A rogue planet (or a rogue anything, for that matter: a celestial body other than a star) is something that's drifting through space without being attached by gravity to any star. They're just out there in the big black void. Is there any evidence that they actually exist? Or are they purely hypothetical?

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    $\begingroup$ Related: astronomy.stackexchange.com/questions/1715/… $\endgroup$
    – userLTK
    Nov 18, 2015 at 10:12
  • $\begingroup$ @userLTK: Barely. The OP actually asks how rogue planets are discovered; the answers treat of discovery methods, all hypothetical, and refer to some "claims." In other words, we're dealing with pure fantasy and wishful thinking. My question is more to the point: hard evidence. Does it exist or doesn't it? If the former is true, I could use some links. If not, a simple "no" would suffice. $\endgroup$
    – Ricky
    Nov 18, 2015 at 10:27
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    $\begingroup$ Why don't you follow the several links that are in my answer to that question and read what the evidence is? If you look at the more recent papers you will find references to other studies too. So, yes there is "hard evidence" for low-mass objects (much lower in mass than the minimum mass of a star) that are free-floating in the sense of not being bound to another star. Whether they could be called "rogue planets" depends on your definition of a "planet". $\endgroup$
    – ProfRob
    Nov 18, 2015 at 16:54
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    $\begingroup$ What is your problem? You have come here, seeking an answer. You've asked a question that has already been answered. I seek clarification about what it is about that answer you don't understand. If you already (think you) know the answer to your question, why bother to ask it. Indeed, why come to Astronomy SE to ask questions that you don't want an astrophysicist or astronomer to answer? I'm genuinely mystified. $\endgroup$
    – ProfRob
    Nov 18, 2015 at 21:18
  • $\begingroup$ @RobJeffries: See what I mean? )) My question had not been answered when I posed it. I have my answer now. I always seek a neutral party's opinion <i>first</i>. If I asked an amateur of music which composers inspired verismo opera, they'd probably say 70% Wagner and 30% Verdi. A professional musician would probably explain why my question was wrong; and then divest himself of a long list of references discussing Bach's fugues, Berlioz's orchestration, Boito's Wagnerism, Giordano's "true verismo" (as opposed to Puccini's less-than-true verismo), etc, and never get around to mentioning Verdi. $\endgroup$
    – Ricky
    Nov 18, 2015 at 23:43

2 Answers 2


Rogue planets have been discovered by infra-red imaging because planets are hot when they form. Here's a list of a few.

There's 2 types of Rogue planets. One is failed stars. condensing pockets of gas and dust that form similar to how our solar-system formed, but that are too small to form stars. Source.

The 2nd type is planets that escape from a star's orbit. This can happen by the star ejecting material and losing mass which causes the planets to expand in more distant orbits, some eventually escaping, or by gravitational assist either planet on planet or by two stars passing quite close to each other. It's statistically impossible for Rogue Planets not to, from time to time, get ejected from solar systems, so they have to exist at least in reasonably large numbers throughout the galaxy, though I don't think it's well known how common there are.

Our solar-system might have ejected a planet - see here. In general, larger planets can eject smaller ones but mostly not the other way around, but two stars that pass too close to each other can eject any planets, mostly ones with more distant orbits. A star that loses a lot of it's mass or a star that goes nova can push planets out of it's orbit too.

