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natural infirmity of the flesh, which I will explain to you in a

one direction along the latter from the beginning to the end of

`That,' said a very young man, making spasmodic efforts to

relight his cigar over the lamp; `that . . . very clear indeed.'

`Now, it is very remarkable that this is so extensively

fourth, Time. There is, however, a tendency to draw an unreal

`That,' said a very young man, making spasmodic efforts to

ALONG IT. But some foolish people have got hold of the wrong

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misconception.'

`Is not that rather a large thing to expect us to begin upon?'

incandescent lights in the lilies of silver caught the bubbles

patents, embraced and caressed us rather than submitted to be sat

he put it to us in this way--marking the points with a lean

said Filby, an argumentative person with red hair.

NIL, has no real existence. They taught you that? Neither has

INSTANTANEOUS cube exist?'

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`Nor, having only length, breadth, and thickness, can a cube

have a real existence.'

have Length, Breadth, Thickness, and--Duration. But through a

relight his cigar over the lamp; `that . . . very clear indeed.'

Dimension do not know they mean it. It is only another way of

side of that idea. You have all heard what they have to say

Length, Breadth, and Thickness, and is always definable by

angles to the other three?--and have even tried to construct a

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or two ideas that are almost universally accepted. The geometry,

ground for it. You will soon admit as much as I need from you.

You know of course that a mathematical line, a line of thickness

`There I object,' said Filby. `Of course a solid body may

exist. All real things--'

`So most people think. But wait a moment. Can an

dimensions, three which we call the three planes of Space, and a

relight his cigar over the lamp; `that . . . very clear indeed.'

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Dimension do not know they mean it. It is only another way of

THE THREE DIMENSIONS OF SPACE EXCEPT THAT OUR CONSCIOUSNESS MOVES

is spoken of as having three dimensions, which one may call

Length, Breadth, and Thickness, and is always definable by

we can represent a figure of a three-dimensional solid, and

similarly they think that by models of thee dimensions they could

thought roams gracefully free of the trammels of precision. And

this new paradox (as we thought it:) and his fecundity.

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`Can a cube that does not last for any time at all, have a real

moment, we incline to overlook this fact. There are really four

distinction between the former three dimensions and the latter,

relight his cigar over the lamp; `that . . . very clear indeed.'

Fourth Dimension, though some people who talk about the Fourth

Dimension do not know they mean it. It is only another way of

thought roams gracefully free of the trammels of precision. And

he put it to us in this way--marking the points with a lean

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accession of cheerfulness. `Really this is what is meant by the

`_I_ have not,' said the Provincial Mayor.

is spoken of as having three dimensions, which one may call

Four-Dimension geometry. Professor Simon Newcomb was expounding

`I think so,' murmured the Provincial Mayor; and, knitting his

brows, he lapsed into an introspective state, his lips moving as

The Time Traveller (for so it will be convenient to speak of

shone and twinkled, and his usually pale face was flushed and

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`There I object,' said Filby. `Of course a solid body may

natural infirmity of the flesh, which I will explain to you in a

moment, we incline to overlook this fact. There are really four

one direction along the latter from the beginning to the end of

looking at Time. THERE IS NO DIFFERENCE BETWEEN TIME AND ANY OF

reference to three planes, each at right angles to the others.

dimensions particularly--why not another direction at right

the thing. See?'

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`Is not that rather a large thing to expect us to begin upon?'

NIL, has no real existence. They taught you that? Neither has

`Nor, having only length, breadth, and thickness, can a cube

have a real existence.'

Filby became pensive. `Clearly,' the Time Traveller proceeded,

one direction along the latter from the beginning to the end of

`That,' said a very young man, making spasmodic efforts to

that flashed and passed in our glasses. Our chairs, being his

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say that we cannot move about in Time. For instance, if I am

length of Time, any more than a savage or an animal has of

`Oh, THIS,' began Filby, `is all--'

`Possibly not,' said the Time Traveller. `But now you begin to

`But I have experimental verification,' said the Time

Man. `Our ancestors had no great tolerance for anachronisms.'

