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Trip to a Black Hole

This journey has thirteen stages!  Each stage is numbered!

ACTIVITY:  Print out a copy of this journey.  Then, look through
the links for "Amazing Space" and "NASA's Hubble Space Telescope" 
for pictures that might illustrate different things you see during 
this journey.  Print the pictures and paste them next to what 
they illustrate!

Try also looking at the pictures collected in the "Black Hole Trip 
Links!"

          "Gift of a star's furnace, it grew heavier
          when brought here . . . "
                                 --John Peck (1978),
                                 describing the key to the 
                                 glass mountain where the
                                 seven ravens were imprisoned
                                 (in the tale of "The 
                                 Seven Ravens").
                                 (From John Peck, "Redemption,"
                                 in "The Broken Blockhouse Wall:
                                 Poems" [Boston: David 
                                 R. Godine Publishers]).
              
    QUESTION:  Why do you think that the black hole's MASS pulls 
    more strongly than an ordinary star of the same MASS--that
    is, why is GRAVITY so strong near a black hole?
    (The MASS of something is the "total amount of matter" in it.) 


1.  Viewing the black hole from a distance:

  * You see a black spot in space, but strange things might
    be happening nearby.

  * You might see gasses streaking past at nearly the speed of light!

  * You might also see lightwaves emitted from the black spot's ends.

  * You might see nearby stars suddenly become brighter as they
    get closer to the black hole's image in space, and then
    fade again as they move away.

    QUESTION:
    Why do you think matter might travel past a black hole at speeds
    close to that of light?  (You'll think about this again at stage
    10 of your journey!)

2.   Approaching the black hole:

   * As you approach the black hole, you would feel much as 
     you would approaching any other star of a similar mass.
     If you stay the same distance from the black hole's center
     as you would stay from the center of another star of the 
     same size, you'll feel just fine, and not fall into the black
     hole at all.

   * As you travel closer to the black hole, you'll see the light
     from stars around the hole and the hole's gravity increasing
     at about the same rate!

3.   Getting closer to the black hole:
 
   * As you get to the point where the normal star's surface would
     be, you'll feel the same gravitational pull on your ship that
     you would from the normal star's surface--even though there
     is nothing there.  

   * However, if you could travel to the interior of a normal star,
     the star's gravity would decrease its pull on you, not 
     increase it.  This is because, as you enter the star, you 
     leave some of its mass behind you.  Thus, you no longer 
     feel the gravity caused by that mass pulling you down.  
     (You might, of course, feel pressure from that mass 
     as gravity pushes it down on you--unless you create
     a tunnel through the star that resists the pressure.)  
     The black hole is different.  The closer you get, the more
     gravity you feel, because none of the mass of the black hole
     has been entered yet!  The entire mass of the
     black hole is still pulling you to it! 
     (Or is there a way to tunnel through it too?  It's so small
     and concentrated--but, of course, I wonder if we can really see 
     all of the black hole, since it's so far away, and light does 
     not escape . . . )
  
4.  Taking another look at the black hole:

  * You'll see a lot of light from orbiting light waves,
    super-heated gasses moving at the speed of light, and
    electrical fields created by or drawn to the black hole's
    super high gravity.  The super-heated gasses will look
    like streaks in the sky. 

  * In the center of all this will be a black area of the sky.

    QUESTION: 
    Why do you think the image of heated gasses which are
    travelling at about the speed of light appears 
    streaked across the sky?
  
5.  Experiencing the surrounding radiation:

  * An ordinary space ship could not withstand the surrounding
    radiation of the black hole--from the light and electromagnetic
    waves (if it is really as concentrated as everyone says!)! 
  
6.  Trying to orbit the black hole:

  * You'll feel gravity pulling you down in a sort of spiral.
    To stay in orbit, and not fall, you'd have to travel very
    fast and create lots of CENTRIFUGAL FORCE to pull you away
    from the black hole.   

