Tag Archives: NASA

Astronomy’s Wonder Woman

2017 saw a major uptick in interest in “Wonder Woman” as the result of the movie where Gal Gadot played the role of the Amazonian princess.  Others remember the character as portrayed by Lynda Carter in the late 1970s TV series.  However, 2017 also saw the first American appearance by a real-life astronomical wonder woman – Pranvera Hyseni.

Pranvera Hyseni 4

Pranvera Hyseni at the 2018 Northeast Astronomy Forum (NEAF)


While both versions of the fictional Wonder Woman came from an exotic island, Pran (as she prefers to be called) came from an unusual location as well – a small part of what was once Yugoslavia and is now known as the Republic of Kosovo.  Kosovo came into existence as the result of the wars that ensued as Yugoslavia disintegrated.  In the final part of the conflict, Kosovo broke off from Serbia and became independent in 1998.  However, Kosovo is only recognized by 115 countries, including the United States, which is held in very high regard over there.  American flags can be seen in government offices and pictures of Bill Clinton (U.S. President at the time Kosovo became independent) are a frequent sight.

Pran was born on April 25th, 1995 in town of Vushtrri.  The first step in her destined path took place in 1999.  Kosovo was in the path of a total solar eclipse.  The news was received in the country with panic and much superstition.  However, Pran’s parents took no stock in that nonsense.  Instead, at the appointed time, they got a large bucket and filled it with water.  Then they and their children, including 4-year-old Pran, looked at the Sun’s reflection on the surface of the water.  This is a surprisingly effective technique when done correctly as the water surface reflects a fraction of the Sun’s visible light and virtually none of the non-visible wavelengths, enabling safe viewing.

The next significant event, astronomically, came in 2011.  Pran had been on Facebook for a time and one of her friends in Macedonia learned of her interest in the night sky.  So he decided to give her a small telescope.  While the 1999 solar eclipse set up the fuse, this telescope lit it.  Pran was so impressed by how much she could see in the night sky using the telescope that she decided to devote herself to astronomy.

Then, a major problem arose.  Pran soon discovered that there were no astronomy books, magazines, software, or websites in Albanian, the language of Kosovo (Kosovo has close ties to Albania).  Rather than give up or sit around and wait for astronomy stuff to appear in Albanian, Pran tackled the problem by teaching herself English.  This feat is not to be underestimated as not many people who come to the United States permanently from other countries are willing, able, or want to do it, instead preferring businesses and the government learn their language.  Pran soon wound up with a very good command of the language for a self-taught non-native speaker.

This opened up a world of astronomical information, allowing Pran to learn about all aspects of space science as well as developing contacts in the astronomical community, both amateur and professional, throughout the world.

Pran soon decided that it would be in the best interests of Kosovo and its population to spread astronomical knowledge and interest.  As a result, she created Astronomy Outreach Kosovo (AOK), the first astronomy club in the whole country.  The primary activity of AOK is hosting outreach events at in towns, cities, and various schools.  Due to this work, Pran was asked by the Ministry of Education to develop an astronomy curriculum to be used in schools throughout Kosovo, which she did.  She also trained schoolteachers in the use of a number of telescopes donated by the German outfit GIZ (Deutsche Gesellschaft für Internationale Zusammenarbeit, GmbH)

Pran’s fame soon spread throughout Kosovo and the astronomical community.  Because of this, she became quite a traveler, representing Kosovo at conferences in locations as diverse as Milan, Italy, Zurich, Switzerland, and even the International SUNday event in Australia.  While on those trips, Pran toured numerous astronomical sites and built up her contacts in the astronomical community – something that would pay off in the near future.  But her greatest trip was yet to come – a visit to the United States.  This came about when Robert Reeves of the Texas Star Party (TSP) invited her to speak at the event.
But it almost didn’t happen.  Despite Kosovo’s good relations with the United States and the fact that Pran’s abilities were well-known to many in the space science community, she was initially denied a visa for her trip (mainly due to the influence of someone with bad hair and supposedly small hands).  But, complaints from the astronomical community as well as many of her social network contacts prompted the State Department to see the light and give Pran her visa.  The trip was on.

