Subaru Telescope

Jupiter's Moon Had A Far-Flung Past
Jupiter's Moon Had A Far-Flung Past December 23, 2004
Jupiter's Moon Had A Far-Flung Past
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The first ground based infrared spectrum of Jupiter's moon Amalthea reveals that it must have formed far from its current location. This new result, based on observations with the Subaru telescope and the NASA Infrared Telescope Facility by a team of researchers from the National Astronomical Observatory of Japan, the University of Hawaii, and the University of Tokyo, sheds new light on our Solar System's turbulent past.
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The Soot Enshrouded End of a Sun-like Star
The Soot Enshrouded End of a Sun-like Star December 15, 2004
The Soot Enshrouded End of a Sun-like Star
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The Coronagraphic Imager with Adaptive Optics (CIAO) on the Subaru telescope captured this near-infrared (wavelengths of 1.25 - 2.2 microns) image of a star at the end of its life. BD +303639 is a planetary nebula, similar to the Ring Nebula in the constellation Lyra, the Harp. It is about five thousand light years from Earth in the direction of the constellation Cygnus, the Swan.
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Subaru Witnesses Galactic Cannibalism in Action
Subaru Witnesses Galactic Cannibalism in Action November 18, 2004
Subaru Witnesses Galactic Cannibalism in Action
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Subaru telescope has witnessed a large galaxy in the act of devouring a small companion galaxy in a new image obtained by Yoshiaki Taniguchi (Tohoku University), Shunji Sasaki (Tohoku University), Nick Scoville (California Institute of Technology) and colleagues. The evidence is a wispy band of stars extending over 500 thousand light years, the faintest and longest known example of its kind.

Image (72dpi, 196 KB)
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Belts of Planetesimals Discovered around Beta Pictoris
Belts of Planetesimals Discovered around Beta Pictoris October 21, 2004
Belts of Planetesimals Discovered around Beta Pictoris
Reveals an Early Extrasolar Planetary System
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A team of researchers from Ibaraki University, ISAS, University of Tokyo, and National Astronomical Observatory of Japan has succeeded in revealing details of the dust disk around beta Pictoris, which shows evidence of a planetary system. The team concludes that there is a "grain replenishment region" consisting of ring or belt like distribution of rocky bodies called planetesimals.
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Dwarf Irregular Galaxies: Not So Pristine After All
Dwarf Irregular Galaxies: Not So Pristine After All August 05, 2004
Dwarf Irregular Galaxies: Not So Pristine After All
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Astronomers have shown for the first time that even the smallest galaxies in the Universe have complex structures that indicate a complex history. Using the Subaru Telescope, a team of astronomers from the National Astronomical Observatory of Japan, the Institute of Physics in Lithuania, the University of Durham, Paris Observatory, Kyoto University, Gunma Astronomical Observatory, and the University of Tokyo have discovered an extended halo of stars with a sharp cutoff in the dwarf irregular galaxy Leo A, a member of the Local Group of galaxies that includes the Milky Way.
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Winds Measured on Saturn's Moon Titan to Help Robot Lander
Winds Measured on Saturn's Moon Titan to Help Robot Lander June 29, 2004
Winds Measured on Saturn's Moon Titan to Help Robot Lander
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On top the windswept summit of a Hawaiian volcano, a NASA instrument attached to the Japanese Subaru telescope measured distant winds raging on a strange world -- Titan, the giant moon of Saturn -- to help the robotic Huygens probe as it descends through Titan's murky atmosphere next January.
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Welcome to a Menagerie of a Million Galaxies
Welcome to a Menagerie of a Million Galaxies June 1, 2004
Welcome to a Menagerie of a Million Galaxies
Subaru/XMM-Newton Deep Survey Team Releases Data to the Public
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At a press conference held on 3 PM (JST), June 1, 2004, in Tokyo Japan, the National Astronomical Observatory of Japan (NAOJ) unveiled visible, X-ray, and radio wavelength images of the Subaru/XMM-Newton Deep Survey, based on data from the Subaru telescope, the European Space Agency's (ESA) XMM-Newton satellite and the Very Large Array. SXDS provides a comprehensive population census of galaxies from the early Universe to the present.
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Spiral Dance in a Planetary Nursery
Spiral Dance in a Planetary Nursery April 18, 2004
Spiral Dance in a Planetary Nursery
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New high resolution near-infrared direct imaging of the protoplanetary disk surrounding the star AB Aurigae shows that this planetary nursery is not the comparatively featureless and smooth place that astronomers had once assumed, but a place where gas and dust swirl in a complex spiral pattern. The new observations are part of a project to study the immediate neighborhood of young stars with greater detail than ever before by combining the large 8.2 meter effective aperture of the Subaru telescope with adaptive optics and a coronagraphic imager.
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Discovery of Water Icy Grains in Comet LINEAR Approaching Earth
Discovery of Water Icy Grains in Comet LINEAR Approaching Earth April 4, 2004
Discovery of Water Icy Grains in Comet LINEAR Approaching Earth
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Near infrared spectroscopic observation of Comet LINEAR (C/2002T7), which will approach the Earth in May 2004 and it is expected to be very bright, was carried out with the Subaru Telescope in September 2003. After analyzing the spectral data, we discovered water icy grains in the coma of Comet LINEAR. Comet Hale-Bopp is the first example of the detection of water icy grains in a cometary coma, and this time is the second one.
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A Treasure Chest of Stars -- Dwarf Irregular Galaxy Sextans A
A Treasure Chest of Stars February 23, 2004
A Treasure Chest of Stars -- Dwarf Irregular Galaxy Sextans A

Young blue stars and older yellow and red stars shine against a dark sky like jewels in a treasure chest in this image of Sextans A from Subaru Telescope’s prime focus camera Suprime-Cam. Sextans A is a dwarf irregular galaxy belonging to a group of galaxies called the Antlia-Sextans group 5 million light years from Earth. Even though five million light years is quite distant, only about 40 galaxies are closer to our own Milky Way galaxy than Sextans A. The Antlia-Sextans group is the closest neighbor of the Local Group..

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