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Kepler Mission Finds 752 Extrasolar Planet Candidates

An anonymous reader lets us know about the initial release of data from the Kepler spacecraft, launched in the spring of 2009, which has been hunting extrasolar planets. The instrument has found 752 candidates to examine in its first 43 days of operation. This is exciting news, because even if only half of the possibilities pan out as exoplanets (as the Kepler team expects) the results would still almost double the count of known planets. And some of the new ones could be Earth-sized, or not too much larger. Controversy has erupted however because NASA has decided to allow the Kepler team to withhold 400 of the best candidates for its own examination, releasing about 350 others to the worldwide community. The reasons for this are complicated and the New York Times does a good job of digging into the issue of proprietary vs. public data. Nature.com first reported two months ago on the decision to hold back some of the data.

30 of 103 comments (clear)

  1. Data Archives by eldavojohn · · Score: 5, Informative
    Here is the notice they are releasing potential extrasolar planetary data and the press release saying that it's data on 156,000 stars. You can search the data or just download the tarfiles via anonymous FTP:

    ftp archive.stsci.edu
    cd /pub/kepler/lightcurves/tarfiles

    If you do a search there appears to be anywhere from half to two thirds of the data that are marked as proprietary data which their search help gives a brief explanation of:

    Clicking on entries in this column will mark the entry for retrieval. To mark all entries, click one of the buttons labelled 'Mark All','Mark public', or 'Mark Proprietary'. (Unmarking all entries can be done the same way using the appropriate button.) For missions with proprietary data, the mark button element will have a yellow background and a '@' symbol to indicate data sets not yet public.

    I think the majority of those that are unreleased are simply Q2 data or later since this data is just from the first 42 days of the mission. What's available as the tar file appears to be all Q0 and Q1 data so I'm not certain if the 400 that are 'censored' are included in that or not. If they are withheld it seems odd that the announcement, release notes and README file make no mention of this. Still, we're talking 12+ GB of compressed data here.

    Overall and despite the reported censoring of the best candidates, I personally applaud their transparency here that surpasses anything another government related organization (or even scientific field for that matter) exhibits. Alright, maybe CERN or the LHC will be as transparent or more transparent but this is still pretty impressive.

    --
    My work here is dung.
    1. Re:Data Archives by DJRumpy · · Score: 2, Interesting

      Who payed for Kepler? This isn't Schrodinger's Cat. Information can most certainly be 'owned', traded, or sold. Got Spam? Exactly...

      If these guys won't release the data due to concerns that they won't spot the next 'earth-like planet' and claim the 'credit', then there are probably thousands who would eagerly take that chance. At this point, it comes down to someone simply evaluating the data. The 'discovery' has already been made in a manner of speaking, so now it's turned into some sort of ugly 'wheres Waldo'.

    2. Re:Data Archives by DerekLyons · · Score: 4, Informative

      If you do a search there appears to be anywhere from half to two thirds of the data that are marked as proprietary data

      Overall and despite the reported censoring of the best candidates

      It's long been NASA policy that the PI and his team (the guys who've spent the last ___ years or decades bringing the instrument to fruition) get first crack at the data, which usually amounts to six months exclusive access. After that, the data is publicly released.
       
      So it's neither censorship nor proprietary data in the usual senses either term are used in, so please be a bit careful in choosing your verbiage and making implications.

    3. Re:Data Archives by toby34a · · Score: 4, Informative

      Mod this guy up. NASA will release the data in its entire form eventually, and in perpetuity once they get the first paper out of it. This is the same whenever NASA puts up a new satellite - they get the data, analyze it, publish the initial results, and release the entire record, for free, for anyone in the world to download. So there's an embargo period- it's not long, and it's not that significant. They are better at putting out free data (as is NOAA/NWS) then anyone else in the world- the Europeans and Chinese are exceptionally hard at getting data out of without paying for it or knowing someone behind the scenes. Anyone can download a GOES image or MODIS image from NOAA or NASA in the span of minutes to hours. It takes days (or months) to get SEVIRI or MERRA imagery from EUMETSAT.

    4. Re:Data Archives by Bacon+Bits · · Score: 3, Insightful

      Exactly. It's only fair that the people who worked on the project get the chance to be credited with at least a few of the important discoveries.

