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HD 129445
HD 129445
is a
G type
star
found in the
Circinus constellation
located
approximately
210
light-years
away
from
the Earth
. The star has been under the
Magellan Planet Search Program
observation due to its
absolute visual magnitude
and
metallicity
. The
Magellan
program
conducted
17
doppler velocity tests
which
spans
a
full
orbital period
. The results led
the program
to
detect
a planet
dubbed
HD 129445 b
whose
readings
was
accurate
to the
Keplerian orbital model
.