Little-go. The German scholars have improved Greek so much.'

`To discover a society,' said I, `erected on a strictly

DAY IN REVIEW

 

DAY IN REVIEW Holiday Asteroid Imaged with NASA Radar The December 2018 close approach by the large, near-Earth asteroid 2003 SD220 has provided astronomers an outstanding opportunity to obtain detailed radar images of the surface and shape of the object and to improve the understanding of its orbit. The asteroid will fly safely past Earth on Saturday, Dec. 22, at a distance of about 1.8 million miles (2.9 million kilometers). This will be the asteroid's closest approach in more than 400 years and the closest until 2070, when the asteroid will safely approach Earth slightly closer. The radar images reveal an asteroid with a length of at least one mile (1.6 kilometers) and a shape similar to that of the exposed portion of a hippopotamus wading in a river. They were obtained Dec. 15-17 by coordinating the observations with NASA's 230-foot (70-meter) antenna at the Goldstone Deep Space Communications Complex in California, the National Science Foundation's 330-foot (100-meter) Green Bank Telescope in West Virginia and the Arecibo Observatory's 1,000-foot (305-meter) antenna in Puerto Rico. The Green Bank Telescope was the receiver for the powerful microwave signals transmitted by either Goldstone or the NASA-funded Arecibo planetary radar in what is known as a "bistatic radar configuration." Using one telescope to transmit and another to receive can yield considerably more detail than would one telescope, and it is an invaluable technique to obtain radar images of closely approaching, slowly rotating asteroids like this one. "The radar images achieve an unprecedented level of detail and are comparable to those obtained from a spacecraft flyby," said Lance Benner of the Jet Propulsion Laboratory in Pasadena, California, and the scientist leading the observations from Goldstone. "The most conspicuous surface feature is a prominent ridge that appears to wrap partway around the asteroid near one end. The ridge extends about 330 feet [100 meters] above the surrounding terrain. Numerous small bright spots are visible in the data and may be reflections from boulders. The images also show a cluster of dark, circular features near the right edge that may be craters." The images confirm what was seen in earlier "light curve" measurements of sunlight reflected from the asteroid and from earlier radar images by Arecibo: 2003 SD220 has an extremely slow rotation period of roughly 12 days. It also has what seems to be a complex rotation somewhat analogous to a poorly thrown football. Known as "non-principal axis" rotation, it is uncommon among near-Earth asteroids, most of which spin about their shortest axis. With resolutions as fine as 12 feet (3.7 meters) per pixel, the detail of these images is 20 times finer than that obtained during the asteroid's previous close approach to Earth three years ago, which was at a greater distance. The new radar data will provide important constraints on the density distribution of the asteroid's interior - information that is available on very few near-Earth asteroids. "This year, with our knowledge about 2003 SD220's slow rotation, we were able to plan out a great sequence of radar images using the largest single-dish radio telescopes in the nation," said Patrick Taylor, senior scientist with Universities Space Research Association (USRA) at the Lunar and Planetary Institute (LPI) in Houston. "The new details we've uncovered, all the way down to 2003 SD220's geology, will let us reconstruct its shape and rotation state, as was done with Bennu, target of the OSIRIS-REx mission," said Edgard Rivera-Valentín, USRA scientist at LPI. "Detailed shape reconstruction lets us better understand how these small bodies formed and evolved over time." Patrick Taylor led the bistatic radar observations with Green Bank Observatory, home of the Green Bank Telescope, the world's largest fully steerable radio telescope. Rivera-Valentín will be leading the shape reconstruction of 2003 SD220 and led the Arecibo Observatory observations. Asteroid 2003 SD220 was discovered on Sept. 29, 2003, by astronomers at the Lowell Observatory Near-Earth-Object Search (LONEOS) in Flagstaff, Arizona - an early Near-Earth Object (NEO) survey project supported by NASA that is no longer in operation. It is classified as being a "potentially hazardous asteroid" because of its size and close approaches to Earth's orbit. However, these radar measurements further refine the understanding of 2003 SD220's orbit, confirming that it does not pose a future impact threat to Earth. The Arecibo, Goldstone and USRA planetary radar projects are funded through NASA's Near-Earth Object Observations Program within the Planetary Defense Coordination Office(PDCO), which manages the Agency's Planetary Defense Program. The Arecibo Observatory is a facility of the National Science Foundation operated under cooperative agreement by the University of Central Florida, Yang Enterprises and Universidad Metropolitana. GBO is a facility of the National Science Foundation, operated under a cooperative agreement by Associated Universities, Inc. JPL hosts the Center for Near-Earth Object Studies (CNEOS) for NASA's Near-Earth Object Observations Program. More information about CNEOS, asteroids and near-Earth objects can be found at: https://cneos.jpl.nasa.gov https://www.jpl.nasa.gov/asteroidwatch For more information about NASA's Planetary Defense Coordination Office, visit: https://www.nasa.gov/planetarydefense More information about the National Science Foundation's Arecibo Observatory can be found at: http://www.naic.edu/ao/ For asteroid and comet news and updates, follow AsteroidWatch on Twitter: twitter.com/AsteroidWatch