      Want first crack at the data? Launch your own satellite. Otherwise get in line.

      --
      The road to tyranny has always been paved with claims of necessity.
    5. Re:Data Archives by BitZtream · · Score: 2, Informative

      Lets get one thing straight.

      IT IS MY SATELLITE.

      My tax money (and yours) paid for it and the salaries of everyone who worked on it.

      On that note however, I still think its just fine and dandy that they get the first shot at looking at the data they busted their asses to get, especially since the reality of it is, they probably know at least 100 times more about what they are looking at than anyone on /.

      I'm fine standing at the back of the line since I only paid a few cents to the project (like everyone else) and I'm highly unlikely to discover anything anyway. Let them get the credit they deserve, but make no mistake, I already paid dues for accessing the data. Without me (my tax money), it wouldn't exist.

      --
      Persistent Volume manager for Kubernetes - https://github.com/dwimsey/openshift-pvmanager
  2. Drake equation? by dkleinsc · · Score: 3, Interesting

    I'm wondering if all this effort in discovering exoplanets is getting us any closer to a better estimate of the fp (fraction of stars that have planets) factor of the Drake Equation. Obviously, a complete survey of the sky isn't practical, and we know that some exoplanets are going to be undetectable, and it might also be skewed by the scientifically minded looking closer at stars likely to have planets rather than stars unlikely to have planets, but at the same time we have a lot more to go on than we once did.

    --
    I am officially gone from /. Long live http://www.soylentnews.com/
    1. Re:Drake equation? by Kjella · · Score: 2, Interesting

      Well, from what I've understood it'll always be easier to see planets that are huge and either a short distance from star or in a very elliptical orbit, so they'll be overrepresented. Also those in plane with the star, but that goes for small and big planets alike. But when we get a little more data, we can probably get good estimates by taking say the closest 1000 ly of stars (the most distant detected is already at 21500 ly) where we can see both small and large planets, longer orbital times etc. to get a representative sample than trying to extrapolate from all the planets found.

      --
      Live today, because you never know what tomorrow brings
    2. Re:Drake equation? by Anonymous Coward · · Score: 2, Interesting

      Kepler is designed in such a way to have a similar likelihood to see a large planet and a small planet. It is based on transit based system . ESA has a good article describing it http://www.esa.int/esaSC/SEMYZF9YFDD_index_0.html

      but the chance of a large and a small planet passing in front of a sun is approximately the same and when that condition happen kepler has the sensitivity to pick up the difference for many of the close planets. So it should be able to determine fp with more accuracy

    3. Re:Drake equation? by Zocalo · · Score: 2, Interesting

      Possibly, but I don't think it's going to help much, at least not just yet. The problem is twofold; firstly the exoplanets found so far are generally inhospitable to all but the most exotic imaginings of what might constitute extra-terrestrial life. Secondly, the articles I have seen tend to imply that planets are much more plentiful than has been thought, and this is a big problem, because even the post pessimistic attempts at the Drake equation have the galaxy teaming with life. If planets are even more plentiful than previously assumed, then that should equate to even more life, so where is everybody? The answer seems to be that either one or more of the assumptions we are making about values in the Drake equation is wildly out of touch with reality or there is another factor to the equation that we are overlooking.

      --
      UNIX? They're not even circumcised! Savages!
    4. Re:Drake equation? by sznupi · · Score: 2, Interesting

      It's approximately the same (in the given time of observations) only assuming comparable orbital periods, isn't it?

      In our system that would overrepresent terrestrial planets. Who knows what is the norm... (most extrasolar planets being gas giants orbiting close to their star might be itself a selection bias)

      --
      One that hath name thou can not otter
    5. Re:Drake equation? by Kjella · · Score: 2, Insightful

      At least some of the estimates I've seen seem to have a very high degree of "if we could, we would". But look at us, we haven't been to the Moon in decades, we probably could go to Mars at some huge expense, but we don't. Now scale this up to interstellar distances and you're looking at an absurdly expensive project that quite probably never will pay off, and at least with current technology take many thousands of years to do. Of course that time is a blink of an eye on the universal timescale, but as a barrier to actually doing it that's huge. And even a self-sustained colony wouldn't be scaled to launch crafts of its own, perhaps if you had terraforming technology so that in time that colony could become another "earth" they could but that's also stuff of serious science fiction. Otherwise it'll never evolve past the home star and a small circle of colonies.

