Skip to main content

Subaru Telescope can now Analyze 2,400 Galaxies Simultaneously

First light is an exciting time for astronomers and engineers who help bring new telescopes up to speed. One of the most recent and significant first light milestones recently occurred at the Subaru Telescope in Hawai’i. Though it has been in operation since 2005, the National Astronomical Observatory of Japan’s (NAOJ) main telescope recently received an upgrade that will allow it to simultaneously observe 2400 astronomical objects at once over a patch of sky the size of several moons.

Those 2400 objects will be observed by the Prime Focus Spectrograph (PFS), which itself has multiple subcomponents and was developed by around a dozen universities and companies on four continents. Its major components consist of a “Prime Focus Instrument,” which contains 2400 individual fibers and lets it concentrate on various parts of the sky. Data from those fibers is then fed to a Spectrograph System (SpS), which analyzes it to produce the data used in scientific papers.

The SpS consists of four separate spectrographs, covering spectra from the ultraviolet to the near-infrared, much more than a human eye can take in alone. Or, as a press release from NAOJ puts it more poetically, it covers “one and a half rainbows.” 

Presentation on how to use the PFS in cosmology.
Credit – ESO (ASIAA) YouTube Channel / Ryu Makiya

Unfortunately, these sensitive instruments won’t usually be used to capture rainbows, but theoretically, the Wide Field Corrector could. It is a seven-lens optical system developed specifically for this upgrade that allows Subaru’s operators to correct for errors in image collection before they become a problem.

There are also some supporting systems to enable the actual data collection to take place. n addition to the SpS, the PFS utilizes a giant 8960 x 5778 pixel CMOS camera known as the Metrology Camera System to track where precisely the fibers collecting the data are located. If any are out of place, it could throw off the data the system collects. 

All of these upgrades come with high hopes – the goal of the PFS upgrade is literally to understand where the universe came from and where it’s going. It will coordinate with the Hyper Suprime-Cam already installed in an effort to “reveal the nature of dark matter and dark energy, structure formation in the universe, and the physical processes of galaxy formation and evolution.

Take a virtual tour of the Subaru telescope.
Credit – SCExAO YouTube Channel

That’s a lot for one telescope upgrade, but it will surely have lots of data to analyze. Maybe the team could implement an eyepiece to attach to the PFS before it starts collecting data like it did when the telescope was first commissioned back in 2005. Potentially, the team that worked so hard on it could even actually see some rainbows then.

Learn More:
NAOJ – 2400 New Eyes on the Sky to See Cosmic Rainbows
Prime Focus Spectrograph
UT – Astronomers set a new Record and Find the Farthest Galaxy. Its Light Took 13.4 Billion Years to Reach us
UT – Subaru Telescope Sees 1800 Supernovae

Lead Image:
Image of the PFS mounted on the telescope.
Credit – Kavli IPMU

The post Subaru Telescope can now Analyze 2,400 Galaxies Simultaneously appeared first on Universe Today.



from Universe Today https://ift.tt/mD5dpXF
via IFTTT

Comments

Popular posts from this blog

SETI Researchers Double-Checked 1 Million Objects for Signs of Alien Signals

We can’t help ourselves but wonder about life elsewhere in the Universe. Any hint of a biosignature or even a faint, technosignature-like event wrests our attention away from our tumultuous daily affairs. In 1984, our wistful quest took concrete form as SETI, the Search for Extraterrestrial Intelligence . Unfortunately, or maybe fortunately, SETI has turned up nothing. Recently, scientists used a powerful new data system to re-examine data from one million cosmic objects and still came up empty-handed. Did they learn anything from this attempt? This effort used COSMIC , which stands for  Commensal Open-Source Multimode Interferometer Cluster . It’s a signal-processing and algorithm system attached to the Karl G. Jansky  Very Large Array  (VLA) radio astronomy observatory. According to SETI, it’s designed to “search for signals throughout the Galaxy consistent with our understanding of artificial radio emissions. “ Modern astronomy generates vast volumes of data and al...

A Magnetohydrodynamic Drive Could Lead to Fuel Stations on Mars

Within the next fifteen years, NASA, China, and SpaceX plan to send the first crewed missions to Mars. In all three cases, these missions are meant to culminate in the creation of surface habitats that will allow for many returns and – quite possibly – permanent human settlements. This presents numerous challenges, one of the greatest of which is the need for plenty of breathable air and propellant. Both can be manufactured through electrolysis, where electromagnetic fields are applied to water (H 2 O) to create oxygen gas (O 2 ) and liquid hydrogen (LH 2 ). While Mars has ample deposits of water ice on its surface that make this feasible, existing technological solutions fall short of the reliability and efficiency levels required for space exploration. Fortunately, a team of researchers from Georgia Tech has proposed a “ Magnetohydrodynamic Drive for Hydrogen and Oxygen Production in Mars Transfer ” that combines multiple functionalities into a system with no moving parts. This syst...

Do Dwarf Galaxies Merge In The Milky Way's Halo?

Our current understanding of the Cosmos shows that structures emerge hierarchically. First there are dark matter densities, then dwarf galaxies. Those dwarfs then merge to form more massive galaxies, which merge together into even larger galaxies. Evidence of dwarf galaxy mergers is difficult to obtain, but new research found some in the Milky Way's halo. from Universe Today https://ift.tt/DXpfOim via IFTTT