On February 1, 1994, a large meteoroid impacted over the Pacific Ocean
at 2.6 degrees N, 164.1 degrees E. The impact was observed by space b
ased IR sensors operated by the US Department of Defense and by visibl
e wavelength sensors operated by the US Department of Energy. During e
ntry the object broke into several pieces, one of which detonated at 3
4 km and another at 21 km altitude. The entry velocity of the object i
s estimated to be 24-25 km/sec. Based on the visible wavelength data,
the integrated intensity of the radiated energy of the fireball was ap
proximately 1.3 x 10(13) joules. Assuming a 6000 K black body and a 30
% efficiency for the conversion of the kinetic energy of the body into
visible light, we estimate the mass of the body to be between 1.6 x 1
0(5) kg and 4.4 x 10(6) kg, and to have a diameter of between 4.4 and
13.5 meters. The object entered at a 45 degrees angle, traveling on a
heading of approximately 300 degrees, i.e. from the southeast to the n
orthwest. Calculations using a gross-fragmentation model indicate that
the body was most likely a stony object larger than 10 m with an Apol
lo orbit prior to impact.