  * The two opposing pulls--that of the centrifugal force
    you create and that of the black hole gravity--will 
    cause TIDAL PULLS on your body. (TIDAL PULLS are the same kind 
    of changing gravitational pulls that cause the Earth's tides 
    --in one place of the Earth, water is pulled 
    one way, and in another, it may be pulled another way.) 
    This means that part of your body will be pulled in one 
    direction and part will be pulled in another direction.
    The closer to the black hole that your orbit is, the stronger
    the tidal pull. 

    QUESTION:  
    What do you think very strong tidal pulls might do to
    the human body? 

7.  Spiralling towards the black hole:

  * Ultimately, you will not be able to stay in orbit very long--
    due to all the tidal pulls on you!
    The shortest distance (or at least the natural way to travel) 
    to the center of a gravitational pull for some reason is not
    a straight line, but a spiral down.  Your ship will start
    spiralling down.

    QUESTION:
    Why do you think that you might spiral towards the hole?

    QUESTION:
    What do you think you will 'weigh?'  Remember, your mass stays
    constant, but your 'weight' varies with changing gravity.  
    So what sort of gravitational fields do you think you might 
    feel? Will you weigh a lot--or a little--as you fall?  (HINT:  
    there are several ways to cause a g-field:  first, gravity can be
    caused simply the pull of mass on mass, which is of course
    affected by the closeness of the two masses pulling on each other
    --for example, the closer you are to a certain mass, the greater 
    the gravitational pull of that mass on you; a second is caused by
    acceleration--for example, the pull back you feel when you accelerate 
    a car suddenly is the result of a g-field caused by acceleration; the
    third kind of gravitational field--which is really related to the 
    second--is the pull caused by spinning around something--in this
    case, you keep changing the direction of your motion in order to circle
    or spin, and so you are pulled in the previous direction as you
    change--this pull is known as CENTRIFUGAL FORCE.  Consider the
    first two kinds of G-fields to decide what gravity you will feel.
    Also, look up the term "FREE FALLING."  Will this feel like 
    FREE FALLING?  Or not?)  

    QUESTION:
    Do you think that there might be a way for people interested
    in long distance space travel to warp space (and the gravity
    that helps determine the way people can travel through
    space) so that astronauts can travel to places along a 
    more direct path than gravity normally allows?  (This was
    proposed in Marcus Chown's article, "Planes, trains, and
    wormholes"--which was published in 1996 in New Scientist.)

8.  Looking back at the universe behind you as you fall rapidly:

  * You'll see rings in the sky where the background stars--
    at a certain distance from the black hole--suddenly
    have double images--so first one ring of stars and then
    another will appear as doubles.  These rings of double
    images are called "Einstein rings."  To see these, go to:

  http://antwrp.gsfc.nasa.gov/htmltest/gifcity/fig2f.gif

    (Just type the above address into your
    web browser window--then use the back button to
    come back to finish the rest of your trip!  [This link
    is also at "Black Hole Trip Links."])
    (The above image is from Robert Nemeroff of NASA's site!)

    QUESTION:  
    Why do you think the images behind you start to double?

    ACTIVITY WITH MULTIPLE IMAGES:  
    For this you'll need two mirrors, probably a hand mirror and
    a wall mirror.  Stand in front of the wall mirror with your
    back to it, and hold the hand mirror in front of you.  Look
    through the hand mirror, positioning it so that you can see--reflected
    in the hand mirror--(1), images of your back reflected in the wall 
    mirror; and (2), images of yourself looking into the hand mirror 
    also reflected in the wall mirror.  Start tracing the
    images.  How many images do you see?  Is the number finite?
    Were all those images reflected at the same time?  What do you think? 
 
