Lucifer Telescope & The Vatican

NOTE: It just so happens that the only way to view some of the “objects” on the way to earth is via infrared. The Vatican seems to show the most interest in tracking these objects. For those of you questioning the role the Vatican will play, and why they have begun to speak openly about “aliens” and the opportunity to baptize them, we highly recommend reading Tom Horn’s research on the subject.

L.U.C.I.F.E.R

The Vatican Observatory Research Group (VORG) operates the 1.8m Alice P. Lennon Telescope with its Thomas J. Bannan Astrophysics Facility, known together as the Vatican Advanced Technology Telescope (VATT), at the Mount Graham International Observatory (MGIO) in southeastern Arizona where sky conditions are among the best in the world and certainly the Continental United States.

IMAGE CREDIT: Red Ice Creations

The instrument on the Large Binocular Telescope is a powerful tool that will gain spectacular insights into the universe from the Milky Way to extremely distant galaxies. An instrument for the world’s largest optical telescope, the Large Binocular Telescope (LBT) on Mount Graham, allows astronomers to observe the faintest and most distant objects in the universe.

The first LUCIFER observations of star-forming regions are giving scientists an idea of the new instrument’s enormous potential. This image depicts a stellar nursery in the Milky Way about 8,000 light-years from Earth. Such clouds are typically opaque to visible light. However, infrared light detected by LUCIFER can penetrate the dust.

The LBT partners in the U.S., Germany, and Italy announced back in 2010 that the first of two new innovative near-infrared cameras/spectrographs for the LBT are available to astronomers for scientific observations at the telescope on Mount Graham in southeastern Arizona.

After more than a decade of design, manufacturing, and testing, the new instrument, dubbed “LUCIFER”, provides a powerful tool to gain spectacular insights into the universe from the Milky Way to extremely distant galaxies. An identical twin instrument will be installed as well.

“With the large light-gathering power of the LBT, astronomers are now able to collect the spectral fingerprints of the faintest and most distant objects in the universe,” said LBT director Richard Green, a professor of astronomy at the University of Arizona’s Steward Observatory.

LUCIFER and its twin are mounted at the focus points of the LBT’s two giant 27.6-foot-diameter (8.4 meters) telescope mirrors. Each instrument is cooled to -351 Fahrenheit (-213 Celsius) in order to observe in the near-infrared wavelength range. Near-infrared observations are essential for understanding the formation of stars and planets in our galaxy as well as revealing the secrets of the most distant and young galaxies.

LUCIFER’s innovative design allows astronomers to observe star-forming regions in unprecedented detail, which are commonly hidden by dust clouds. The instrument is remarkably flexible, combining a large field of view with a high resolution. It provides three exchangeable cameras for imaging and spectroscopy in different resolutions, according to observational requirements.

Astronomers use spectroscopy to analyze incoming light and answer questions such as how stars and galaxies formed and what composes them.