 

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ground for it. You will soon admit as much as I need from you.

`Nor, having only length, breadth, and thickness, can a cube

INSTANTANEOUS cube exist?'

`any real body must have extension in FOUR directions: it must

because it happens that our consciousness moves intermittently in

`That,' said a very young man, making spasmodic efforts to

relight his cigar over the lamp; `that . . . very clear indeed.'

overlooked,' continued the Time Traveller, with a slight

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incandescent lights in the lilies of silver caught the bubbles

this new paradox (as we thought it:) and his fecundity.

said Filby, an argumentative person with red hair.

`That is all right,' said the Psychologist.

`Nor, having only length, breadth, and thickness, can a cube

him) was expounding a recondite matter to us. His grey eyes

incandescent lights in the lilies of silver caught the bubbles

`You must follow me carefully. I shall have to controvert one

DAY IN REVIEW

 

DAY IN REVIEW The Coolest Experiment in the Universe What's the coldest place you can think of? Temperatures on a winter day in Antarctica dip as low as -120ºF (-85ºC). On the dark side of the Moon, they hit -280ºF (-173ºC). But inside NASA's Cold Atom Laboratory on the International Space Station, scientists are creating something even colder. The Cold Atom Lab (CAL) is the first facility in orbit to produce clouds of "ultracold" atoms, which can reach a fraction of a degree above absolute zero: -459ºF (-273ºC), the absolute coldest temperature that matter can reach. Nothing in nature is known to hit the temperatures achieved in laboratories like CAL, which means the orbiting facility is regularly the coldest known spot in the universe. Seven months after its May 21, 2018, launch to the space station from NASA's Wallops Flight Facility in Virginia, CAL is producing ultracold atoms daily. Five teams of scientists will carry out experiments on CAL during its first year, and three experiments are already underway. Why cool atoms to such an extreme low? Room-temperature atoms typically zip around like hyperactive hummingbirds, but ultracold atoms move much slower than even a snail. Specifics vary, but ultracold atoms can be more than 200,000 times slower than room-temperature atoms. This opens up new ways to study atoms as well as new ways to use them for investigations of other physical phenomena. CAL's primary science objective is to conduct fundamental physics research - to try to understand the workings of nature at the most fundamental levels. "With CAL we're starting to get a really thorough understanding of how the atoms behave in microgravity, how to manipulate them, how the system is different than the ones we use on Earth," said Rob Thompson, a cold atom physicist at NASA's Jet Propulsion Laboratory in Pasadena, California, and the mission scientist for CAL. "This is all knowledge that is going to build a foundation for what I hope is a long future of cold atom science in space." Laboratories on Earth can produce ultracold atoms, but on the ground, gravity pulls on the chilled atom clouds and they fall quickly, giving scientists only fractions of a second to observe them. Magnetic fields can