Initial data came from the TRENDS (TaRgetting bENchmark - objects with Doppler Spectroscopy) high - contrast imaging survey that uses adaptive optics and related technologies to target older,
faint objects orbiting nearby stars, and precise measurements were made at the W. M. Keck Observatory on the summit of Mauna Kea, Hawaii.
Not exact matches
XMM - Newton is on a distended
orbit that takes it one - third of the way to the moon; this keeps it out of Earth's shadow long enough to stay pointed at — and collecting photons from — the same
faint object for more than a day.
For example, an instrument on one satellite could block the glare of the sun or a distant star, making it possible for a camera on the other to image
faint objects such as the sun's ghostly corona or exoplanets
orbiting a star.
Ground - based and
orbiting telescopes employ exquisitely sensitive detectors to search for
objects that are much farther away, and much
fainter, than could have been detected just a few years ago.
David Jewitt of the University of Hawaii and Jane Luu, now at Stanford University, found a
faint slow - moving
object beyond the
orbit of Pluto a year ago, and a second in March.
Astronomers are stuck with such indirect methods of detection because current telescope technology struggles to image very distant and
faint objects - especially when they
orbit close to the glare of a star.