Despite a near-total lack of coverage by the mainstream American media, she wound up getting invitations from all over the country.  Joe Bergeron of the Grand Canyon Star Party invited her to his event.  While in Arizona, she got to see many attractions as well as some of the famous observatories there, including Lowell Observatory.  Later she toured part of New England, visiting Rhode Island (no, she didn’t waste her time trying to find Quahog – she knew it wasn’t real) and Brown University, as well as MIT and the Harvard Astrophysical Observatory in Massachusetts.  There were a number of speaking engagements, including one at Spacefest in June at Tucson, Arizona.  At this event was that Pran got to meet almost all the surviving Apollo astronauts except for Buzz Aldrin, who was out of the country at the time.

Also on this trip she got to visit some of NASA’s spaceflight centers, Kennedy in Florida and Marshall in Alabama.  While at those facilities, Pran was granted very high levels of access, including a visit to the roof of the Vehicular Assembly Building (VAB) at Kennedy.

During trip, Pran received numerous gifts from astronomical organizations, clubs, and admirers.  These ranged from telescopes to meteorites, including a lunar and Martian one.  This raised questions how they would be shipped back home to Kosovo as well as how to handle customs.  But Pran solved that problem and now has the largest meteorite collection in Kosovo as well as having increased the number of telescopes in the country.

It was fitting that Pran, whose interest in astronomy began with a solar eclipse, got to witness the totality of the August 21st solar eclipse.  After some discussion at the Kosovo Embassy in New York, she got an extension on her trip to allow this.  In another stroke of good fortune, a fan who happened to own a plane came forward, allowing her to fly to Springfield, Tennessee, near the path of totality, which she witnessed using much better equipment than the bucket of water she used back in 1999.

In one of their few moves that even AAI member and noted IAU critic Laurel Kornfeld would agree with, the International Astronomical Union (IAU) named an asteroid in Pran’s honor.  It is 45687 Pranverahyseni and, like 9967 Amastrinc (AAI’s asteroid), is a small (about 13 kilometers in diameter) body in the main asteroid belt.  Pranverahyseni can be observed through very large amateur instruments from dark locations or via astroimaging.

These days, it seems every major success inspires a sequel, Pran’s American tour was no exception.  This time, it is a six-month tour (let’s hope she never goes on a three-hour one – we all know how that ended up for one group of people).  It started in April and the first major stop was NEAF (North East Astronomy Forum) at Rockland County College in Suffern, New York.  She was a speaker at the event, but she had to share the stage with two other astronomers in a group that was billed as “Celestron’s Young Astronomers”.  She deserved her own billing, something I discussed with Stephen Ramsden of the Charlie Bates Solar Astronomy Project (one of Pran’s best American friends) and we both agree on this.  But as a consolation, Pran was the best prepared speaker of the three (she never used index cards, doing it all from memory) and the only one who got a standing ovation.

The most recent project AOK has embarked on is setting up, with the cooperation of the government, the first ever observatory in Kosovo.  At NEAF, Corey Lee, the president of Celestron announced that his company would be donating a 14-inch telescope with associated hardware to this project.  I heard this from Pran herself very shortly after she was informed of this.

The ongoing tour is expected to visit many astronomical locations all over the United States, including some of the more noteworthy events such as ALCON (the Astronomical League Convention, not the Weird Al Yankovic fan event of the same name).  One major highlight already was that Pran finally got to observe her asteroid through a telescope at the Texas Star Party.  Those who want to keep up with the tour can follow Pran and AOK on Facebook.

And Pran has an even bigger and longer trip to the United States planned in the future.  Due to the lack of advanced astronomical education opportunities in Kosovo, Pran is hoping to get a PhD in planetary science at the University of Arizona.   So we will probably be hearing more about Pran for some time to come.

Though Pranvera Hyseni is no Gal Gadot or Lynda Carter, as far as space science goes, she is definitely a wonder woman.

(Trivia note: Lynda Carter does know about Pran and is impressed.)


The Traffic Jam They Don’t Talk About


This coming Monday, August 21st, is the Great American Eclipse, the first total solar eclipse to pass through a large part of the United States since 1979 and the first coast-to-coast American total solar eclipse since the Woodrow Wilson administration.

The narrow zone of totality crosses from Oregon to South Carolina.  And many eclipse observers who can afford it and can get the time off will travel to the area.  As predicted, the airlines have jacked up their fares substantially.  Other observers will drive to the path of totality.  Even if they get to the path ahead of time, in most cases, they will have to drive quite a bit more to dodge cloud cover.


The interstates may not be the only superhighway clogged with eclipse traffic.