      --
      Live today, because you never know what tomorrow brings
    6. Re:Drake equation? by farble1670 · · Score: 2, Interesting

      yes but that's the thing about kepler,

      it's aim is to discover h-congruous planets. kepler doesn't detect the planet, it detects the planet's transit across it's sun. it can find earth-sized planets in this way. they can estimate the size based on change in apparent magnitude.

      also, based on the frequency of transit (kepler makes long-term observations of candidate planets) it can estimate the distance from the star, and based on the type / size of the star, it can figure out if the planet is in the "habitable zone" for C-based life, as we understand it anyway.

    7. Re:Drake equation? by Chris+Burke · · Score: 4, Insightful

      Secondly, the articles I have seen tend to imply that planets are much more plentiful than has been thought, and this is a big problem, because even the post pessimistic attempts at the Drake equation have the galaxy teaming with life. If planets are even more plentiful than previously assumed, then that should equate to even more life, so where is everybody?

      The galaxy could be teeming with life, it could even be teeming with intelligent life, and yet we could be completely oblivious to the fact.

      This is only a shocking and serious problem if you had assumed that intelligent life would inevitably discover a way around the speed of light.

      Think about it -- we're are only just able to identify the existence of planets around other stars, not even ones like ours that are at a comfortable distance from their stars, and still only in a tiny area of the sky. And we can do little more than identify their period and their mass. Actual spectroscopy of exoplanets is at an even more infant stage than simply finding them. The rocky planets we already know of could be teeming with life, and we just have no way of knowing yet!

      So the only way we'd know about some advanced civilization is if they were spamming the galaxy with transmissions and probes, and the wave front/probe passed us during the narrow window during which we've been looking. And look at us -- the amount of radiation we as a civilization are blasting out into space has vastly reduced as we've figured out how to be more efficient, or replaced broadcast transmission with fiber-optic cables and so on. So the brief period of time in which we've been looking would have to coincide (accounting for distance) with the brief period in which they were broadcasting enough for us to see. And they have to have been close enough for us to be able to see. And we have to have noticed.

      Hell, how do we know that an alien probe, launched thousands of years ago, didn't pass through our solar system just last year?

      I'm not about to get all despondent about the Drake Equation based on the logic of "Well why haven't we seen alien life already?" Let's wait until we can do enough research on our own to get even the sketchiest idea of how common life itself is before we start getting worried about why aliens haven't said hello, okay?

      --

      The enemies of Democracy are
    8. Re:Drake equation? by Plekto · · Score: 2, Interesting

      The answer seems to be that either one or more of the assumptions we are making about values in the Drake equation is wildly out of touch with reality or there is another factor to the equation that we are overlooking.
      *****
      Several of the typical assumptions in the Drake equation *are* off by a couple of orders of magnitude. My astronomy class back in the early 90s decided to figure out a more reasonable number and only concentrate on planets that could support any form of life (only variable we were really looking for was liquid water) The estimate came out to something like 1/50 stars. I felt it was closer to 1/20 myself if you added moons and so on.

      But that's a big difference compared to "Hi, how are you?" Almost all of it would be microbes and simple plants and so on.

      We plugged that back into the equation and added in the fact that we would be looking for a slice of 200 years, tops, for radio waves(the assumption was that they would figure out FTL/point-to-point communication * by then), and then a 25% chance that they didn't blow themselves up/have a disaster/etc before they got there, we came up with 4 or 5 in our galaxy. Anything more advanced would not be using means to communicate that we can detect or will avoid us if they are ever aware of us, that is. Given the raw materials in the outer solar system (Ort cloud, Kupier Belt, etc) it's likely that most civilizations also wouldn't leave their solar system for many thousands of years except to maybe send a probe to check something out. And only if it's close by. (if you scaled the galaxy to the size of your living room wall, you'd hardly see 50-100LY as a movement at all, which is as far as most conventional/slower than light exploration is likely to happen)

      *Note - this was more than a decade before theories about quantum entanglement and micro-wormholes became well-known, but we felt it was reasonable that any advanced civilization would have a super-sized version of the internet even if they couldn't ever physically travel faster than light.

