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First Planet Known To Orbit a White Dwarf Is Falling Apart (nasa.gov)

schwit1 writes: It's virtually certain that some white dwarfs still have planets in orbit despite their violent histories, but seeing those planets has proven difficult... at least, until now. Astronomers using the Kepler space observatory have spotted a planet circling around WD 1145+017, a white dwarf 570 light years away. Not that it's in great shape, mind you. The unusual light signature (PDF) from the dying star hints that the planet is disintegrating under the star's gravitational pressure, leaving behind a giant dust cloud. Researchers suspect it fell into its fatal orbit after the star's rapid change in mass triggered a planetary collision.

You should see more discoveries like this in the future, since the weaker light of a white dwarf is less likely to obscure planets. There's even a chance (however small) that collisions have bumped some planets into habitable zones, giving scientists an unusually clear view of worlds that could support life. Either way, it's evident that planetary systems don't vanish simply because their host stars are running out of time.

67 comments

  1. I new Al Gore was an Alien! by DrTJ · · Score: 1
  2. Star's rapid change in mass? by sinij · · Score: 2

    Can someone explain to non-physicist how this rapid change in mass happens?

    1. Re:Star's rapid change in mass? by micahraleigh · · Score: 1

      I was wondering the same thing. Maybe its referring to a nova or something like that so there's not much less.

      I would think that in a red giant or even black hole stage it would still have the same mass.

    2. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      According to the White dwarf article at Wikipedia, a white dwarf is left behind when a red giant sheds "its outer layers to form a planetary nebula".

    3. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 1

      From TFA:

      As stars like our sun age, they puff up into red giants and then gradually lose about half their mass, shrinking down to 1/100th of their original size to roughly the size of Earth. This dead, dense star remnant is called a white dwarf.

    4. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      A star is in a constant tug of war between fusion trying to blow it apart and gravity holding it together. After it burns so much fuel in it's core that there isn't enough energy to fight gravity it collapses. But the outer shell still has enough fusion to overcome gravity and it becomes a really big H-bomb.

    5. Re: Star's rapid change in mass? by troon · · Score: 2

      Still doesn't change mass. Yes, density is a lot greater, but gravity doesn't care about that.

      --
      Ydco co ,df C erb-y go. a Ekrpat t.fxrapev
    6. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      Yes, it's called a supernova.

      https://en.wikipedia.org/wiki/Supernova

    7. Re: Star's rapid change in mass? by troon · · Score: 1

      It doesn't. The media have confused surface gravity of a much denser object with gravity at orbit distance, which will be unchanged.

      --
      Ydco co ,df C erb-y go. a Ekrpat t.fxrapev
    8. Re: Star's rapid change in mass? by Anonymous Coward · · Score: 0

      Gravity doesn't change from a galactic standpoint, but it changes as felt from the orbiting planets because the mass is ejected beyond their orbit.

    9. Re: Star's rapid change in mass? by gstoddart · · Score: 1

      Well, the actual Nasa article talks about changes in mass, and stars pretty constantly eject material.

      And this says:

      This also means the massive stars (with masses greater than 1.4 solar masses) must shed most of their mass as planetary nebula or the final contraction to a white dwarf cannot be stopped by the degenerate electrons.

      So, I'm more inclined to believe there is loss of actual mass going on.

      It certainly sounds like changes in mass are part of the explanation for the mechanics of this. (Not that I claim to actually understand that.)

      --
      Lost at C:>. Found at C.
    10. Re: Star's rapid change in mass? by Anonymous Coward · · Score: 2, Insightful

      "gradually lose about half their mass,"

      "Still doesn't change mass"

      So losing half the mass doesn't change the mass?

    11. Re: Star's rapid change in mass? by Anonymous Coward · · Score: 4, Insightful

      The mass of the star has changed, in that perhaps half of its mass has been expelled into a planetary nebula. That expelled mass is beyond the planet's orbit, and the orbit of the planet is subsequently determined only by the remaining stellar mass. Also, that expelled mass is moving away from the remaining white dwarf, and is being diluted in interstellar space. I've forgotten enough college physics to be unable to say what the expected effect on the planet is due to the combined effects of the force of expulsion and the reduced mass of the central star on the planet's orbit should be (does it move in or out, etc).