9.  Approaching and passing through the black hole's EVENT HORIZON:

  * Everything beyond the EVENT HORIZON of the black hole
    looks totally black, with only a little radiation escaping.
    This is because the EVENT HORIZON is the point at which 
    gravity is so great that nothing that we know of can get 
    out--not even your radio signals which you try to send back to Earth--
    everything is 'infinitely red-shifted,' because it is travelling
    away from us so fast (due to "THE DOPPLER EFFECT," which you
    will want to learn more about--read more below about how light 
    moving away from us vibrates less frequently!).  Radiation near
    a black hole, such as light waves and radio waves becomes too 
    faint and weak for us to detect it.  
    (Of course, most known black holes are so far from the 
    Earth that it takes years for light waves, radio waves, and other
    RADIATION to travel between the part of the universe where 
    the black hole is and Earth, anyway!)  
    It seems then that no one outside of the black hole's 
    event horizon will ever hear what you had
    to say over your radio as you crossed the event horizon.
    (The EVENT HORIZON is a sphere of high gravity that surrounds
    the black hole, and that is 'powered' by the matter in the
    black hole.) 

    QUESTION:
    What is a horizon on earth?  When ships sail over the horizon, can
    we still see them?

10. Accelerating through the PHOTON layer:

  * The black hole's gravity will accelerate you more and
    more rapidly.

  * You will fall to a point where not even matter that can
    spin away from something at the speed of light can escape.
    Even PHOTONS (particles with no mass and no charge that 
    make visible images; the particles in light waves) that 
    enter this layer cannot escape.  They start orbiting the
    black hole at the speed of light and possibly losing their
    energy to the black hole's gravity, thus vibrating less and
    less frequently (light waves that vibrate less frequently
    than visible light are INFRARED waves), or may even 
    accelerate into the black hole completely, and be absorbed
    by it.
    (Remember, the speed of light is relative to the speed of
    the matter that light comes from; all matter in the universe
    is moving relative to each other; there is no way
    to decide that some matter is moving and that some matter
    is standing still; the speed of all matter must be measured
    relative to what other matter is doing; likewise, the speed 
    of light must be measured this way--this is called
    RELATIVITY!--remember Einstein!)  

  * As you pass through this photon layer and start accelerating towards
    the hole, you will see your image streaking behind you.   

    QUESTION:
    Why do you think your image appears streaked or mirrored
    behind you?

    QUESTION:  
    SUPPOSE gravity travelled in waves, much like light, but at a much
    faster speed. (We really do not know exactly how gravity
    travels.)  IF you accelerated away from a point, toward another
    point, at the speed at which the gravity waves travelled, what
    would you experience?  

11. Approaching the surface of the black hole:

  * Looking behind you, you'll see the sky shrink into a disk
    surrounded by blackness.  Try looking at the images
    listed below--in order--to see what happens! 

  http://antwrp.gsfc.nasa.gov/htmltest/gifcity/fig2o.gif
 
  http://antwrp.gsfc.nasa.gov/htmltest/gifcity/fig2p.gif

    (Just copy the first address into your web browser
    window, and then use the back button to go back to
    this page.  Copy the second address and do the same!
    To really simulate the trip, save the addresses somewhere,
    and go to them in order without going back to this page!) 
    (Both of these images are from Robert Nemeroff of NASA!)

    QUESTION: 
    How much do you think that the sky will shrink
    behind you?
    
12. Impacting the surface of a black hole:

  * If the black hole is not a singularity--that is, if its
    radius is a little greater than 0--you'll hit a surface just below
    the photon layer, and all the matter in you will collapse 
    under gravitational and tidal pulls.  The physical matter
    in you will collapse to a density greater than that of
    an atom's nucleus, as even nuclear forces will not be
    able to keep the particles separate.
    (To see what this might look like, try going to
    the "Movies from the Edge of Spacetime" at the
    University of Illinois'"Spacetime Wrinkles" site--
    or try going to the following "thumbnail clips" from
    the "Spacetime Wrinkles" site:
    
  http://www.ncsa.uiuc.edu/Cyberia/NumRel/Images/DistortedBH3_tn.jpg
  
  http://www.ncsa.uiuc.edu/Cyberia/NumRel/Images/DistortedBH2_tn.jpg

  http://www.ncsa.uiuc.edu/Cyberia/NumRel/Images/DistortedBH1_tn.jpg

    Just copy one of the above addresses into your
    browser window--then use the "Back" button to finish your
    trip!  [Some of these "Thumbnail Clips" are also available
    at the "Black Hole Trip Links" page!])    