be used to "trap" the atoms and hold them still, but that restricts their natural movement. In microgravity, the cold atom clouds float for much longer, giving scientists an extended view of their behavior. The process to create the cold atom clouds starts with lasers that begin to lower the temperature by slowing the atoms down. Radio waves cut away the warmest members of the group, further lowering the average temperature. Finally, the atoms are released from a magnetic trap and allowed to expand. This causes a drop in pressure that, in turn, naturally causes another drop in the cloud's temperature (the same phenomenon that causes a can of compressed air to feel cold after use). In space, the cloud has longer to expand and thus reach even lower temperatures than what can be achieved on Earth - down to about one ten billionth of a degree above absolute zero, perhaps even lower. Ultracold atom facilities on Earth typically occupy an entire room, and in most, the hardware is left exposed so that scientists can adjust the apparatus if need be. Building a cold atom laboratory for space posed several design challenges, some of which change the fundamental nature of these facilities. First, there was the matter of size: CAL flew to the station in two pieces - a metal box a little larger than a minifridge and a second one about the size of a carry-on suitcase. Second, CAL was designed to be operated remotely from Earth, so it was built as a fully enclosed facility. CAL also features a number of technologies that have never been flown in space before, such as specialized vacuum cells that contain the atoms, which have to be sealed so tightly that almost no stray atoms can leak in. The lab needed to be able to withstand the shaking of launch and extreme forces experienced during the flight to the space station. It took the teams several years to develop unique hardware that could meet the precise needs for cooling atoms in space. "Several parts of the system required redesigning, and some parts broke in ways we'd never seen before," said Robert Shotwell, chief engineer for JPL's Astronomy, Physics and Space Technology Directorate and CAL project manager. "The facility had to be completely torn apart and reassembled three times." All the hard work and problem solving since the mission's inception in 2012 turned the CAL team's vision into reality this past May. CAL team members talked via live video with astronauts Ricky Arnold and Drew Feustel aboard the International Space Station for the installation of the Cold Atom Laboratory, the second ultracold atom facility ever operated in space, the first to reach Earth orbit and the first to remain in space for more than a few minutes. Along the way, CAL has also met the minimum requirements NASA set to deem the mission a success and is providing a unique tool for probing nature's mysteries. Designed and built at JPL, CAL is sponsored by the International Space Station Program at NASA's Johnson Space Center in Houston, and the Space Life and Physical Sciences Research and Applications (SLPSRA) Division of NASA's Human Exploration and Operations Mission Directorate at NASA Headquarters in Washington.

 

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NASA's InSight Places First Instrument on Mars

 

