 
| Journal Home Page | Apollo 16 Journal | 

| Animation made from seven LROC images of the Apollo 16 landing site, ordered from sunrise to sunset, and showing the changing length and location of the shadow cast by the U.S. flag erected by the crew. The frames are: (1) M116215545RC, Sun 8 degrees above the eastern horizon; (2) M131548593RC, 10 deg. east; (3) M144524996LC, 43 deg. east; (4) M142164190RC, 69 deg. east; (5) M122108795LC , 61 deg. west; (6) M117392541LC, 7 deg. west; and (7) M132732855RC, 2 deg. west. LROC images courtesy NASA/GSFC/Arizona State University. | 
| Detail from AS16-113-18339,
              taken early in EVA-1. View to the south toward Stone
              Mountain.  The LM landed on level terrain but, beyond
              25 meters from the spacecraft, slopes could be 6-10
              degrees.  The flag is pointing somewhat north of
              west.  Note
              that John Young jumped about 0.42 meters off the
              ground.  (Click on the image for a larger version.) | 
    
| Detail from AS16-116-18723,
              taken by John Young on his way back to the LM from the
              Rover's final parking place. The view is to the
              west.  The camera was tilted about 4-5 degrees to the
              right when Young took the photo.  It is possible that
              Young took the photo with the camera handheld, almost
              certainly at chest height. The spacecraft landed tilted
              back to the east by 2.3 degrees and rolled left (south) by
              0.4 degrees. (Click on the image for a larger version.) | 
    

    
| Frame from the Rover TV taken
              after LM liftoff.  The TV camera is tilted to the
              left by about 9 degrees because the Rover was parked about
              50 meters east of the LM on uneven ground.  Note that
              the flag is pointing more to the north than it was in
              Young's photo (above) and that the flagpole is tilted to
              the right. | 
      Based on a comparison of pre- and post-ascent images, the flag did
      not fall, but the pole seems tilted by 30 degrees off the local
      vertical.  Since the rover took video from the East, the
      orientation of the flag suggests it offers a shadow perpendicular
      to the Sun’s rays at dusk and dawn.  At LM liftoff (about
      01:26 UTC on 24 April 1972, the Sun was at an azimuth  of 77
      degrees and an elevation of 50 degrees.  Consequently, the
      dark spot on the ground near the flag is the flag's shadow. 
      It seems unlikely that either the flag or the support rod that
      runs along the top edge of the flag is touching the ground. 
      Rover TV images show the rest of the flag below this edge fairly
      well which would not be the case if the top support rod was
      touching the ground (the flag on the bottom edge would be bent and
      crinkled).  A TV frame
      taken moments after John Young erected the flag shows its
      condition at that time.  Although no TV coverage is available
      of the actual deployment, it is evident that Young pushed the
      flagstaff into the ground by hand.  He did not comment on the
      depth of penetration.  The Apollo 17 crew chose to hammer the
      lower section of the flagstaff into the ground before fitting the
      upper section.  A comparison
      between the Apollo 16 and 17 flags, as deployed, indicates that
      the lower section of the Apollo 17 flagstaff (below the gray joint
      section) is about 10-20 cm farther in the ground than the Apollo
      16 flagstaff.  Seeing the obvious tilt of the Apollo 16
      flagstaff in the post-liftoff TV may have convinced the Apollo 17
      crew that they should hammer in the lower section of theirs.
       
      The following animation made from a detail from Figure 6-13 in the Apollo 16
        Preliminary Science Report and a detail from an LROC image M142164190RC,
      taken with the Sun only 31 degrees east of the zenith, shows the
      layout of the site near the LM.  North is up.  
      
    

    
    
| With the Sun near the zenith,
              variations in surface brightness in the LROC image are
              small.  Contrast adjustments made to bring out
              details makes the soil the astronauts disturbed around the
              LM nearly black.  The flag shadow northwest of the LM
              is well defined.  The crater immediately east of the
              LM has a diameter of about 25 meters. | 
    

    
| This stack displays the seven
              LROC images details used to make the animation at the top
              of the page.  The vertical yellow lines approximate
              the east-west location of the flagpole. In the early
              morning images at the top of the stack, the flag shadows
              start from points west of the flagpole and end farther
              west.  The situation is reversed for the late
              afternoon images at the bottom of the stack. | 

| Flag assembly prior to
              deployment.  The upper part of the flagpole is at the
              top, with the support rod for the top of the flag attached
              by a latching hinge at the right.  The bottom section
              of the pole is below those two items.  The portion of
              the bottom section that is pushed or hammered into the
              surface on on the right, with two short knurled sections
              indicating how far the pole should be pushed in for
              adequate stability. | 
    
The flag height depended upon how far
      the pole could be placed into the regolith, which varied from
      mission to mission. Assuming vertical deployment of a flat
      surface, with the flagpole 87 inches from the ground to the top of
      the pole and the bottom hem of the flag 50 inches above the
      ground, for the near sunrise image (8 degree solar elevation), the
      nearest part of the shadow would be 356 inches (9.0 meters) from
      the flagpole and the farthest part would be 619 inches (15.7
      meters) away.
    
| Journal Home Page | Apollo 16 Journal |