    QUESTION:
    Do you think that Einstein's equations still work when
    nuclear forces no longer can hold up an atom's nucleus?
    
13. Reaching the singularity:

  * If, however, the black hole is a singularity, with a radius
    of 0, all of its matter is concentrated into a point in space
    approaching 0 volume, and hence, infinite density (density
    remember, equals mass divided by volume; since the volume
    approaches 0, you have to divide the huge mass by a number
    approaching 0, and so a singularity is infinitely dense).

  * If you fall to a singularity, you fall to just a single 
    point in space.  At any moment, you take up only a point 
    in space, and only move along in space as the black hole
    moves.  So space becomes something like time--remember, we can only
    move through time as time moves us.  Thus we move in time like
    a point moving along a line (a 'ray') or vector, and our
    velocity seems to be controlled by the vector!  This is how the
    matter in a singularity moves through space:  it is all concentrated
    into that tiny point, and its movement is controlled by the movement
    of the black hole's singularity!

  * What happens to time?  No one is sure.  Gravity pulls you
    to any point--within the confines of the
    singularity--instantly, and all matter in a black hole's 
    singularity can affect all other matter in the 
    singularity instantly.
    There is no travel time from one point in the singularity to
    another.  

    QUESTION: 
    Do you think that time travel is possible in a singularity?

    QUESTION:
    Do you think all 'black holes' are pretty much the same?
    And what are they?  Furnaces that break matter down and compact
    and change it?  Or are they simply tunnels that suck things into
    places we cannot see?  Or what?  
    
    (Black holes, remember, were only recently 'discovered.'  
    They are a type of 'variable star,' and originally all variable 
    stars were grouped together by astronomers who were studying
    the variable stars--stars whose light intensity
    varied.  Some of these stars turned out to be double stars 
    rotating around each other--when one star in a double was hidden 
    behind another, the double star appeared dimmer--Alpha 
    Centauri is an example of this; some turned out to be pulsars, 
    very dense stars that emitted light pulses periodically; and some 
    turned out to be stars magnified by something that appeared to 
    have gravity even more concentrated
    than in pulsars!  These were named Black Holes.  But what are
    Black Holes?)  
  

                    
* * * * * * * * * * * * *END OF THE TRIP!* * * * * * * * * * * * * * 

     (The information in this section comes from Robert J. Nemiroff 
of NASA and the Goddard Space Flight Center (1993), Visual 
distortions near a neutron star and black hole, The American 
Journal of Physics, 61: 619 (published on the web 
November 13, 2000); 

and from the various websites--
including NASA's "Ask the Space Scientist; NASA's "Hubble Space 
Telescope;" NASA's "Amazing Space;" and the University of 
Illinois' "Spacetime Wrinkles."

     This information has been compiled and interpreted by C. E. 
Whitehead.  Any errors in it are hers.  It has been sent out to 
several astronomers and space scientists so that its accuracy can 
be reviewed; while awaiting feedback, Ms. Whitehead has checked 
the information carefully herself, too.)

NOTE TO TEACHERS AND STUDENTS:  Select pictures from the list above, 
save in order in "favorites," and, to finish illustrating your black 
hole journey, add your favorite black hole pictures to these, putting 
them in the order you think they might go in on the trip 
in "favorites" also.  Now, click on these in order to see your trip! 

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Last Modified: Thursday, January 22, 2009
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