If lots of eclipse observers do this simultaneously, there will be huge traffic jams on the highways reminiscent of what happens with those mandatory evacuations that they have for coastal storms.  But, aside from the photo illustration, this post will concentrate on the other traffic jam – the one nobody talks about as well as how effective a possible remedy would actually be.


It has been known for quite some time that NASA-TV will be having quite a bit of coverage of this event.  Sounds like a good idea.  But due to the fact that very few, if any, cable services and only one satellite network carry NASA-TV (the reasons for this will be the topic of a future post), this means that NASA-TV is pretty much an Internet-only TV channel.  This works under normal conditions, but is a major problem for events like the eclipse.  For those who are a bit unfamiliar with how the Internet works, NASA-TV uses web servers to put their content online.  And these servers can only handle up to a certain number of people hooking up to them to view the content.  As the number of people viewing increases, the performance of the server in delivering the content deteriorates.  If the number gets high enough, it malfunctions.  Historically, this has happened to NASA quite often during major events.  Not surprisingly since their computer hardware, like everything else, was put in by the lowest bidder on a government contract.  While this isn’t too bad for rockets as the engineers at those contractors work with physical things and they generally do a reasonably good job building rockets, when it comes to computers, those people are a different breed.  In physical engineering, it is common practice to build things a bit stronger than they actually need to be so there is some reserve capacity and also to cope with the unexpected.  However, when it comes to web servers, computer people tend to go with the minimum capacity for the job.  It would be better if they followed what I call “The Roebling Rule” (named in honor of the Roebling company that built the Brooklyn Bridge).  They insisted that, if a part on the bridge was supposed to support one ton, it had to be able to support six to ten tons.  As a result, the Brooklyn Bridge is a sturdy structure that is still around today.  Another company built a similar bridge, the Williamsburg Bridge, but was told to keep the budget down.  Due to the corners that were cut, the bridge had to be replaced years later at enormous cost.

The other online eclipse coverage sites also suffer from the small server problem.  The Exploratorium in San Francisco has done eclipse coverage in the past and has had problems.  Compounding things are their rather amateurish production skills.

On top of all this, those people who do not have broadband Internet or have metered bandwidth (only so many gigabytes per month) will have problems accessing the online coverage.

If only there was a way to get video coverage of the eclipse that didn’t depend on bandwidth and server issues and can handle any number of viewers… wait, such a technology does exist and we have had it for years… television!

While this eclipse is well suited for television coverage as it does pass through quite a few cities and towns in the United States, the response from the mainstream (referred to hereafter as “lamestream” to use a term coined by Jim Kurdyla of Facebook fame) media has been extremely underwhelming.  The remainder of this post will discuss the TV eclipse options known to me as of the moment of this writing.  Some of this information may be subject to change.  Here goes…

One would expect that the lamestream broadcast networks (ABC, CBS, Fox, NBC, and PBS) would have an interest in this.  Sadly, that interest appears to be rather small.

ABC: This network was probably the first national broadcast network to announce eclipse coverage.  The show will feature Sara Haines, Rebecca Jarvis, T.J. Holmes, Ginger Zee, Matt Gutman, David Kerley, Nick Watt, Adrienne Bankert, and Eva Pilgrim.  I suppose if you crammed all their astronomical knowledge together, you might get something equivalent to an entry-level amateur astronomer.  There are reports that some affiliates will go above and beyond this.

CBS: The national network seems to be taking the wimpy way out on this one.  They will only be having coverage online.  Some affiliates, mainly those along the path of totality, may take matters into their own hands.  One reason given by some wags is that CBS doesn’t want to preempt their daytime programming at eclipse time.  This consists of two daytime dramas (News flash: Daytime drama is a dying genre) and “The Talk”  Guess they don’t want to preempt “The Talk” or it might get Les Moonves in trouble with the wife at home.

Fox: Unknown.  They might decide to leave it up to affiliates.

NBC: Evidently realizing what ABC is doing, NBC will be doing a one-hour national show as well.  It will be hosted by Al Roker, Lester Holt, and Dylan Dreyer.  Not ideal, but it is better than CBS and Fox.  Wonder how these astronomical lightweights will manage?

