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STELLAR CHEMISTRY
Seeing the Whole Galaxy with a 'Second Eye on the Sky'
by Staff Writers
Baltimore MD (SPX) Mar 31, 2017


The "first light" observations for the APOGEE South spectrograph. The dots show stars whose spectra were observed by APOGEE. Some example spectra are shown (colors are representative only, as APOGEE spectra are in the infrared). The first light observations included spectra of supermassive stars in the Tarantula Nebula. This nebula in the Large Magellanic Cloud is forming stars more rapidly than any other region in our Local Group of galaxies. It can only be seen from the Southern Hemisphere, underscoring the importance of APOGEE South's location. The spectrograph will allow us to study the chemistry and evolution of the stars in the nebula in greater detail than ever before. Image courtesy SDSS collaboration; Tarantula Nebula image from Herschel/Spitzer

Earlier this month, the Sloan Digital Sky Survey (SDSS) reached an important milestone by opening its "second eye on the sky" - a new instrument called the "APOGEE South spectrograph." This new instrument at Las Campanas Observatory in Chile is the twin of the APOGEE North spectrograph, and will let astronomers study stars across the whole Milky Way like never before.

The name APOGEE is short for the Apache Point Observatory Galaxy Evolution Experiment, based on the location of the experiment's first "eye" at Apache Point Observatory, New Mexico. "The original APOGEE made history by measuring extremely detailed properties of more stars than ever before," said Steven Majewski of the University of Virginia, principal investigator of the APOGEE experiment.

"But we always wanted a more complete view, especially because the center of the galaxy is best seen from the Southern Hemisphere. With the APOGEE South spectrograph, we are finally realizing that vision." Data collected by the twin instruments will help astronomers make a map of the entire Milky Way, with an unprecedented combination of size and detail.

The APOGEE South spectrograph in Chile is identical to the original APOGEE spectrograph in New Mexico. Both work by spreading starlight into detailed rainbow patterns called "spectra." Astronomers use these spectra to determine the chemical compositions of those stars, and also to find subtle shifts due to the Doppler effect created by the stars' motion through space.

These pieces of information - composition and velocity - are combined with the known stellar positions to create an incredibly detailed map of our galaxy.

John Wilson of the University of Virginia, APOGEE's instrument scientist, explains the decision to build identical instruments in two hemispheres: "If the two spectrographs are exactly the same, then the spectra we collect from them will also be the same. We don't need to worry that differences we see are due to differences in instrument design. We can directly compare the parts of our galaxy we can see from the Northern and Southern Hemispheres."

The APOGEE experiment to date has measured more than one million spectra of 277,000 individual stars, making it the largest high-resolution, near-infrared spectroscopic sample of stars ever observed.

By working in infrared light, the APOGEE instruments can peer through the thick clouds of dust that obscure the inner Milky Way. By the end of APOGEE South's mission, the number of stars observed will double, resulting in the most complete map of the Milky Way ever created.

The new APOGEE South spectrograph is located at the Irenee du Pont Telescope at Las Campanas Observatory, located at an elevation of 2,400 meters (8,000 feet) in the Atacama Desert of Northern Chile - about the same distance south of the equator as the New Mexico site of the original APOGEE spectrograph is to the north.

"Looking from the Southern Hemisphere will allow us to study the innermost regions of our galaxy," said Manuela Zoccali of Pontifica Universidad Catolica de Chile and the Millennium Institute of Astrophysics, the chair of the SDSS Chilean Participation Group.

"This is the first time that a large team of Chileans has worked with colleagues around the world on such an ambitious project. We are pleased we can now work together on the first data."

The director of the SDSS-IV project, Michael Blanton of New York University, agrees. "Working with our colleagues in Chile has helped us extend our survey in exciting new ways. Ever since we began in 2000, people have asked us when we would go to the Southern Hemisphere. We are delighted to have found a second home at Las Campanas."

STELLAR CHEMISTRY
GUSTO Explorer Will Study Churning Chaos in Milky Way
Greenbelt MD (SPX) Mar 28, 2017
NASA has selected a science mission that will measure emissions from the interstellar medium, which is the cosmic material found between stars. This data will help scientists determine the life cycle of interstellar gas in our Milky Way galaxy, witness the formation and destruction of star-forming clouds, and understand the dynamics and gas flow in the vicinity of the center of our galaxy. ... read more

Related Links
Sloan Digital Sky Survey
Stellar Chemistry, The Universe And All Within It

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