DAY IN REVIEW NASA's InSight Places First Instrument on Mars NASA's InSight lander has deployed its first instrument onto the surface of Mars, completing a major mission milestone. New images from the lander show the seismometer on the ground, its copper-colored covering faintly illuminated in the Martian dusk. It looks as if all is calm and all is bright for InSight, heading into the end of the year. "InSight's timetable of activities on Mars has gone better than we hoped," said InSight Project Manager Tom Hoffman, who is based at NASA's Jet Propulsion Laboratory in Pasadena, California. "Getting the seismometer safely on the ground is an awesome Christmas present." The InSight team has been working carefully toward deploying its two dedicated science instruments onto Martian soil since landing on Mars on Nov. 26. Meanwhile, the Rotation and Interior Structure Experiment (RISE), which does not have its own separate instrument, has already begun using InSight's radio connection with Earth to collect preliminary data on the planet's core. Not enough time has elapsed for scientists to deduce what they want to know - scientists estimate they might have some results starting in about a year. To deploy the seismometer (also known as the Seismic Experiment for Interior Structure, or SEIS) and the heat probe (also known as the Heat Flow and Physical Properties Probe, or HP3), engineers first had to verify the robotic arm that picks up and places InSight's instruments onto the Martian surface was working properly. Engineers tested the commands for the lander, making sure a model in the test bed at JPL deployed the instruments exactly as intended. Scientists also had to analyze images of the Martian terrain around the lander to figure out the best places to deploy the instruments. On Tuesday, Dec. 18, InSight engineers sent up the commands to the spacecraft. On Wednesday, Dec. 19, the seismometer was gently placed onto the ground directly in front of the lander, about as far away as the arm can reach - 5.367 feet, or 1.636 meters, away). "Seismometer deployment is as important as landing InSight on Mars," said InSight Principal Investigator Bruce Banerdt, also based at JPL. "The seismometer is the highest-priority instrument on InSight: We need it in order to complete about three-quarters of our science objectives." The seismometer allows scientists to peer into the Martian interior by studying ground motion - also known as marsquakes. Each marsquake acts as a kind of flashbulb that illuminates the structure of the planet's interior. By analyzing how seismic waves pass through the layers of the planet, scientists can deduce the depth and composition of these layers. "Having the seismometer on the ground is like holding a phone up to your ear," said Philippe Lognonné, principal investigator of SEIS from Institut de Physique du Globe de Paris (IPGP) and Paris Diderot University. "We're thrilled that we're now in the best position to listen to all the seismic waves from below Mars' surface and from its deep interior." In the coming days, the InSight team will work on leveling the seismometer, which is sitting on ground that is tilted 2 to 3 degrees. The first seismometer science data should begin to flow back to Earth after the seismometer is in the right position. But engineers and scientists at JPL, the French national space agency Centre National d'Études Spatiales (CNES) and other institutions affiliated with the SEIS team will need several additional weeks to make sure the returned data are as clear as possible. For one thing, they will check and possibly adjust the seismometer's long, wire-lined tether to minimize noise that could travel along it to the seismometer. Then, in early January, engineers expect to command the robotic arm to place the Wind and Thermal Shield over the seismometer to stabilize the environment around the sensors. Assuming that there are no unexpected issues, the InSight team plans to deploy the heat probe onto the Martian surface by late January. HP3 will be on the east side of the lander's work space, roughly the same distance away from the lander as the seismometer. For now, though, the team is focusing on getting those first bits of seismic data (however noisy) back from the Martian surface. "We look forward to popping some Champagne when we start to get data from InSight's seismometer on the ground," Banerdt added. "I have a bottle ready for the occasion." JPL manages InSight for NASA's Science Mission Directorate in Washington. InSight is part of NASA's Discovery Program, which is managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. Lockheed Martin Space in Denver built the InSight spacecraft, including its cruise stage and lander, and supports spacecraft operations for the mission. A number of European partners, including CNES and the German Aerospace Center (DLR), support the InSight mission. CNES provided SEIS to NASA, with the principal investigator at IPGP. Significant contributions for SEIS came from IPGP, the Max Planck Institute for Solar System Research in Germany, the Swiss Institute of Technology in Switzerland, Imperial College and Oxford University in the United Kingdom, and JPL. DLR provided the Heat Flow and Physical Properties Package (HP3) instrument, with significant contributions from the Space Research Center of the Polish Academy of Sciences and Astronika in Poland. Spain's Centro de Astrobiología supplied the wind sensors. For more information about InSight, visit: https://mars.nasa.gov/insight

 

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incandescent lights in the lilies of silver caught the bubbles

this new paradox (as we thought it:) and his fecundity.

ground for it. You will soon admit as much as I need from you.

have a real existence.'