    9. Re:Drake equation? by BitZtream · · Score: 2, Insightful

      The reality is ... our radiation is useless for others to detect us.

      By the time any signal from our planet that we generate gets to any other known planet, its completely undetectable in the background noise, even if you KNOW the signal is there and exactly what you're looking for, you still couldn't find it.

      --
      Persistent Volume manager for Kubernetes - https://github.com/dwimsey/openshift-pvmanager
  3. NASA is just acting on orders: by tverbeek · · Score: 5, Funny

    "All these worlds are yours, except for this list of 400. Attempt no landings there."

    --
    http://alternatives.rzero.com/
  4. Re:Earth to slashdotters by Pojut · · Score: 5, Interesting

    NASA is indeed a scientific organization. I know a decent number of people who have/currently do work for NASA, due to my step father being an electrical engineer for Orbital (formerly Fairchild) (he helped design some of the tools used in the earlier Hubble Repair Missions. He no longer works there [he is, for all intents and purposes, retired at this point], but he worked for Fairchild/Orbital for a little over 20 years.) They are a dedicated, unbelievably intelligent group of people, who are amongst the most passionate people in the whole country.

    The people in charge of their funding, those are the folks that are political. The people who actually work for NASA are just trying to utilize what little freedom they have been given.

  5. well its not very sensitive data by circletimessquare · · Score: 2, Interesting

    if china or al qaeda get information about where exoplanets are, its not like bin laden is going to go there to hide. there's little anyone can do about exoplanets right now except look at them, and it will be this way for generations to come

    but if the scientific research were about nanotechnology or particle physics, meanwhile, i would expect everything to be censored, as it should be, even if funded with tax dollars

    --
    intellectual property law is philosophically incoherent. it is your moral duty to ignore it or sabotage it
  6. Re:Candidates? by sznupi · · Score: 2, Interesting

    The IAU definition of a planet that you speak of is about Solar System only. Why would you be annoyed about status of some rock anyway? (except for trying to maintain consistency of course, which the IAU tries to do)

    Besides, there will be quite a mess with extrasolar systems too; what is a giant planet and what is a sub-brown dwarf? Or what about moons of gas giants that will turn out to be larger than Earth?

    --
    One that hath name thou can not otter
  7. Approximately 50% of your base... by moondawg14 · · Score: 3, Funny

    ... are belong to us.

  8. Planet Pantent Trolls by Goffee71 · · Score: 2, Funny

    Pretty sure you can't patent a celestial body. Also pretty sure that some idiot will try.

    --
    If he's the Walrus then can I be a penguin please?
  9. Re:Candidates? by MozeeToby · · Score: 2, Interesting

    Besides, there will be quite a mess with extrasolar systems too; what is a giant planet and what is a sub-brown dwarf? Or what about moons of gas giants that will turn out to be larger than Earth?

    A sub-brown giant is a body with less than 13 Jupiter masses that doesn't orbit a start or stellar remnant. If it goes around the star and is below that size limit it is a planet. A moon the size of the earth is still a moon by definition, size alone doesn't determine what is or isn't a planet; if it orbits a planet it is a moon. An as yet unanswered question would be "What about two planet sized bodies that orbit around a common center of gravity?"

  10. Re:Woooow! oh my.... by Convector · · Score: 3, Informative

    If by "cancel", you mean "increase the budget of", then yes. It's only Constellation that's getting canceled. Science is getting a boost.

  11. Standard procedure by goodmanj · · Score: 5, Insightful

    This is standard operating procedure for major spacecraft missions. Cassini and Galileo missions to Saturn and Jupiter did the same thing. Kepler's choice of the word "proprietary" is unfortunate: Cassini and Galileo used "embargoed", which is less of a Slashdot buzzword.

    To understand why it works this way, you need to realize that your average spacecraft scientist will spend their *entire career* designing and implementing one mission. Two if they're lucky.