    12. Re: Star's rapid change in mass? by Anonymous Coward · · Score: 1

      This. A typical main-sequence star (like our Sun), will eventually burn through (fuses) it's hydrogen, it then fuses the resulting helium and other elements and expands in a red-giant (for low and medium mass stars, high mass stars will form supergiants). Eventually the star will shed its outer layers (forming planetary nebula) and the core of the star made up of carbon and oxygen will collapse into a very dense white dwarf. White dwarves cannot sustain fusion, and as a result succumb to immense gravitation pressure, as a result are very dense with high mass (comparable to the Sun, even though star would have lost a mass as it shed it's outer layers) but the volume of Earth. Since volume does not dictate gravity, mass does, the gravity from very dense white dwarf star is no more than the original star. In fact, if the Sun were today to form a very high density but low volume black hole, but with still the same amount of mass, the gravity would not change in relation to the Earth, all other things being equal.

    13. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      This is a planetary nebula stemming from the demise of a sun-like star. No supernova happening in this case.

    14. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      You remember when yo momma went to that fat camp? It's kinda like that.

    15. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      it's means it is.

    16. Re: Star's rapid change in mass? by DigiShaman · · Score: 1

      As the saying goes - a candle that burns twice as bright burns for half as long.

      If it's a white star, it's only because it's mass is so dense that it's able to burn through its fuel (hydrogen, helium, other elements) at a much MUCH faster rate. As such, the more it converts mass into energy, the less dense it becomes. That whole E=MC2 thing.

      --
      Life is not for the lazy.
    17. Re:Star's rapid change in mass? by sexconker · · Score: 1

      It's been nice proving you wrong.

    18. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      The first letter of the first word in a sentence should be capitalized.

    19. Re: Star's rapid change in mass? by Anonymous Coward · · Score: 0

      Wrong - as a white dwarf it has already burned through its fuel, and fusion has stopped. The star is now only radiating heat that was present at the time that it became a white dwarf, and will eventually become a black (non-radiating) dwarf after many billions of years have passed (much longer than the current age of the universe). This information is all readily available in the first few paragraphs of the wikipedia article about white dwarfs.

    20. Re:Star's rapid change in mass? by ceoyoyo · · Score: 1

      When a star starts to run out of hydrogen in it's core fusion slows and the core contracts, and gets hotter. If it gets hot enough, it will start fusing helium, then carbon. The core ends up small, hot and producing a lot of energy. That energy causes the outer layers of hydrogen and helium to expand and the star becomes a red giant. Material from the outer layers eventually gets blown entirely off the star to form a nebula. That's where the mass goes.

      I guess it's fairly rapid in the context of a star's lifetime, but it's not like it happens overnight. Unless you're talking about a big star, where the core finds itself suddenly exceeding what can be supported by electron degeneracy pressure and collapsing. IIRC that process happens very quickly, and the energy produced blows the outer layers off in a supernova.

    21. Re: Star's rapid change in mass? by cyn1c77 · · Score: 2

      I've forgotten enough college physics to be unable to say what the expected effect on the planet is due to the combined effects of the force of expulsion and the reduced mass of the central star on the planet's orbit should be (does it move in or out, etc).

      Ah, I still remember that extremely painful integration in BC Calculus.

      The planet's orbit increases due to the decrease in stellar mass: F = G M1 M2 / r^2 . (The stellar mass expanded around the planet will asymptotically cancel itself out as the mass expansion radius grows large relative to the planet's orbit.)

      It's tricky to mentally model the effect of force expulsion on the planet. But if it interacted significantly with the planet, it would have forced it radially outwards with a relatively short impulse, which would result in a more elliptical orbit. It also could have induced drag on the planet's orbit during the expulsion time and the star's expansion phase, slowing the planet. But that effect would have been minimal compared to the mass reduction due to the low density of the star's outer layers.

      Of course, it could also scorch the heck out of the planet's surface.

    22. Re:Star's rapid change in mass? by Anonymous Coward · · Score: 0

      hydrogen in it's core fusion

      "its", "core, fusion".

