fall towards the sun. And the visible sunlight reflects from the spread-out cloud of dust, making the comet shine in our night sky.
Again, with older/experienced participants, now is the time to clue them in that radiation pressureâthe totally cool idea that sunlight itself exerts pressureâexists because light is electromagnetic radiation and electromagnetic radiation is a wave and a wave [http://physics.info/em-waves/] pushes on the objects it encounters. You may not feel battered and bruised by the TV and radio waves powering through you day and night or be physically bowled over by the sunlight forming a gorgeous rainbow. But: itâs enough to push fine grains of dust. The only sad thing about radiation pressure is itâs not common knowledge yetâitâs been proven since 1873.
To represent these solar forces, we need to make a breeze. For that job, a fan does the trick. When we turn it on, it blasts a healthy âsolarâ wind. (Be sure to experiment in advance with your fan and sample comet–there’s a lot of variation in fan settings.)
Inbound Comet
Hold the comet in the âinboundâ position, with the front of the birdie pointed at the Fan Sun. Yes! We were all correct: the tail points behind the comet as it moves towards the sun.
If the fan is strong enough, you can also use the model to hint at how the length of the cometâs tail changes. Far from the sun, the comet has no tail; far from the fan, our streamers dangle to the floor. A little closer in, a real comet’s tail appears as a pale streak behind it; as you approach your fan, the model’s streamers lift up and begin to flutter weakly behind it. Near the sun, the tail stretches out millions of miles behind a real cometâs head; near the fan, the your streamers stretch their full length.
Now, what about when the comet is heading away from the sun? Which way will the tail be pointing, now that we know about the solar “wind”? Nearly everyone will see, now, that it must point away from the sun.
Outbound Comet
Demonstrate that this works: you point the birdieâs nose away from the fan, turn on the blast, and the streamers flow out over the front of the birdie. The shape of the birdie helps emphasize the incongruity of our expectationâthat the tail goes behindâwith the reality: the solar forces push the tail.
If the class has patience for one more test, add the third question: what happens when the comet is rounding the far side of the sun, and is pointed âsidewaysâ? Hold the comet model perpendicular to the flow of the fan.
Comet At Perihelion
Let everyone see how the tail sweeps out to the side of the comet. It always points away from the sun, no matter what direction the comet is pointing.