See NEAR during its Thurs. night Earth swingby

Joan and David Dunham (dunham@erols.com)
Wed, 21 Jan 1998 02:59:42 -0500

You might be able to see the Near Earth Asteroid Rendezvous (NEAR) 
interplanetary spacecraft as it swings by the Earth Thursday night 
and Friday morning.  You can generate your own topocentric ephemeris 
of NEAR at the "topocentric ephemeris for NEAR flyby" item that is 
available at the I.A.U. Minor Planet Center's Web site:

http://cfa-www.harvard.edu/cfa/ps/mpc.html

Topocentric ephemerides for NEAR for 32 locations around the world 
will also be posted on the following Web sites from which they can 
be downloaded: 

http://sd-www.jhuapl.edu/NEAR/             (NEAR site)
http://www.sky.net/~robinson/iotandx.htm   (IOTA lunar site)
http://www.anomalies.com/iota/splash.htm   (IOTA asteroidal site)

These have an improved format, with the time in hours and minutes, 
and with the Sun altitude given (with no lines when the Sun is above 
the horizon), that supersedes the ephemerides distributed to some 
of you yesterday.  In addition, data for January 23rd U.T. are now 
included, including the closest approach with the sunglint phase for 
the U.S.A. and after the closest approach for the Southern 
Hemisphere.  Later today, a more detailed "groundtrack" ephemeris 
(long., lat., and altitude) will be placed on the NEAR Web site 
covering the Sunglint times (Jan. 23, 6:24 - 6:50 U.T.) at one-
minute intervals.  The Sunglints, when NEAR will shine briefly about 
as bright as Capella for many regions of the U.S.A., are described 
in items on the IOTA and NEAR Web sites; timed observations of them
are sought to measure solar panel misalignments.  This evening, CNN 
plans to broadcast a short clip about NEAR's Earth swingby and the 
Sunglints, including an interview with me.  An improved local-time 
map of the U.S.A. showing the predicted track of the Sunglint is now 
on the NEAR Web site (although it has a few small errors in the city 
and timezone locations that we'll try to fix by late this afternoon).  
Skyviews locating the Sunglint for nine different regions are on the 
NEAR Web site, with one for Hawaii on the IOTA asteroidal site. 

There is a chart of Perseus, with north up, showing in more detail 
the location of NEAR during the Sunglint maneuvers for almost 40 
cities; it will help those using large binoculars or telescopes 
which, however, are not necessary; the glint should be easily 
visible with the naked eye.  Note that the Sunglint maneuvers are 
performed only by rotating the spacecraft slightly using momentum 
wheels, powered by the ample electricity available from the solar 
panels; there are no thrusting maneuvers using the spacecraft's fuel 
to accomplish these pointings.  They are a byproduct of a navigation 
test of the satellite. 

Most of the time, NEAR will not be reflecting Sunlight from its 
solar panels and will then be quite dim; see the geocentric 
ephemeris below.  The list of locations for which topocentric 
ephemerides have been computed are as follows: 

Location            Latitude  E. Longitude

AUCKLAND, N.Z.      -36.908   174.777
TOKYO, Japan        35.6605   139.7702
BRISBANE, Queens.   -27.516   153.070
MELBOURNE, Vict.    -37.75    145.0
NANKING, China       32.0666  118.8210
PERTH, W. Austrl.   -31.95    115.83
NAINI TAL, India    29.3608    79.4567
KODAIKANAL, India   10.2306    77.4686
MOSCOW, Russia      55.755     37.570
MITZPE RAMON,Isrl.  30.597     34.763
CAPE, S. Africa    -33.933     18.475
TIRGO Obs., Switz.  45.98447    7.79167
HERSTMONCEUX, UK    50.871      0.338
SAN FERNANDO, Spn.  36.462     -6.200
LA PALMA, CanaryIs  28.75833  -17.8800
RIO DE JANEIRO,Br. -22.8975   -43.18625
ST. JOHN'S, Nfld.   47.537    -52.753
CARACAS, Venezuela  10.5068   -66.928
SANTIAGO, Chile    -33.41833  -70.630
Boston, MA          42.3567   -71.0569
Chelmsford, MA      42.62     -71.39
Charlotte Hall, MD  38.51     -76.76
Miami FL            25.77667  -80.19167
near Chicago, IL    42.317    -88.00
Houston, Texas      29.6049   -95.1086  
Coal Creek Can.,CO  39.877   -105.391  
Mt. Hopkins, Ariz.  31.5647  -110.8846
Casa Grande, Ariz.  32.9583  -111.6542 
Los Angeles CA      34.05500 -118.24167
Seattle WA          47.60833 -122.33667
ANCHORAGE, Alaska   61.21    -149.87
Honolulu HI         21.30667 -157.86000

