Astronomers have measured the most massive known black hole in our cosmic neighborhood by combining data from a giant telescope in Hawai'i and a smaller telescope in Texas.
On December 6-8, 2010 about a dozen representatives from AURA converged at Gemini’s base facility in Hilo, Hawai‘i to discuss a broad range of topics related to diversity in the workforce.
The composite image, taken on Nov. 18, 2010 by the Gemini North telescope in Hawaii, shows a belt that had previously vanished in Jupiter's atmosphere is now reappearing.
The discovery of an unusual stellar system combined with Gemini North NIRI observations has allowed astronomers to confirm the spectral type of a cool methane dwarf and determine its temperature, mass, and age with confidence.
Phillip Cargile (Vanderbilt University) and team take advantage of the time-dependent destruction of lithium in young stars to measure the age of the open cluster Blanco 1.
A pristine new coat of protected silver now glistens on the Gemini South primary mirror (M1) as part of a routine shut-down on Cerro Pachón in Chile.
A team of astronomers have discovered what is currently the coldest star-like object. The object, called UGPS J0722-05, is also of particular interest because it is one of our closest neighbors.
Amateur astronomers used high-speed, video-monitoring equipment to capture a fireball streaking through the atmosphere of Jupiter. Shortly thereafter, the world’s largest telescopes examined Jupiter for debris left behind.
Astronomers have used the Thermal-Region Camera Spectrograph (T-ReCS) on the Gemini South telescope to obtain the first resolved image of the debris disk around the 12 million year old star HD191089.
Cristina Ramos Almeida and collaborators obtained deep imaging data using the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope to study the morphologies of a complete sample of 46 intermediate redshift (0.05<z<0.7) PRGs.
Using NICI on the Gemini-South telescope in Chile, an international team led by University of Hawai‘i astronomers have directly imaged a brown dwarf in a tight orbit around a young Sun-like star.
The first two accepted papers based on observations with NICI at Gemini South include discoveries of several previously unknown companions in binary star systems as well as the study of the age distributions of stars in the outer regions of the galaxy M83.
A Canadian-U.S. team's analysis, based on follow-up observations using the Gemini North telescope and the Multiple-Mirror Telescope (MMT), shows a clear signature of a tidally destroyed dwarf planet that once orbited the parent star.
Using NIRI on the Gemini North telescope, James De Buizer and William Vacca (SOFIA-USRA) obtained spectra that, for the first time, directly identify the origin of “green fuzzy” emission.
Gemini Observatory aims to be one of the most energy efficient astronomical facilities, with the highest standards of environmental protection.
The discovery of a very young planet-like object, paired with a low-mass brown dwarf. appears to have formed in about a million years–more rapidly than some theories of planet formation predict.
A striking new Gemini Observatory image of the Owl Nebula, a prominent object visible in the northern sky, was released today (March 25, 2010) as the culmination of a nationwide student essay contest in Canada.
Barry Rothberg and Jacqueline Fischer of the Naval Research Lab find that IR-luminous mergers appear younger and less massive in the near-IR but indistinguishable from old, massive ellipticals at optical wavelengths.
A dramatic new image from the Gemini North telescope illustrates the dynamic and sometimes violent process of star birth. It also demonstrates the capabilities of new filters available to researchers using the GMOS.
Observations at the Gemini Observatory provide convincing new evidence that stellar heavyweights may be born in much the same manner as lightweights like our Sun.