Also, if planets form in a binary star system, what do the orbits look like ?
Given the formation of our own solar system, how could a star not form a solar system from surrounding debris ?
Given the formation of our own solar system, how could a star not form a solar system from surrounding debris ?
yes, such an encounter could possibly strip a star of its planets.I remember hearing about some extragalactic stars - idea was that a binary system gets too near a large black hole. One of them is captured by the black hole and maybe consumed, the other gets flung out of the galaxy at high speed. Could an event like this strip it of any associated planets?
Given the extraordinary size of our universe, I can't imagine that it has never happened before.
Also, i can see no reason why a star must have planets.
Do we actually know there are stars WITHOUT planets ?
there most definitely are planets around some neutron stars. in addition, there exists strong evidence that planets can not only end up orbiting neutron stars, but may also form around them:I'm pretty sure there aren't any planets around a neutron star...
To good approximation, their orbits will be conic sections focused at the center of mass of the 3-body system (star, star, planet). Since the planet will have mass much smaller than the stars, it will look like a normal orbit, except instead of about the center of the Sun, as is with the Solar system, it will be about the center of mass of the binary system.
could you elaborate on this? i don't see your logic...There is also a good chance not to find any planets in stars belonging to very small constellations.
there most definitely are planets around some neutron stars. in addition, there exists strong evidence that planets can not only end up orbiting neutron stars, but may also form around them:
http://science.nasa.gov/science-news/science-at-nasa/2006/05apr_pulsarplanets/Planets Around Dead Stars
Any planets around the stars that gave rise to pulsars would have been incinerated when the stars blew up. The pulsar disk discovered by Spitzer might represent the first step in the formation of a new, more exotic type of planetary system, similar to the one found by Wolszczan in 1992.
could you elaborate on this? i don't see your logic...
could you elaborate on this? i don't see your logic...
Well, the reality is almost certainly much more complicated than simple self gravitation.
There are many problems currently faced by planetessimal formation. A couple of them are:
How do you go from dust to about metre sized objects? This is difficult to get working in models, many simulations start with metre sized objects which can accrete from there.
How long does the whole thing take? There are constraints on how long planet formation can take, and a simple cloud of dust takes too long to form planets if you assume simple self attraction. i.e. there is other physics happening.
How do you get a planet the size of jupiter in an orbit the size of mercury's? Exo-planet statistics show a large number of planets in this regime.
Next, think about the environment of a forming star, its usually in a dense stellar environment like a cluster...how does this affect planet formation?
How do you get planets around pulsar/neutron stars ?!?
This is just the tip of the ice berg, its not clear at all why some stars form planets and others don't.
did you miss this part of the article?Eh, they haven't discovered any planets around the stars, but it does seem likely from the remnants that they could form.
The finding represents the missing piece in a puzzle that arose in 1992, when Aleksander Wolszczan of Pennsylvania State University found three planets circling a pulsar called PSR B1257+12. Those pulsar planets, two the size of Earth, were the first planets of any type ever discovered outside our solar system. Astronomers have since found indirect evidence the pulsar planets were born out of a dusty debris disk, but nobody had directly detected this kind of disk until now.
note what the article specifically says about when the planet(s) are incinerated - it happens during the supernova that creates the neutron star, not during the lifetime of the neutron star itself. i don't disagree with you that neutron stars exist for some period of time without planets, the duration of which is debatable. but if a neutron star endures an epoch without planets, i would tend to think that it is because 1) planets have not yet formed out of the debris disk orbiting it (assuming a debris disk exists in the first place), 2) it hasn't yet captured any planets with its gravity, or 3) any previously existing planets it may have had in the past were flung out of their orbits by an external gravitational influence. but i can't imagine that a "planet-less" epoch would be induced by the radiation of the pulsar vaporizing any existing planets...perhaps gaseous planets, but not rocky planets like the ones found in our inner Solar System.I was thinking of this though:
So at least for a good long time, there aren't any planets around every neutron star. They may form new planets, or may capture some, but they get all blowed up.Any planets around the stars that gave rise to pulsars would have been incinerated when the stars blew up. The pulsar disk discovered by Spitzer might represent the first step in the formation of a new, more exotic type of planetary system, similar to the one found by Wolszczan in 1992.
ok, now your logic makes sense to me. you threw me through a loop when you mistook constellations for star clusters. you see, the constituent stars of a constellation/asterism are generally not members of a common star cluster (open or globular), regardless of how large or small the constellation may be. take the small constellation Lyra for instance, which contains the bright star Vega, and approximates the shape of a small square/rhombus. while i haven't researched it myself, i'd be willing to be that if you research the 4 stars that comprise the constellation Lyra, you'll find that their distances from us vary greatly, perhaps by orders of magnitude. so while they appear to be close together in the sky, one star may be 100 times farther away from us than another (i.e. its a depth perception issue). therefore , the constituent stars of a constellation typically are 99% of the time not gravitationally bound. for the stars of a cluster on the other hand, you're assertion makes perfect sense...particularly globular clusters, as their stars are typically more densely packed than those of an open cluster.IF. If the distance between the stars of a small constellation is small, let's say star to star around the size of our solar system, then the gravities of the stars would have different effects of any planets rotating in the area. As a result those planets caught in the gravity field of that constellation would eventually get drawn into a star. This is close to what Fallen Kell said.