    23. Re:Star's rapid change in mass? by TheTurtlesMoves · · Score: 1

      Main sequence stars die in different ways depending on start mass. Near the end of its life the star, like our sun will expand to huge sizes. The outer layers are sheded and eventually the fusion process stops. What is left collapses. Our sun is not big enough to become a neutron star, so it eventually becomes a white dwarf. Electron degenrate matter basically.

      --
      The Grey Goo disaster happened 3 billion years ago. This rock is covered in self replicating machines!
  3. Alternate explanation by Anonymous Coward · · Score: 0

    Another Dyson Sphere detected!

  4. We'll probably not see many of these by Anonymous Coward · · Score: 1

    regardless of what the summary says, because
    A) The star itself is smaller than a 'normal' star, making an occlusion more unlikely, and
    B) Most inner planets are likely gone after the red giant phase, leaving only planets further away which are less likely to occlude the line of sight from Earth, and
    C) Any configurations like this particular one are fleeting and on a cosmological timescale it is exceedingly unlikely we'll catch it at the right moment.

    1. Re:We'll probably not see many of these by Anonymous Coward · · Score: 0

      The submitter seems to wrongly think that planets are detected because their light is added to the light of the star. I wouldn't put any value on the second paragraph of the summary.

    2. Re:We'll probably not see many of these by Anonymous Coward · · Score: 0

      The submitter doesn't seem to think that at all. If the star is too bright, then small planets will not be able to block enough light from the star for us to be able to detect it as a clear dip in the light output. So if the star is dimmer like a white dwarf, smaller planets will block a larger percentage of the light than if the star was a large red giant or even a main sequence star.

    3. Re:We'll probably not see many of these by Anonymous Coward · · Score: 0

      The submitter said

      since the weaker light of a white dwarf is less likely to obscure planets

      No one would write "the weaker light" to mean "the smaller size", they would write "the smaller size" because that's what directly determines the blocked percentage of light. The two are not even perfectly correlated. Luminosity grows as radius^2, but also as surface_temperature^4, so it's possible to have a large dim red star, and a small bright blue star.

  5. habitable zone? by phayes · · Score: 3, Insightful

    Nope.

    White dwarfs are stars that have gone through an expansion to red giants & then shrink back down once they run out of low atomic level fuel like hydrogen & helium.

    All planets close enough to be in a white dwarf's "habitable zone" would have been well inside the star during the star's red giant phase.

    Unless someone comes up with a mechanism for the planets to escape from the red giant & then migrate even further inward to the white dwarf's now much smaller & closer "habitable zone", its extremely implausible.

    Somebody please reassure me that this is once again a "journalist" attempting to talk of matters that far outstrip his comprehension & not an astrophysicist gone barking mad.

    --
    Democracy is a sheep and two wolves deciding what to have for lunch. Freedom is a well armed sheep contesting the issue
    1. Re:habitable zone? by Anonymous Coward · · Score: 1

      Unless someone comes up with a mechanism for the planets to escape from the red giant & then migrate even further inward to the white dwarf's now much smaller & closer "habitable zone", its extremely implausible.

      The mechanism is in the summary, along with the disclaimer that it's very unlikely but possible. I get not RTFA, but at least read to the end of the summary.

    2. Re:habitable zone? by Anonymous Coward · · Score: 1

      Nope.

      White dwarfs are stars that have gone through an expansion to red giants & then shrink back down once they run out of low atomic level fuel like hydrogen & helium.

      All planets close enough to be in a white dwarf's "habitable zone" would have been well inside the star during the star's red giant phase.

      Unless someone comes up with a mechanism for the planets to escape from the red giant & then migrate even further inward to the white dwarf's now much smaller & closer "habitable zone", its extremely implausible.

      Somebody please reassure me that this is once again a "journalist" attempting to talk of matters that far outstrip his comprehension & not an astrophysicist gone barking mad.