PBS: Some PBS stations (not all) will be carrying a one hour program titled “Total Eclipse Live”.  I have no further details on it.  But, later that evening, PBS will show its talent for after-the-fact coverage of astronomical events with a special episode of “Nova” that will incorporate some footage from that day’s eclipse.  This is a rather rapid turnaround since it usually takes a few weeks at least for the “Nova” crew to put together something on an astronomical event.  As with the other networks, some affiliates might do something on their own.

Eclipse coverage is a lot like the Emmy awards in the fact that cable channels trounce the broadcast ones.

The Science Channel: This network is going to cover the eclipse completely in a program called “The Great American Eclipse”.  And in a departure from what the commercial broadcasters are doing, this program will be hosted by actual astronomers.  And, if that isn’t enough, there will be a recap show that evening.

The Weather Channel: The one channel on just about every cable system is doing quite a bit of coverage on eclipse day.  Their special “Total Solar Eclipse” will feature coverage from all over the eclipse track as well as from a ship off South Carolina.  And they are prepared.  In the event of bad weather at any location, NASA-TV coverage will be used as backup.

Of course, this information may be subject to change between now and the eclipse.  So, if you can’t see totality or are clouded out, keep an eye on the TV listings.  But, if you are where the eclipse is visible, don’t forget to see it for yourself (using proper safety methods).

Has Science Been Fair to the Fair Sex?

I know Women’s History Month is almost over, but the points raised in this post are still very valid.

The film, “Hidden Figures” has been in the news quite a bit recently.  It is a dramatization of the real-life story of Katherine Johnson, Dorothy Vaughan, and Mary Jackson, three African-American women who did heavy-duty mathematical calculations at NASA in the 1960s. Even though computers did exist in those days, they were the size of large refrigerators and had far less computing power than even the lowly Commodore VIC-20 (a nearly 40-year old personal computer).  Thus, humans were still needed to do the mathematical work that the early manned space missions required.

However, those women had several things going against them.  One was that they were women.  Another was that they were African-American.  On top of that, NASA facilities were mostly in the South.  In the case of Kennedy Space Center (though it wasn’t called that until after the assassination of John F. Kennedy), it was due to considerations of orbital mechanics.  As for the other NASA centers, it was to placate influential politicians.  As a result, segregation was in full force at the time.  Johnson and her team worked in a separate office, had a separate lunch area, and were treated as second class people by most at NASA.  However, John Glenn judged them by their work and treated them well.  In fact, he demanded that Johnson personally handle the computations for his orbital flight.

This got me to look back at other women in the history of science.  It turns out that the snubs and treatment that Johnson and her team got were not new.

One famous example was Caroline Herschel.  Due to her growth being stunted in childhood by disease, she was quite short.  On top of that, her parents told her that she would amount to nothing.  However, she helped out her brother, William Herschel, the greatest observational astronomer of his era.  Eventually, she learned enough that she became an observer herself, discovering several deep sky objects as well as a few comets.  Despite her superb training, her contributions were largely forgotten.  Even among modern astronomers, she is little known.

Another case was Maria Mitchell.  She was born into a Quaker family and, since the Quakers believed in equal education, she received far better education than most women of that era.  Mitchell developed an interest in astronomy early in life and became one of America’s first professional astronomers and the first female one.  During the 1840s, the King of Denmark gave an annual award to people who discovered comets.  In 1841, Mitchell discovered a comet and was up for the award.  However, there were astronomers who felt that she did not deserve to get it and raised quite a furor over the matter.  Finally, the Danish authorities intervened and Mitchell got her medal.

Jumping forward to the early 20th century, Harvard Observatory hired a number of women to do mathematical work and measurements of images on glass photographic plates.  Much like Katherine Johnson and her team, these women were referred to as “computers”.  Unlike Johnson, these computers earned sweatshop wages.  But, it was far safer than most of the work women got in that era, working in dangerous mills as well as garment manufacturing (anybody recall the Triangle Shirtwaist fire?). One of these women, Henrietta Swan Leavitt was assigned the task of studying stars on glass photographic plates.  Her job was to locate stars in the Magellanic Clouds that varied in brightness.  Doing so, she discovered that one class of stars (what we call Cepheid variables) had a brightness that was proportional to their period (cycle of variability).  This became known as the period-luminosity relationship and laid the foundation for finding distances to nearby galaxies.  Since she was just a lowly computer, her bosses took credit for the discovery.  But the truth eventually won out and the story is well known in astronomical circles today.