`There I object,' said Filby. `Of course a solid body may

The Time Traveller (for so it will be convenient to speak of

him) was expounding a recondite matter to us. His grey eyes

incandescent lights in the lilies of silver caught the bubbles

DAY IN REVIEW

 

DAY IN REVIEW NASA Satellites Spot Young Star in Growth Spurt An adolescent star in the midst of a dramatic growth phase has been observed with the help of two NASA space telescopes. › Read the full story InSight Engineers Have Made a Martian Rock Garden Reconstructing Mars here on Earth lets them practice setting down the lander's science instruments. › Read the full story

 

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Meet JPL Interns: From Struggling in School to 'Killing It at NASA,' a VR Dream Come True Until she discovered game development, Michelle Vo's daydreams were a problem. She couldn't focus in her computer science classes. Her grades were dipping. She wondered whether she was cut out to be a programmer or for school at all. So she took a break to make something just for fun, a self-help game. And help her, it did. Now focusing on virtual and augmented reality, Vo is back at school, studying not just computer science, but also cognitive science, linguistics and digital humanities. It's a lot, but to create a virtual world, she says one has to first understand how people navigate the real one. This summer, at NASA's Jet Propulsion Laboratory, the UCLA student applied her talents to VR and AR experiences that help scientists explore a totally different world, Mars. While Vo's tendency to daydream hasn't gone away, she now knows how to use the distractions for good; she turns them into VR inspiration. Read her story   Explore these related links for students and educators: NASA/JPL Internships - Explore internship opportunities at NASA's Jet Propulsion Laboratory and apply today! Get started Meet JPL Interns - Read stories from interns pushing the boundaries of space exploration and science at the leading center for robotic exploration of the solar system. Read more Computer Science Lessons - Explore a collection of standards-aligned computer science lessons for grades 3-12 and featuring NASA missions and science. Check it out

 

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Teachable Moment: Voyager 2 Reaches Interstellar Space The Voyager 2 spacecraft, launched in 1977, has reached interstellar space, a region beyond the heliosphere – the protective bubble of particles and magnetic fields created by the Sun – where the only other human-made object is its twin, Voyager 1. The achievement means new opportunities for scientists to study this mysterious region. And for educators, it's a chance to get students exploring the scale and anatomy of our solar system, plus the engineering and math required for such an epic journey. In the latest Teachable Moment from NASA/JPL Edu, education specialist Ota Lutz explains how the Voyager mission took advantage of a rare planetary alignment to embark on a journey no spacecraft had before – or has since. Plus, how do we know Voyager 2 has entered interstellar space and what can we expect for the future of the mission? Click the button below to find out more and explore related lessons for educators and activities for students. Read the Blog   Explore the entire Teachable Moments collection and related lessons on our new landing page! Related Activities for Educators and Students Use these standards-aligned lessons and related activities to get students doing math and science with a real-world (and space!) connection. Solar System Bead Activity (Grades 1-6) - Students create a scale model of the solar system using beads and string. Get started Catching a Whisper From Space (Grades 4-12) - Students kinesthetically model the mathematics of how NASA communicates with spacecraft. Get started Solar System Scroll (Grades 5-8) - Students predict the scale of our solar system and the distance between planets, then check their answers using fractions. Get started *NEW* Modeling the Structure of the Solar System (Grades 6-12) - Students will learn about the structure of the solar system and be able to identify analogous regions in a dynamic, 2-D kitchen-sink model. Get started Hear Here: A 'Pi in the Sky' Math Challenge (Grades 10-12) - Students use the mathematical constant pi to determine what fraction of a signal from Voyager 1 – the most distant spacecraft – reaches Earth. Get started

 

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---

NIL, has no real existence. They taught you that? Neither has

a mathematical plane. These things are mere abstractions.'

`That is all right,' said the Psychologist.

that flashed and passed in our glasses. Our chairs, being his

thought roams gracefully free of the trammels of precision. And

for instance, they taught you at school is founded on a

ground for it. You will soon admit as much as I need from you.