      The red giant phase causes the start to swell up to massive sizes, albeit at insanely low density. This actually could have an aero-braking effect on planets further out, causing them to spiral inward, and they may survive this phase and end up close enough to be in the habitable zone BUT...
      Because the luminosity of white dwarves is so much lower than main sequence stars, the habitable zone is much much closer than a main-sequence star. This causes two issues. One is that as the habitable zone get closer, it also shrinks in width, making the chances of a planet residing there less and less likely. The second issue is that tidal forces start to kick in as you get closer and closer to a star as well. Within the habitable zone of white dwarves tidal locking is almost guaranteed, meaning one face of the planet will always be bathed in light, while the other resides in darkness. From what we know about tidally locked systems within our own solar system, that kind of situation doesn't seem very conducive to life.

    3. Re:habitable zone? by Anonymous Coward · · Score: 0

      Unless someone comes up with a mechanism for the planets to escape from the red giant & then migrate even further inward to the white dwarf's now much smaller & closer "habitable zone", its extremely implausible.

      Actually the dragging caused by the gas in the expansion phase can be significant enough to take away the planet's orbital momentum, causing the orbit to decay to a place closer to the star. That's what may be happening with this specific case.

    4. Re:habitable zone? by phayes · · Score: 1

      The posited mechanism is implausible to the point of being ridiculous but then your post was probably typed by a bunch of monkeys so I suppose that implausible is no longer a problem...

      --
      Democracy is a sheep and two wolves deciding what to have for lunch. Freedom is a well armed sheep contesting the issue
    5. Re:habitable zone? by phayes · · Score: 3, Insightful

      Habitable zone == zone where surface temperatures would be such that liquid water could be found at the surface of the planet. Any significant dragging would also have the effect of heating all volatiles & stripping the planet's atmosphere. A waterless cinder with no atmosphere even at temperatures between 0 & 100C is not conducive to life as we now define it.

      --
      Democracy is a sheep and two wolves deciding what to have for lunch. Freedom is a well armed sheep contesting the issue
    6. Re:habitable zone? by Rei · · Score: 2

      On the other hand, when you're subjecting planets to increased tidal forces, you're also unlocking a new source of energy: tidal flexure heating. You're bending a massive chunk of rock into a new shape, there's a tremendous amount of heat released in the process (you're probably also tidal locking it if it wasn't already).

      Counterproductive if the body ends too close to the star, but useful if the body ends up too far from the star. Unless it's to the extremes covered in this article where the tidal forces are sufficient to rip the planet into a ring.

      --
      "Oh, goodness. Look at my wrist, I have to go." "But what about your clothes?" "I don't love these."
    7. Re:habitable zone? by Anonymous Coward · · Score: 0

      All planets close enough to be in a white dwarf's "habitable zone" would have been well inside the star during the star's red giant phase.

      The planet could be a planet captured from another star.

      The capture could be intentional as well. How long is the lifetime of a white dwarf star's habitable zone compared to a different star? Even buying another 10Gry is quite a long time. A very sentimental and advanced civilization could build a shkadov thruster and get their planet captured by a different star before the parent star got too far off the main sequence.

      A black hole or active neutron star might not be so kind. A red dwarf is a safer bet with fusion lifetime measured in trillions of years. But a white dwarf might work in a pinch.

      Then again the planet may just be re-coalesced dust from the original star or the core of an extinguished close-in gas giant.

    8. Re:habitable zone? by Anonymous Coward · · Score: 1

      All planets close enough to be in a white dwarf's "habitable zone" would have been well inside the star during the star's red giant phase.

      Unless someone comes up with a mechanism for the planets to escape from the red giant & then migrate even further inward to the white dwarf's now much smaller & closer "habitable zone", its extremely implausible.

      Why have you assumed that a planet must escape from the "habitable zone" before the red giant phase, and then migrate back in afterwards? There's no need for the planet to have been close to the star before the red giant phase. If a planet begins well away from the star, and only comes near it after it's become a white dwarf, you avoid half the problem: you need to explain it migrating inwards, but you don't need a mechanism for it to migrate outwards earlier.

      An inward migration is the easier problem to solve, too. All you need is friction - say, drag in the intense stellar wind produced by the star during the red giant phase. Drag can't raise a planet's orbit, but it can lower it, and circularise it too.

