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  1. #1
    jsavard@ecn.ab.ca's Avatar
    jsavard@ecn.ab.ca Guest

    Default Friday the 13th is CERTAIN to be unlucky



    The data the JPL had on the asteroid Apophis back on July 3, 2005 led
    to the possibility that the asteroid might, in the near encounter on
    Friday, April 13, 2029, go through one of several "keyholes".

    One keyhole would have changed its orbital period to 5/4 of a year,
    leading to it having a close encounter with the earth in 2034.

    Another would have changed its period to 6/5 of a year, making the date
    of its return one year later, in 2035. Still another would have made
    the period 7/6 of a year, so it would return in 2036, and then another
    would make it 8/7 of a year, so it would return in 2037.

    And then, yet another one would have made the period 17/15 of a year,
    for a return in 2046, and another would have made it 19/17 of a year,
    for a return in 2048.

    Improved data available on June 20, 2006 left only the 2036 return a
    strong contender, with the keyhole for a 2037 return just outside the
    3-standard-deviation error ellipse.

    What's wrong with this picture?

    For one thing, they seem to have left out other fractions. What about
    9/8 of a year? Or 11/9, 13/11, or 15/13 of a year?

    Just between 7/6 and 8/7, though, there are other possible resonances,
    or, at least, rational numbers, besides 15/13, which could lead to the
    asteroid hitting the Earth in 2044.

    22/19 and 23/20. 29/25 and 31/27. And on and on.

    The size of the "keyhole" for a 2036 impact is only 641 meters, less
    than 1/5000 of the length of the error ellipse.

    For a given small, but finite value epsilon, what proportion of the
    points on the real number line are within epsilon of a rational number?
    As any mathematician will tell you, all of them are.

    However, that implies there is no upper bound to the denominators on
    the fractions involved. That Apophis might be deflected into an orbit
    which would cause it to collide with the Earth a few billion years
    _after_ the Sun left the main sequence would not be a concern.

    If, however, the "window" for, say, the 151/131 resonance, leading to a
    collision with the Earth in the year 2180, were also around 600 meters
    or so in width, which may not be the case, then, with room for about
    5000 keyholes between the 7/6 resonance and the 8/7 resonance, the
    denominators don't have to grow to billions or even millions.

    Unless it is deflected, it therefore is certain to strike the Earth
    sometime in the next few thousand years. And, furthermore, even if it
    is deflected, so as to avoid an imminent collision with the Earth, in
    the relatively simple ways in which it is currently envisaged to
    deflect it, it would remain in an Earth-crossing orbit which would
    eventually cause it to strike the Earth.

    Suitably altering an encounter with the Earth so as to deflect an
    asteroid into an orbit which passes close by either Venus or Mars would
    be likely to lead to the asteroid ceasing to be an Earth-crossing
    asteroid. Still, just delaying an imminent impact by centuries is both
    worthwhile, and a good way to get some practice.

    John Savard


  2. #2
    Henry Spencer's Avatar
    Henry Spencer Guest

    Default Friday the 13th is CERTAIN to be unlucky

    In article <1160275510.112627.206830@m73g2000cwd.googlegroups .com>,
    <jsavard@ecn.ab.ca> wrote:

    It's not. In general, the larger the denominator -- that is, the more
    years elapsed before the next encounter -- the more time there is for
    small errors to build up to a miss, and hence the narrower the keyhole is.
    Note also, if I recall correctly, that the 641-m keyhole is for a 2036
    *close encounter* of some kind, not a 2036 *impact* -- only a very small
    part of that keyhole steers the asteroid to an actual impact.

    Moreover, remember that the story is more complex than just hitting one of
    those resonances. There are perturbations present, notably from other
    planets. For many denominators, there may *be* no plausible numerator
    that actually produces a close encounter, because perturbations may chance
    to affect the close-encounter cases more than other cases. (The flip side
    of that is that you can get focusing effects, which widen the keyholes for
    specific cases.) This is probably why they seem concerned about only a
    few specific resonances.