  • $\begingroup$ Thank you. Great stuff! Let me just make sure. 1. Type One, failed stars: at least one has been confirmed. 2. The existence of Type Two is hypothetical; it is probable according to today's paradigm, but none have been discovered. 3. Some calculations point to the ejection of a gas giant from the Solar System at some point in the past, but those are not as solid as, say, the calculations that suggested the positions of Neptune and Plato prior to their discovery. Does that sound about right? $\endgroup$
    – Ricky
    Nov 18, 2015 at 11:11
  • $\begingroup$ @Ricky Sedna might be a captured rouge planet of the second type, formed by one star but ejected to another early on as several stars formed simultaneously in a crowd out of the same nebula. If so, it would be the first rouge (or rather now adopted) planet directly observed. Says something about how common they should be, I just don't know what. $\endgroup$
    – LocalFluff
    Nov 18, 2015 at 11:46
  • $\begingroup$ @LocalFluff: Well, it does orbit the Sun, so it kind of doesn't count. Or does it? $\endgroup$
    – Ricky
    Nov 18, 2015 at 11:53
  • $\begingroup$ @Ricky If it was an ejected planet, it would have been a rogue in the time prior to its capture by the Sun so, yes, it does count as evidence that rogue planets of the second type exist given that it is indeed an example of an ejected planet. $\endgroup$
    – called2voyage
    Nov 18, 2015 at 15:45
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    $\begingroup$ @Ricky given the nature of 3 body or N greater than 2 body gravitational systems, saying rogue planets "hypothetically exist" is like saying some workers at a large company "hypothetically are looking for better jobs" the statistics make it impossible for ejected Rogue planets not to exist, even if none have been definitively observed. $\endgroup$
    – userLTK
    Nov 18, 2015 at 21:00

Giant planets when first formed are big and hot. They radiate their own light, mostly in the infrared. So young isolated planets can be seen directly.

There have been various claims in the literature that objects as small as a few Jupiter masses have been identified in young star forming regions. See various papers by the IAC brown dwarf research group





Another object that is part of the beta Pic moving group, recently discovered by Liu et al. (2013), has an estimated mass of about 8 Jupiter masses (Biller et al. 2015).


These claims are open to criticism - sometimes it is hard to tell whether a faint object really belongs to the star forming region observed, rather than being an unassociated background object. The claimed masses also depend heavily on models for the luminosity-mass relation as a function of age, and the ages of these objects are not easily constrained. The likelihood is that at least some of these objects are below 10 Jupiter masses and would rank as planets by some definitions; though none of the individual objects could be said to be proven beyond any doubt.

Nevertheless it would not be surprising if, in the maelstrom of the formation of a cluster of stars, some planetary systems were stripped from their parent stars by close encounters with other objects and indeed numerical simulations of planetary systems in dense star clusters show that this process occurs (e.g. Davies 2011).


The chances of seeing older, isolated, planetary mass objects are slim, but microlensing appears to be the only technique presently available. The microlensing signature of a free-floating planet is of course unrepeatable so a discovered planet could not be followed up in any way. However, surveys of microlensing events could be a way of saying something statistically about how common such objects are. See for example http://astrobites.org/2011/05/24/free-floating-planets-might-outnumber-stars/

It is also worth noting that the whether these things really are "planets" at all is disputed. They could either be genuine planets, formed in the same way that is hypothesised for most giant planets - that is by accretion onto a rocky core that formed around a star. They could then have been displaced from their parent star by dynamical interactions with other bodies in their system or with a third body. As I said above, N-body simulations do predict that this will happen (e.g. Liu et al. 2013).

On the other hand they could represent the very lowest mass gas fragments that are able to form during the collapse and fragmentation of a molecular cloud and that for some reason were unable to accrete further gas (i.e. they are really more like low-mass brown dwarfs). This so-called "fragmentation limit" is of order 10 Jupiter masses, but if it were a little lower it might explain the free-floating "planets" that have been seen so far.

  • $\begingroup$ Thank you for your answer. It is everything I expected it to be and more: it is thoughtful, informative, and impeccably worded. The links are fascinating. I don't mean to be a nag, but I feel I must reiterate, that in my (admittedly very amateurish) view, claims and predictions do not constitute hard evidence, which means that the answer to my question is "No." Thanks again! I'll have to revisit the links a couple of times just to make sure. You are, in fact, a lot more objective and infinitely more courteous than most astrophysicists I know. $\endgroup$
    – Ricky
    Nov 19, 2015 at 2:47

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