      Something like this must have happened in this case, because this planet, per the linked press release, has an orbital period of 4.5 hours. That's really short - Mercury, for comparison, has an orbital period of 88 days. If this star has a mass similar to the Sun's (which it should, being a white dwarf ... at least to within a factor of three or so), this planet would be at an orbital radius of ~1 million km. That's barely bigger than the radius of the Sun - orders of magnitude less than the radius of a red giant. So either (a) this planet was inside the star when the star was a red giant, or (b) this planet was further away, and migrated closer afterwards.

      The full article is, unfortunately, paywalled, so I can't go into any more detail than that.

    9. Re:habitable zone? by Anonymous Coward · · Score: 0

      There are mechanisms for planets to migrate. As an example, it's thought by scientists that Jupiter, Saturn, Uranus and Neptune were formed closer to the Sun than they are now, that they migrated outwards early in the Solar System's existence, and that Neptune and Uranus might possibly have exchanged positions. There may have also been a fifth large planet that was ejected from the Solar System in the process.

      Take a look at the wikipedia articles 'Nice Model', 'Nice 2 Model' and 'Planetary Migration'.

    10. Re:habitable zone? by Anonymous Coward · · Score: 0

      The posited mechanism is implausible to the point of being ridiculous but then your post was probably typed by a bunch of monkeys so I suppose that implausible is no longer a problem...

      Pretty sure my comment wasn't written by your family. But I guess some random guy on the internet is knows more than the dozen or so NASA scientists that authored the paper.

    11. Re:habitable zone? by Anonymous Coward · · Score: 0

      I didn't realise your earlier post was addressing the possibility of the planet being life-bearing, which I agree is much more remote than the planet being at a habitable-zone distance. That said, the stripping of volatiles depends on how fast the dragging happens, doesn't it? Let me do a back-of-the-envelope check.

      Let's say that we have an Earth-sized planet that needs to migrate inwards towards a red-giant-becoming-white-dwarf. The required change in velocity is of a similar order to the Earth's orbital velocity, 30 km/s. This has to happen during the red giant phase, which lasts about a billion years, so the required acceleration is 10^-12 m/s^2. For the mass of the Earth, this corresponds to a force of 6*10^11 N. Over the cross-sectional area of the Earth, this corresponds to a pressure of 0.005 Pascals.

      This is roughly the pressure of Earth's atmosphere at an altitude of 40 km, which (I think?) means that this much drag pressure would strip off the atmosphere above this altitude. As the atmosphere recirculates, more gas rises above this altitude and gets stripped off, and this continues for a billion years. But I don't know how to work out just how much gas is lost in this process.

      The other issue is heating. Multiplying the force and velocity above gives us 2*10^16 W, which is the kinetic energy of the material flux striking the planet. Dividing cross-sectional area again gives us 150 W/m^2. This is smaller than, but not insignificant compared to, solar power flux at Earth, which is ~1000 W/m^2. So the heating would be enough to raise the temperature noticeably, but not dramatically.

      (A 15% increase in power corresponds, by the Stefan-Boltzmann law, to a 15/4 ~4% increase in temperature. Starting from a temperature of ~300K, that's a 12K rise: not nearly enough to wipe out life.)

      So, in summary, the heating isn't a major problem, but the atmosphere-stripping probably is. I wonder, though, whether the atmosphere could be replaced by volcanic outgasing. Even if the planet was tectonically dead, it could be reheated by tidal effects once it was close enough to the star.

    12. Re:habitable zone? by phayes · · Score: 1

      No-one doubts that there are planets orbiting white dwarf stars & nobody cares that there are burnt-out cinders orbiting far off stars. It's the possibility of life being able to exist on the discovered planet "in the habitable zone" that would make it news.

      Your BOTE calculations forgot to take into account the following points:
      - No inner planet will survive being englobed by a red sun. Stellar density will be high enough to slow them down so that they impact the stellar core long before the red giant phase is over.
      - For planets further out to migrate inward to the point that they are in the habitable zone they would have to be englobed by the sun in it's red giant phase as well. Thus the solar flux cannot be calculated as a more or less one point source but from all points. Add at least 3 zeros to your 15% and it changes the outcome. By the time the star evolves on to be a white dwarf, all volatiles would have long been baked off & stripped away.

      --
      Democracy is a sheep and two wolves deciding what to have for lunch. Freedom is a well armed sheep contesting the issue
    13. Re:habitable zone? by phayes · · Score: 1

      That there are mechanisms that make it possible for some animals to fly doesn't mean that pigs can fly. You're trying to perform a similar leap of logic.