NIL, has no real existence. They taught you that? Neither has

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`That,' said a very young man, making spasmodic efforts to

Dimension do not know they mean it. It is only another way of

`It is simply this. That Space, as our mathematicians have it,

Four-Dimension geometry. Professor Simon Newcomb was expounding

represent one of four--if they could master the perspective of

`I think so,' murmured the Provincial Mayor; and, knitting his

are curious. For instance, here is a portrait of a man at eight

years old, another at fifteen, another at seventeen, another at

DAY IN REVIEW

 

DAY IN REVIEW Engineering Fun and Function at JPL Invention Challenge Whether via bungee cord, half-inch chain, servo motors, torsion springs, electronics or just plain gravity, 20 middle- and high-school student teams used a range of equipment to compete in this year's JPL Invention Challenge at NASA's Jet Propulsion Laboratory in Pasadena, California. The teams - mainly from Southern California but including ones from as far away as Ethiopia and Guam - took part in the "Upright Pipe Contest" on Friday, Dec. 14. The objective was to get a 24-inch length of two-inch PVC pipe from a horizontal position to an upright position on a platform using whatever device they could come up with, instructions not included. "I give them nothing," said Paul MacNeal, a JPL mechanical systems engineer and the contest's organizer. "I give them a blank piece of paper. The entry fee is $0, and the typical devices we see here cost between $25 to $100. The idea is to not be a financial burden to any school. This has a low entry fee, and it still encourages the creative juices to get going." While the rules required contestants to get the pipe upright in under 60 seconds, the top three teams didn't even need two. The winning student team, from Oakwood High School in North Hollywood, got the pipe upright and steady on the platform in just 1.37 seconds. The speedy time brought oohs and aahs from the crowd, and even surprised the Oakwood team members, who had been tinkering with their device just minutes before taking the stage. "We decided to use a drill as the motor to pull," said junior Seth Kleinberg. "It came from a device we built a couple of years ago (for a previous Invention Challenge)." Oakwood's time in the November regional competition clocked in at 11 seconds, but after seeing some of the times of the competing schools, the team regrouped, upped the drill speed and added components to the device - including a ketchup packet. "Today we went through at least five or six different iterations," said junior Tyler Brown, but after seeing one of the first teams get near two seconds, they knew what they had to. "We were like, okay we gotta go fast," said freshman Maggie Brown. Second place went to Hamilton High School's team named We Made It, whose time of 1.59 seconds was a marked improvement over the groups' showing in last year's challenge. "Last year, we were all excited to compete and had our machine tested the morning of and ready to go," said senior Ethan Layne. "We put it on the trailer to go to JPL, and we thought we had it strapped down, but apparently not secure enough, and it blew off the trailer on the freeway." The team went back to look for it but found no sign of the lost machine. So this year, they were just glad to have "made it." "It's definitely nice, after working so hard last year and having it basically just disappear, coming back this year and do as well as we did," Layne said. In third place, Los Angeles High School's Wildcats team fused function with art, constructing a device that utilized torsion springs and surgical tubing to erect the pipe in 1.67 seconds, and they decorated it with a cat, flower and a giant butterfly. "Most of our team are ninth-graders, and seven out of nine team members are girls," Dante Madali, a math and computer science teacher. "I always encourage them to be artistic and creative. To apply the creativity. Of course, the challenge is the first priority. But if they still have time, then I encourage them to be creative about their work." What makes the Invention Challenge unique is the involvement of JPLers, who compete alongside the students but in a separate division. MacNeal sees that as invaluable in changing the perspective of engineering as a profession. "The students get to see professional engineers competing and having fun at the same time. The basic overall theme here is engineering is fun, and we're trying to bring some levity into all of the schoolwork these guys have. This is something that's hands-on. It's an experience, not a grade." This year, the top JPLers were Alan Devault, with a time of 2.38 seconds, Ria Dawar at 4 seconds, and Richard Goldstein at 4.65 seconds. Caltech in Pasadena, California, manages JPL for NASA.

 

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