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The ESO Releases the Most Detailed Infrared Map of our Galaxy Ever Made

October 1, 2024
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The ESO Releases the Most Detailed Infrared Map of our Galaxy Ever Made
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Regardless of a long time of large-scale optical surveys, there are nonetheless mysteries concerning the Milky Approach galaxy that astronomers are wanting to resolve. That is significantly true of its inner construction and the core area, which is troublesome to survey attributable to clouds of fuel and dirt within the interstellar medium (ISM). This materials absorbs seen gentle, making fainter objects troublesome to see in optical wavelengths. Fortunately, advances in infrared astronomy have enabled surveys of the Milky Approach which have revealed issues that will in any other case stay invisible to us.

For greater than 13 years, a world workforce of astronomers has been observing the Milky Approach utilizing the ESO’s 4.1-meter Visible and Infrared Survey Telescope for Astronomy (VISTA). In a recently published study, they introduced the discharge of their closing knowledge product: a huge infrared map of the Milky Approach containing greater than 1.5 billion objects—probably the most detailed map our galaxy has ever created! With over 200,000 photos and 500 terabytes of knowledge, this map can also be the biggest observational undertaking ever carried out with an ESO telescope.

Situated on the European Southern Observatory’s (ESO) Paranal Observatory in Chile, the VISTA telescope is chargeable for mapping giant areas of the sky. This newest map accommodates knowledge gathered by the VISTA Variables in the Via Lactea (VVV) survey and its companion undertaking, the VVV eXtended (VVVX) survey. Led by Dante Minniti, an astrophysicist at Universidad Andrés Bello in Chile, these surveys used the VISTA InfraRed CAMera (VIRCAM) to survey the Milky Approach, the Small and Massive Magellanic Clouds (SMC, LMC), and extragalactic house.

This spectacular view of the VISTA telescope was taken from the roof of the constructing throughout the opening of the enclosure at sundown. The VLT is seen on the neighboring mountain. Credit score: VVV Survey/ESO

This newest map accommodates about ten instances as many objects because the previous version, which the VVV Survey workforce launched in 2012. As all the time, the flexibility to see the Universe within the infrared wavelength permits astronomers to see objects that will in any other case be obscured by clouds of fuel and dirt. These embrace new child stars embedded in dusty globular clusters, brown dwarfs, and free-floating planets (FFP)—aka rogue planets—that don’t orbit stars. “We made so many discoveries, now we have modified the view of our Galaxy without end,” mentioned Minniti in a current ESO press release.

The observations started in 2010, utilizing the digicam’s 16 particular detectors with a mixed decision of 67 million pixels to survey billions of level sources of sunshine in an space measuring 520 deg2. By observing every patch of sky many instances, the workforce might decide the places and correct motions of the 1.5 billion objects and monitor them for modifications in brightness. The workforce additionally tracked hypervelocity stars kicked out of our galaxy’s central area attributable to gravitational interplay with the supermassive black gap (SMBH) there – Sagittarius A*.

The observations lasted for 420 nights, ending within the first half of 2023. The ensuing map supplies an correct 3D view of the Milky Approach’s interior areas that had been beforehand obscured by mud. With the surveys now full, the ESO’s Paranal Observatory is getting ready for future surveys by upgrading the VISTA with the 4-meter Multi-Object Spectrograph Telescope (4MOST) instrument. This new instrument will enable VISTA to carry out giant spectroscopic surveys, capturing the spectra of 2400 objects concurrently over an space of the sky equal to twenty full Moons.

In the meantime, the Very Massive Telescope (VLT) will obtain the brand new Multi-Object Optical and Near-infrared Spectrograph (MOONS) instrument. MOONS consists of two equivalent cryogenic spectrographs (with 500 fibers every), permitting astronomers to acquire optical and near-infrared spectra for about 1000 objects concurrently. The mixed energy of those devices will present spectra for thousands and thousands of the objects surveyed by VVV and VVX, and lots of extra discoveries are anticipated!

Additional Studying: ESO, Astronomy & Astrophysics

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