      --
      Democracy is a sheep and two wolves deciding what to have for lunch. Freedom is a well armed sheep contesting the issue
  6. Doc Brown is tearing space-time apart! by Anonymous Coward · · Score: 0

    That explains Slashdot's new slogan:

      Yesterday's news, tomorrow.

    1. Re:Doc Brown is tearing space-time apart! by AmiMoJo · · Score: 1

      This was happening 570 years ago. Some kind of /. record?

      --
      const int one = 65536; (Silvermoon, Texture.cs)
      SJW, n: "Someone I don't like, and by the way I'm a fuckwit" - AC
  7. Might yet be aliens! by Anonymous Coward · · Score: 0

    May not be a Dyson Sphere, could still be (the result of) a Death Star!

  8. "Is"? by Anonymous Coward · · Score: 0

    Shouldn't the verb be, "was"? I mean, we're talking about over half a century ago when all this happened.

    1. Re:"Is"? by Anonymous Coward · · Score: 0

      I meant "millenium", not "century", duh

    2. Re:"Is"? by Anonymous Coward · · Score: 0

      "Falling apart" is a process, and you've failed to argue that it's currently over. We commonly say "is" when something is likely to be ongoing, otherwise we're have to use the past tense all the time in everyday life. You'd tell a girl "you were beautiful" because of the nanosecond delay, and wonder why you're alone.

    3. Re:"Is"? by Anonymous Coward · · Score: 0

      speed of light it about 1 foot per nanosecond...however human reaction time is on the order of 200 milliseconds.

      regardless of how close you are it will take you nearly 1/5 a second to recognize how beautiful she is.

      so if she asks you if she is looks fat, your best option is to just run away, because she is going to wonder why it is taking so long for you to answer.

  9. I meant "millenium", not "century", duh. by Anonymous Coward · · Score: 0

    I meant "millenium", not "century", duh.

  10. You should see more discoveries like this by xxxJonBoyxxx · · Score: 1

    >> You should see more discoveries like this in the future

    I'm sorry, I don't currently have access to the Kepler space observatory. Perhaps YOU'LL see...

  11. timey wimey wibbly wobbly by Anonymous Coward · · Score: 0

    We're now observing what happened 570 years ago. It's important and sciency to keep that in perspective.

  12. Pedantic, but by Anonymous Coward · · Score: 0

    the planet fell apart 570 years ago.

  13. The Dink by PopeRatzo · · Score: 1

    We don't call them "White Dwarf" any more. Now, they're known as "White Little People".

    --
    You are welcome on my lawn.
    1. Re:The Dink by Anonymous Coward · · Score: 0

      Oh you mean like crackers!

    2. Re:The Dink by PopeRatzo · · Score: 1

      Wha?

      --
      You are welcome on my lawn.
  14. What's "gravitational pressure"? by wonkey_monkey · · Score: 1

    the planet is disintegrating under the star's gravitational pressure

    I'm guessing that's not the actual scientific term for whatever's happening to it. So what is? Is it a tidal forces thing?

    --
    systemd is Roko's Basilisk.
    1. Re:What's "gravitational pressure"? by Blaskowicz · · Score: 2

      See the Roche limit, this term describes the boundary where you are at risk of disintegrating. A small moon around a gas giant would end up as big Saturnian rings.
      Yes ocean tides would be a very tiny version, or Jupiter melting Io is more dramatic but not quite disintegrating.

      If the moon came much closer I'm sure we'd have no danger of the Earth disintegrating but perhaps we would all be dead from earthquakes and tsunamis (or worse)

  15. Planet? by Anonymous Coward · · Score: 0

    Most of the articles that I've read on this matter say 'planetesmil' (or something like that), not planet . This implies that it's more likely the size of an asteroid, or perhaps slightly larger, not planet-sized.

  16. It's a good thing we have seen this happen by Anonymous Coward · · Score: 0

    so many times before in our own solar system so we could calibrate our instruments and correlate the actual observed phenomena to these changes in light to allow us to then see those light changes in a distant solar system and therefore know what is happening out there........ oh...... um......wait, it guess we have NOT ever actually observed such an event and therefor this bit of change in light from a distant star is only fueling speculation about what is happening in that distant solar system.

