October 1951 | Kadena AFB, Okinawa
3. Date
te Metgnar a
_ocal,
|
S. HoT ot rT Rr
10. |
| | SHE CASH FILE.
_ Mil
O Al=Vi ol
| & SOURCE
1 = Ly.
_ba dena AM FP 5
| §
~
m
0Q
>
AJ
o
O
>
a
oC
= An: ane BA
GM
October 1951 | Terre Haute, Indiana
JECT 10073 RECORD CARD
“12. cConcLusions |
ry O Wos Bolloon
| Terre Haute, Indiana 0 Probably Balloon
Eg TYPE OF ERAT = 0 Possibly Balloon
2 Ground- Visual O Ground-Rodor Wos Aiicroft
a
O P
GM
OCR recovered text quality varies — view PDF for accurate reading.
ce EE TE _
PROJECT 10073 RECORD CARD
a
CONCLUS ION 5
po
a
0
n
>
=
0
z
M
Wos Balloon l
Probably Belloon |
Possibly Ballaon
| | 28 Sep—9 0 Oct Douglasville, Georgia
ooo
DATE-TIME GROUP d. TYPE OF OBSERYATION
| | BH Ground: Visual
0 Ai=Yi su ol
18. SOURCE
GMT — _
| 5. PHOTOS
0D Ground-Radar
O Air-lntercep! Rader
(ret) & Civilian
og ooo
7. LENGTH OF OBSERVATION | 8. NUMBER OF OBJECTS
9, COURSE
Was Alicralt
Probably Aireralt
Possibly Aireraht
Wos Astronomicol |
Probobly Astronomical
Possibly Astronomicol
Dither__
Insufficient Data lor Evaluation |
LI rile mre wen |
| different for
3-4 hrs three | each object |
ooo
10. BRIEF SUMMARY OF SIGHTING 11. COMMENTS
| 3 objects were observed at different times. Descriptions, motions
{Object nrs 1 end 3 initially observed at same terist: the ob; I sd by the
time. Object nr 2 observed aprox 3 to 4 hrs | witnesses fit such astroncmical objects
later, on 28, 29, 30 Sep and 1 end 9 Oct. as planets and stars. An example is the
Objects much brighter than any star, possibly ge object fits in et ay tl lane
0 times brighter than evening star. Path of Jupiter. From the available informatic
|all objects vas avay from obsdrver in general it is impossible to determin
straight dance-like | + ut in
— nce-like | Lg agraniy
|
ATIC FORM 329 (REV 16 sep 57)