I could go on and on with other examples, such as the career of Lise Meitner, who had to contend with sexism as well as the rise of Nazi Germany, the story of how Watson and Crick might have “borrowed” information from a female colleague to aid their discovery of the structure of DNA, but here is a case of how a woman scientist made a discovery, only to have it stolen from her.

In 1968, Jocelyn Bell was working at Cambridge when she made an odd discovery.  When the radio telescope was pointed at a spot in the constellation of Vulpecula, a rapid pulsing signal was detected.  The pulses were very precise, enough that some people thought it was an alien radio beacon.  This idea soon fell by the wayside and it was learned that the object responsible was a pulsar, a rapidly rotating neutron star that emitted radio energy like the beam of a lighthouse.  Once the significance of this became apparent, Anthony Hewish and Martin Ryle, Bell’s bosses, took credit for the discovery.  Though she did win a Michelson Award (along with Anthony Hewish) in 1973, she was totally ignored when the Nobel prize in physics was handed out in 1974 with Hewish and Ryle getting the prize.  Despite protests from other prominent physicists, Bell was denied Nobel recognition.  While the history books got things right in the end, it was too late for Bell to get the prize.  But she was made a Dame by Queen Elizabeth II some years later.

Sometimes, the side of good wins.  In 1979, Voyager 1 passed through by Jupiter and made many observations.  About three days after closest approach, navigation engineers were poring over the images sent back.  This was to refine the position of the spacecraft as well as the orbits of the Galilean moons.  One of those people, a woman by the name of Linda Morabito, noticed something odd in an image of Io.  It appeared that there was a limb of another moon peeking out from behind Io. Instead of jumping to conclusions, Morabito enhanced the image and, probably echoing the thought of Han Solo when he first saw the Death Star, found that was no moon.

converted PNM file

The first image of Io’s volcanism

It was actually the plume from a volcanic eruption on Io, the first display of active volcanism outside Earth.  Morabito was determined to get credit for this find and pushed her case.  Finally, with the mainstream media on her side, she was credited with the find, securing her place in scientific history.

These days, Morabito is involved in advocating for science.  In additon to her personal website, she also maintains a Facebook group, Linda Morabito’s Space Place where she offers commentary on various scientific issues.

So, as Women’s History Month draws to a close, remember the contributions women have made in science and let’s hope for the day when science gives credit where it is due without regard to whether it was a man or a woman who made the discovery.

Orion Oversold?

December 4th is the date set for the first test flight of NASA’s new Orion capsule.  It will be launched into Earth orbit using a Delta IV rocket at about 7:05 AM.  Then, Orion will circle the Earth twice, conduct some test maneuvers, then enter the atmosphere at about 80% of the velocity the capsule would have if it was returning from the Moon.  If the reentry systems work properly, Orion should splash down in the Pacific off the coast of San Diego, California before noon.  Unless it lands like the capsule in “Gravity”, Orion will be bobbing at the surface and picked up by a waiting ship.

NASA has been loudly promoting Orion, claiming that it is the vehicle that will take American astronauts beyond low Earth orbit and to destinations such as the Moon and Mars.  Much ink and many pixels have been used to promote Orion as a truly advanced spacecraft.  But let’s see it for what it is.

I dimly recall back in the early 1970’s there was a proposal to build a larger version of the Apollo-era command module.  The plans were all drawn up for it, then it was decided that there was no need for it.  Orion looks like the resurrection of this project.  Of course, Orion does have some updated technology, such as new heat shield material, far superior computers, nicely decorated interior, and touchscreen panels (like the controls you would find on “Star Trek: The Next Generation” or on an Asgard ship from the “Stargate” franchise, if you prefer).  But don’t be fooled, it is still based on your father’s (or grandfather’s depending on your age) Apollo command module.

Actually, there is something about Orion that is actually inferior to the original Apollo-era vehicle.  The Orion will use a service module that is based on the ESA’s (European Space Agency) Automated Transfer Vehicle (ATV) that has been used to send supplies up to the ISS.  This ATV-derived service module will use solar panels instead of fuel cells to generate electrical power and will certainly have far less powerful engines than the original Apollo-era service module did.

Then, there was a statement made about the Orion by a Russian commentator who pointed out that, for a vessel that is supposed to house a crew for up to three weeks or so, it lacked certain amenities.  While on a short trip to the Moon, that might not be a big deal since the original Apollo astronauts didn’t complain about the lack of a convenience, it could pose a problem for longer trips.