    As above, it's not that simple. Moreover, near misses are much more
    likely than direct hits, and any near miss will change the orbit yet
    again. This process can easily pump the orbit up or down enough that the
    object encounters other planets. If memory serves, for a random case, the
    long-term probability of impact on *any* of the inner planets is only
    something like 20%. The most likely end result is for perihelion to be
    pumped down far enough that it goes into the Sun, and the next likeliest
    is for aphelion to be pumped up enough to encounter Jupiter, which almost
    invariably expels the object from the solar system.
    --
    spsystems.net is temporarily off the air; | Henry Spencer
    mail to henry at zoo.utoronto.ca instead. | henry@spsystems.net

  3. #3
    William Elliot's Avatar
    William Elliot Guest

    Default Friday the 13th is CERTAIN to be unlucky

    On Sat, 7 Oct 2006 jsavard@ecn.ab.ca wrote:

    After 2029? No, that can't be. By the time it get's here to wipe US
    (including UN etc) out, it'll be too late. US (and UN etc) will have
    already wiped US (including UN etc) out. Damn, and to think if it wasn't
    for Bush accelerating the date, I would have resting peacefully, missed
    the whole event.


  4. #4
    jsavard@ecn.ab.ca's Avatar
    jsavard@ecn.ab.ca Guest

    Default Friday the 13th is CERTAIN to be unlucky

    Henry Spencer wrote:


    Ah, of course.


    You're quite right.


    True, but each near miss is another shot at a hit.


    That's interesting. I would have thought that *any* encounter with
    planet A always, invariably, leads to the body being perturbed from one
    A-crossing orbit to another A-crossing orbit - since when it gets far
    enough away from the planet, it stops being deflected by it in a major
    way.

    Thus, an encounter with Jupiter might lead to the body being, almost
    invariably, perturbed into a cometary orbit with a period over 50,000
    years, but as far as acquiring solar system escape velocity, that
    should not happen. Of course, this may well be based on some simplistic
    assumptions.

    John Savard


  5. #5
    jsavard@ecn.ab.ca's Avatar
    jsavard@ecn.ab.ca Guest

    Default Friday the 13th is CERTAIN to be unlucky

    jsavard@ecn.ab.ca wrote:



    Oh, silly me. Of course the new orbit still has to cross the orbit of
    Jupiter. But it can be a hyperbola instead of an ellipse.

    John Savard


  6. #6
    Henry Spencer's Avatar
    Henry Spencer Guest

    Default Friday the 13th is CERTAIN to be unlucky

    In article <1160307137.800175.4890@k70g2000cwa.googlegroups.c om>,
    <jsavard@ecn.ab.ca> wrote:

    Correct, but *on average*, you get many near misses before a direct hit.
    The "near miss" zone around Earth is far larger than Earth itself.


    True, but as you note in your followup, the new orbit can be hyperbolic,
    so it's not coming back. Jupiter is massive enough and moving fast enough
    that the chances of that happening on a random encounter are substantial.
    (New Horizons's Jupiter gravity assist never takes the spacecraft closer
    than 2.2 million km, and nevertheless boosts it well past solar escape.)
    And if a particular Jupiter encounter doesn't do that, then the new orbit
    still intersects Jupiter's, and there'll probably be another encounter
    fairly soon. Jupiter has such clout that, by the standards of the sort of
    orbit evolution we're talking about, this happens very quickly.
    --
    spsystems.net is temporarily off the air; | Henry Spencer
    mail to henry at zoo.utoronto.ca instead. | henry@spsystems.net

  7. #7
    Hop David's Avatar
    Hop David Guest

    Default Friday the 13th is CERTAIN to be unlucky

    jsavard@ecn.ab.ca wrote:


    Of interest here is the "height" of a rational number.

    "Every rational number has the form p / q, and we may assume that q is
    always positive. Define the height of a rational number p / q as |p| + q."
    From http://web01.shu.edu/projects/reals/...s/cntbl_q.html

    By this definition a rational number can have many heights. But I'm
    thinking of the smallest possible height when numerator and denominator
    are co-prime.

    Orbital periods with small heights can have regular, frequent fly bys.

    Most of the "short" rational number periods we know about are greater
    than 1. For example the height of Toutatis' period is 4+1 which is 5.

    Of more concern are the short rationals that are less than one. For
    example an NEO with a period of 2/3 year has the same height as
    Toutatis' period but could visit near earth space every two years
    instead of 4.

    If an NEO's apohelion is at or slightly less than 1 a.u., it becomes
    difficult to detect. It spends most of it's time in the day sky. On the
    rare occasions it's visible, it's near the horizon around sundown or
    sunset. The phase angle during close approaches also conspires to make
    these objects hard to see.

    In my opinion this is a major blind spot in our search for NEOs.

    Hop





  8. #8
    Chris Jones's Avatar
    Chris Jones Guest

    Default Friday the 13th is CERTAIN to be unlucky

    henry@spsystems.net (Henry Spencer) writes:


    Depends on what you mean by "boosts it ... past" since NH has been
    moving faster than solar escape velocity since its launcher stages
    finished their job.



 

 

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