An abbreviated geocentric ephemeris of NEAR is given below.  The 
magnitude could be wrong by a few units; we hope to receive some 
observations soon so that it might be calibrated and updated.  A 
more detailed version of the geocentric ephemeris is on the IOTA 
lunar Web site.  Due to the relatively unfavorable phase angle after 
the closest approach (which occurs on 1998 Jan. 23, 7:23 U.T. over 
the Middle East, in daylight), NEAR will likely be much fainter than 
during its approach.  Also, after the swingby, you can see from the 
table below that NEAR will be visible only from southern-hemisphere 
observatories. 

 Geocentric ephemeris for NEAR from JPL ephemeris file p_tcm11_n0a
 generated 1998 Jan. 19

  Calendar           Solar         J2000       min.topo.
    Date       UTC   Elong.    R.A.      Dec.   Distance  NEAR
 Year Mo Day   h  m   deg.     deg.      deg.      km     Mag.

 1998 JAN 21  12:00 140.31  81.01973  21.19753   1097657  17.3
 1998 JAN 22   0:00 139.74  80.92815  21.42858    798920  16.7
 1998 JAN 22  12:00 139.10  80.73434  21.93338    499065  15.6
 1998 JAN 22  18:00 138.69  80.51496  22.50639    348217  14.9
 1998 JAN 22  20:00 138.52  80.39282  22.82385    297669  14.5
 1998 JAN 23   0:00 138.02  79.96055  23.93556    195848  13.6
 1998 JAN 23   2:00 137.59  79.51691  25.05603    144317  12.9
 1998 JAN 23   3:00 137.24  79.15099  25.96415    118277  12.5
 1998 JAN 23   4:00 136.70  78.57920  27.35372     91951  12.0
 1998 JAN 23   5:00 135.71  77.54841  29.76695     65184  11.2
 1998 JAN 23   5:30 134.80  76.63340  31.80984     51545  10.7
 1998 JAN 23   6:00 133.20  75.05630  35.11400     37647  10.0
 1998 JAN 23   6:10 132.35  74.23407  36.73016     32938   9.8
 1998 JAN 23   6:20 131.22  73.13511  38.78023     28182   9.4
 1998 JAN 23   6:30 129.65  71.58201  41.47221     23373   9.0
 1998 JAN 23   6:40 127.33  69.19788  45.17163     18509   8.5
 1998 JAN 23   6:50 123.60  65.01014  50.57217     13597   7.9
 1998 JAN 23   7:00 116.91  55.51731  59.04067      8687   6.9

 1998 JAN 23   7:40  46.40 255.52222 -34.21045      5871   6.9
 1998 JAN 23   7:50  54.21 247.58190 -47.43933     10697   8.1
 1998 JAN 23   8:00  59.34 241.27041 -54.45557     15620   8.8
 1998 JAN 23   8:30  67.14 227.87440 -63.41631     30142  10.1
 1998 JAN 23   9:00  70.69 219.29026 -66.74216     44221  10.9
 1998 JAN 23  10:00  74.10 209.08617 -69.31563     71530  11.9
 1998 JAN 23  12:00  76.79 199.60940 -70.80685    124420  13.1
 1998 JAN 23  15:00  78.35 193.72607 -71.40726    201865  14.1
 1998 JAN 23  18:00  79.11 190.90908 -71.61942    278269  14.8
 1998 JAN 24   0:00  79.89 188.16638 -71.78267    429611  15.7

David Dunham, NEAR Mission Design, 1998 Jan. 21, 8h U.T.