What bothers me is how NASA keeps pushing the idea that Orion will take astronauts to Mars.  It is simply way too small for the job (unless someone manages to develop the technology used to create the sub-light propulsion systems of mainstream science fiction programs).  Even Robert Zubrin (creator of the Mars Direct concept of a reasonably priced program of Mars exploration) and his colleagues and the folks at Mars Direct have put more thought into designing a spacecraft to take people to Mars.

Why has NASA gone so far overboard in promoting Orion?  Probably because that it is about the only idea they have left for manned spaceflight (besides the Space Launch System – SLS – heavy rocket).

Hopefully the test flight of Orion will go well and not wind up exploding, running out of power,  sinking on splashdown, or anything like that.  But do you think that Orion’s “Back to the Future” approach is the way to go or do you think it’s another one of NASA’s ideas that will fall well short of the mark?

What is the Real Cost of Saving Kepler?

Kepler K2 Mission Diagram

Diagram of Kepler’s K2 Mission

In March of 2009, the Kepler mission was launched.  It was placed in an Earth-trailing orbit around the Sun and observed a patch of sky located in the Milky Way near the constellation of Cygnus to look at thousands of stars to detect any dimming that was caused by a planet passing in front of a star.  This mission was by any criterion a great success and racked up an impressive number of discoveries, including the first rocky planets in the habitable zone of a star.

However, in April of 2013, one of the spacecraft’s reaction wheels (powered gyroscopes used to control the pointing of the vehicle) failed.  One had failed earlier, but there were still enough wheels for the mission to continue.  This time was different.  Kepler was placed into a safe mode which allowed it to communicate to Earth.  For the next three months, various strategies were tried to see if the reaction wheel that failed earlier could be restarted.  It was restarted but did not function well.

Then, some on the team had a stroke of brilliance.  After doing the complicated math and computer simulations, they came up with a way to save the mission by using the pressure of solar radiation (a major cause of instability to Kepler) as a means to help keep the spacecraft stable.  NASA liked the idea, known as “K2” (no connection to the extremely dangerous Himalayan mountain of the same designation) and depicted in the above diagram.  So, Kepler was saved, but at what cost?

In terms of dollars and cents, it was a great bargain.  However, when it came to Kepler’s capabilities, it turns out to be an almost Faustian deal.

The great strength of the original Kepler mission was that it kept one well-known section of sky under continuous surveillance.  That way, Kepler would not miss anything that took place.  As a result, Kepler discovered planets of longer periods and was able to observe the three transits required to confirm the discoveries.  The success of this strategy can be seen in the large number of planet discoveries from the mission.

Due to the use of solar radiation pressure as stabilization, Kepler has to be pointed at the ecliptic plane (the plane where the planets of the solar system tend orbit).  That doesn’t sound so bad, but since the Sun appears in the ecliptic plane, Kepler has to move to observe another field about every 83 days so the Sun doesn’t shine into the instrument and burn out the detectors.  Factoring in the time it would take to adjust Kepler each time it moved to one of the eight fields, that yields less than 83 days per field.  So, the concept of continuous surveillance goes right out the window.

Since a “year” for Kepler in its solar orbit is 379 days and only about four and a half fields can be observed in one Kepler “year”, that means quite a bit of time will pass before it returns to a field for further observation.  A lot can happen in that time and a many potential planets will be missed.  Mission scientists naturally downplay this and claim that the increased number of viewing locations will make up for it.  True, there will be some discoveries made from the K2 mission, but they won’t be anywhere near as numerous due to the spotty nature of the observations.  If you are a fan of extrasolar planets, you better get used to most of the new discoveries being hot Jupiters, hot Neptunes, and lava worlds, rather than the more interesting habitable zone planets, because the short duration of observations in each field will favor the planets with really short orbital periods, even with the new policy of requiring only two repeat transits to confirm a planet instead of three.

And this approach of observing lots of area for shorter intervals appears to be the wave of the future in searching for extrasolar planets from space.  If you like the K2 mission, you’ll love the followup mission to Kepler called TESS (Transiting Exoplanet Survey Satellite) which will survey most of the sky while in an eccentric Earth orbit with little time devoted to each field.

You can read the full gory details about K2 here.  Is the new strategy of observing more area in less time worth it for extrasolar planets or should there be a return to more time in less area in the future?