    The people pushing this narrative may very well be correct, BUT there may also be some explanation that they simply have not thought of. The idea that their explanation of their observations is the only possible explanation in the universe is patently absurd. We used to get treated to all sorts of sciencey paintings of what Mars was like based on fuzzy optical observations from far away - and the concept art for Mars included water-filled canals and huge regions of green vegitation that changed seasonally, obviously farmed by Martians. There are far too many of these bold proclamations pouring out of NASA these days accompanied by concept art to illustrate the claims. Until we have actual observations that produce actual images, rather than creative concept art painted to match the preconceived notions of the astronomers involved, there's no "there" there. This is as solid and scientific as "The Wizard of Oz" (which also included some science-related facts like "tornadoes destroy farms" and "hot air rises and can lift manned balloons"...) though there will doubtless be more research grants forthcoming.

    1. Re:It's a good thing we have seen this happen by ceoyoyo · · Score: 2

      Eclipses and transits are fairly common in the solar system. If you recall, a few years ago there was a somewhat rare transit of Venus across the sun. There was quite a bit of excitement about observing it because the information could be used to tune some of the models of exoplanet discovery.

  17. The star isn't running out of time by spauldo · · Score: 1

    Considering white dwarfs live an insanely long time, the star isn't "running out of time."

    If a habitable planet was orbiting a white dwarf, life on that planet could potentially go on for billions and billions of years, barring any planet-killing catastrophes. The star would slowly cool, but life once formed might be able to adapt to the cooling temperatures over billions of years.

    A red dwarf would be better, though. They're practically immortal and keep a steady output over their lifetime. Only problem there is that the habitable zone is really, really close to a red dwarf.

    --
    Those who can't do, teach. Those who can't teach either, do tech support.
    1. Re:The star isn't running out of time by Anonymous Coward · · Score: 0

      I have not done the math, but it may be impossible for life to exist in a so called habital planet around a white dwarf. While the energy output might be enough to sustain life, white dwarfs iirc are abnormally radioactive. So life would have to survive that. Also, any planet that was inside a red giant (before becoming a white dwarf) would be sterilized as the entirety of the surface of the planet down past the mantle would likely be melted (look at Venus which suffered from a less fate).

    2. Re:The star isn't running out of time by spauldo · · Score: 1

      If that's the case, then surface life would probably be difficult. I don't think radiation wouldn't be very harmful for life in an ocean, however.

      And yeah, I'm not suggesting a habitable planet would stay habitable after being inside a red giant. However, if a planet became habitable after the red giant phase (imagine the amount of chaos going on after the star collapsed - planets would change position, possibly collide, lose their atmospheres, possibly gain new atmospheres and oceans from outgassing, etc.), it could potentially allow life a longer time to evolve than it would have had before.

      I'm sure that's not horribly likely, but hey, there's a whole lot of stars out there.

      --
      Those who can't do, teach. Those who can't teach either, do tech support.
  18. That's nice, but by Anonymous Coward · · Score: 0

    it has little to do with this other than the general concept of observing a stellar transit.

    The point is that there is more speculation here than actual science. There is SOME interesting observation data, but nothing to calibrate it with and compare it to. The conclusions and artwork are as tethered to facts as the pronouncements of Carmack the Magnificent and as likely to be proven wrong someday as the aforementioned pronouncements about Mars were once we actually sent a probe to Mars for REAL up-close observations. Now that we have seen Mars up-close, we CAN make useful conclusions about things we see at Mars from a distance (like from Hubble). Same for all the other bodies in this solar system. Once we have directly imaged them in sufficient detail to know what's there, generally and what sort of body we are observing, THEN we can make great volumes of well-established conclusions about subsequent remote observations.

    Just look at all the surprises we are seeing at Pluto from one probe flyby that are re-writing the book on the planet and its moons relative to what was learned and believed from remote observations before the fly-by. Do you have a firm grasp of just how much farther away that white dwarf is than Pluto is? It's many orders of magnitude farther. The observations are likely to be that much more inaccurate.