    So suppose you've been working on making the Kepler mission a reality since 1990. Every day for 20 years you've spent designing instruments, writing proposals, doing proof-of-concept studies, to make it happen. Then one day, the mission launches, and you release data to the public in realtime. The next day, some random dude like myself hits your website, happens on just the right file, writes a quick note to Nature, and gets the credit for discovering the first Earthlike extrasolar planet. You get a brief mention in the acknowledgements.

    Folks on Slashdot are used to thinking of the value of data as measured in pennies or dollars. This data's value is measured in lifetimes. Without this sort of "embargo" system, no scientist could afford to pursue a multidecadal project, and cool things like Kepler wouldn't happen.

  12. Big takeaway here: more Earth-like planets. by Anonymous Coward · · Score: 2, Interesting

    Most of the previously-discovered exoplanets are Jupiter-sized, and many are in close and/or eccentric orbits which would seem to preclude Earth-like planets. BUT this MIGHT have been due to sampling bias from the methods we'd been using. So this mission was really important to determine if big, disruptive planets in close orbits were the rule (thus making Earth-analogs less common) or an exception that was just easy to detect.

    What this mission seems to show so far is that - at least for very close orbiting planets - rocky worlds are much more common than gas giants. This is a very, very good sign, because if the 1/R^2 relation holds at orbits around 1 AU, there will be about as many systems with Earth-sized planets in the habitable zone as there are systems with larger (2+ Earth-radius) planets. Combining what we learn here from what we've learned before, it seems that *when* big planets are in closer orbits than they are in our solar system, they tend to have disruptive orbits, *but* these are not the common case.

    The big question will be where the 1/R^2 relation between planetary radius and frequency shown in this study breaks down. In our solar system, there are two Earth-sized bodies, a number of bodies between 1/4 and 1/2 Earth radius (especially if you count moons), and many, many smaller bodies. But the smallest body in a planetary orbit is only about 1/3 Earth size. Again, this could be error due to very small sample size but there is probably a minimum mass/radius to achieve a stable, clear orbit; I'm still guessing it's considerably smaller than Earth, however, and so our chances of finding Earth analogues in habitable orbits is hopefully quite good.

  13. Obligatory XKCD by Hurricane78 · · Score: 2, Funny

    Obligatory XKCD: http://xkcd.com/384/

    --
    Any sufficiently advanced intelligence is indistinguishable from stupidity.
  14. three regular eclipses to verify by peter303 · · Score: 2, Interesting

    Most of these data were just a single transit. Some could have been a non-orbital passing objct, a sunspot, etc.

    It would take 2-3 years to verify an Earth-like planet, so 700 already is amazing.

  15. Re:Candidates? by Narishma · · Score: 4, Funny

    if it orbits a planet it is a moon

    Not necessarily. It could be a giant space station.

    --
    Mada mada dane.
  16. We could find alien life pretty soon by Hazelfield · · Score: 3, Interesting

    I hope more people share my opinion that finding and characterizing exoplanets is THE most exciting scientific field of our time. My elderly astronomy professor at Stockholm University said three years ago that he hoped to live to see the day when they discover alien life the first time.

    His explained that all the evidence is out there - all we need is better instruments. With Kepler we can now find many more planets. If some of them turn out to be of roughly the same size as Earth and in the habitable zone, the next thing to do would be analyzing the atmospheric spectrum of the planet. Presence of free oxygen in such a spectrum would be a VERY strong indication of life. Oxygen is highly reactive and if not for the constant re-supplying of free oxygen by plants, the percentage of free oxygen in the atmosphere would be next to nothing.

    Best thing of all is that the upcoming James Webb Space Telescope will be able to measure spectra from exoplanets (maybe just jovian planets though, not sure on the details so someone please enlighten me). This means that with extreme luck, the first discovery of alien life could come as soon as 2014 (not that I actually believe that, but just so you get a sense of the timescale.) Extra-terrestrial life has for a long time had a reputation of being a subject for philosophers and conspiracy theorists, but this isn't sci-fi or some far-flung ideas that will never work - this is real science and we're doing it now.

    The next few decades could very well turn out to be the most exciting years ever in the history of astronomy. I just wish more people could realize how cool this really is.