Tag Archive for 'Gemini Observatory'

A 5-light-year-long section of the western wall in the Carina Nebula, as observed with adaptive optics on the Gemini South telescope. This mountainous section of the nebula reveals a number of unusual structures including a long series of parallel ridges that could be produced by a magnetic field, a remarkable almost perfectly smooth wave, and fragments that appear to be in the process of being sheared off the cloud by a strong wind. There is also evidence for a jet of material ejected from a newly-formed star. The exquisite detail seen in the image is in part due to a technology known as adaptive optics, which resulted in a ten-fold improvement in the resolution of the research team’s observations. Image credit: International Gemini Observatory / NOIRLab / NSF / AURA / Patrick Hartigan, Rice University / Travis Rector, University of Alaska Anchorage / Mahdi Zamani / Davide de Martin.

Astronomers Capture Best Ever Image of Carina Nebula’s Western Wall

Oct 6, 2020 by News Staff

Astronomers using twin 8.1-m telescopes at Gemini Observatory in Chile have captured the most detailed near-infrared image yet of the Carina Nebula’s...

These images of comet C/2020 F3 (NEOWISE) were obtained with the Gemini North telescope on August 1, 2020. Image credit: Gemini Observatory / NOIRLab / NSF / AURA / M. Drahus / P. Guzik.

Astronomers See Spirals in Gaseous Coma of Comet NEOWISE

Aug 31, 2020 by News Staff

New images of comet NEOWISE (C/2020 F3) show rapidly expanding spiral features in its coma produced by the rotation of its 5-km (3-mile) wide nucleus. These...

SDSS J141637.44+003352.2, a dual quasar at a distance for which the light reaching us was emitted 4.6 billion years ago. The two quasars are 13,000 light-years apart on the sky, placing them near the center of a single massive galaxy that appears to be part of a group, as shown by the neighboring galaxies in the left panel. In the lower panels, optical spectroscopy has revealed broad emission lines associated with each of the two quasars, indicating that the gas is moving at thousands of kilometers per second in the vicinity of two distinct supermassive black holes. The two quasars are different colors, due to different amounts of dust in front of them. Image credit: Silverman et al, doi: 10.3847/1538-4357/aba4a3.

Astronomers Find Three Luminous Dual Quasars

Aug 27, 2020 by News Staff

Using the Subaru Telescope and W. M. Keck and Gemini observatories, astronomers have spotted three dual quasars — merging galaxy systems that have...

The afterglow of GRB 181123B (marked with a circle), captured by the Gemini-North telescope. Image credit: Gemini Observatory / NOIRLab / NSF / AURA / K. Paterson & W. Fong, Northwestern University / Travis Rector, University of Alaska Anchorage / Mahdi Zamani / Davide de Martin.

Short Gamma-Ray Burst Localized to Extremely Distant Galaxy

Jul 16, 2020 by News Staff

An international of astronomers has observed an optical afterglow of a short gamma-ray burst, thought to be from the merger of two neutron stars, and localized...

This image shows Jupiter’s Great Red Spot. Image credit: NASA / ESA / M.H. Wong, University of California, Berkeley.

Juno, Hubble, Gemini Observatory Probe Jovian Storm Systems

May 8, 2020 by News Staff

Multiwavelength observations from the NASA/ESA Hubble Space Telescope and Gemini Observatory combined with close-up views from NASA’s Juno spacecraft...

This image, taken by the Gemini Multi-Object Spectrograph on the Gemini South telescope on Cerro Pachón in Chile, shows the planetary nebula CVMP 1. Image credit: Gemini Observatory / NSF’s National Optical-Infrared Astronomy Research Laboratory / AURA.

Astronomers Snap Photo of Beautiful Planetary Nebula

Feb 27, 2020 by News Staff

Astronomers using the Gemini South telescope on the summit of Cerro Pachon in Chile have taken a picture of CVMP 1, a planetary nebula located some 6,500...

This image, taken by the Gemini Multi-Object Spectrograph on the Frederick C. Gillett Gemini North telescope, shows the interacting galaxy pair NGC 5394-NGC 5395. Image credit: NSF’s National Optical-Infrared Astronomy Research Laboratory / Gemini Observatory / AURA.

Gemini North Telescope Captures Stunning Galaxy Collision

Dec 13, 2019 by Enrico de Lazaro

Astronomers working at the NSF-supported Gemini Observatory have captured a new photo of interacting spiral galaxies NGC 5394 and NGC 5395, collectively...

Voyager 2 image of Triton showing the south polar region with dark streaks produced by geysers visible on the icy surface. Image credit: NASA / JPL.

Astronomers Find Exotic Ices on Neptune’s Moon Triton

May 24, 2019 by News Staff

In the lab, scientists have pinpointed a specific wavelength of infrared light absorbed when molecules of carbon monoxide and nitrogen join together and...

Color composite image of the globular cluster HP 1 obtained using the Gemini-South telescope in Chile. Image credit: Gemini Observatory / AURA / NSF / Mattia Libralato, Space Telescope Science Institute.

HP 1: One of Milky Way’s Oldest Star Clusters Discovered

Mar 25, 2019 by News Staff

A team of astronomers using the Gemini-South telescope has discovered one of the oldest stellar clusters in the Milky Way. The team’s results date the...

This composite, false-color infrared image of Jupiter reveals haze particles over a range of altitudes, as seen in reflected sunlight. It was taken using the Gemini North telescope’s Near-InfraRed Imager (NIRI) on May 18, 2017. The multiple filters corresponding to each color used in the image cover wavelengths between 1.69 microns and 2.275 microns. Jupiter’s Great Red Spot (GRS) appears as the brightest (white) region at these wavelengths, which are primarily sensitive to high-altitude clouds and hazes near and above the top of Jupiter's convective region. The GRS is one of the highest-altitude features in Jupiter’s atmosphere. Narrow spiral streaks that appear to lead into it or out of it from surrounding regions probably represent atmospheric features being stretched by the intense winds within the GRS, such as the hook-like structure on its western edge (left side). Some are being swept off its eastern edge (right side) and into an extensive wave-like flow pattern, and there is even a trace of flow from its northern edge. Other features near the GRS include the dark block and dark oval to the south and the north of the eastern flow pattern, respectively, indicating a lower density of cloud and haze particles in those locations. Both are long-lived cyclonic circulations, rotating clockwise -- in the opposite direction as the counterclockwise rotation of the GRS. A prominent wave pattern is evident north of the equator, along with two bright ovals, which are anticyclones that appeared in January 2017. Both the wave pattern and the ovals may be associated with an impressive upsurge in stormy activity that has been observed in these latitudes this year. Another bright anticyclonic oval is seen further north. High hazes are evident over both polar regions with much spatial structure not previously been seen quite so clearly in ground-based images. Image credit: Gemini Observatory / AURA / NASA / JPL-Caltech.

Infrared Images of Jupiter from Subaru and Gemini Telescopes to Enhance Juno Flyby

Jul 4, 2017 by News Staff

High-resolution imaging of Jupiter and its Great Red Spot by the Subaru Telescope and the Gemini North telescope, both on Hawaii’s Mauna Kea peak, is...

Gemini Observatory Captures Sharpest-Ever Ground-Based Image of Pluto and Charon

Sep 27, 2012 by News Staff

Using a method called reconstructive speckle imaging, a team of astronomers at the Gemini Observatory has captured the sharpest ground-based image ever...

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