*Credit:* NASA [ http://www.nasa.gov/], ESA [ http://www.spacetel…], L. Sromovsky (University of Wisconsin, Madison), H. Hammel (Space Science Institute), and K. Rages (SETI)
Acknowledgement
*Credit:* NASA [ http://www.nasa.gov/], ESA [ http://www.spacetel…], L. Sromovsky (University of Wisconsin, Madison), H. Hammel (Space Science Institute), and K. Rages (SETI)
Acknowledgement
Fast Facts:
Technical facts about this news release:
About the Object Object Name: Uranus Object Description: Planet Distance: The semi-major axis of Uranus's orbit about the sun is 19.18 Astronomical Units (A.U.) or roughly 2.9 billion km. Dimensions: Uranus (without rings) has a diameter of roughly 32,000 miles (51,000 km) at the equator. About the Data Data Description: This image was created from HST data from the following proposal 10805: PI: L. Sromovsky (University of Wisconsin, Madison), H. Hammel (Space Science Institute), and K. Rages (SETI Institute). Instrument: ACS/WFC Exposure Date(s): July 26, 2006 Filters: FR782N at 750nm, 770 nm, and 790 nm About the Image Image Credit: NASA, ESA, and L. Sromovsky (University of Wisconsin, Madison) Release Date: August 31, 2006 Colors This image is a composite of many separate exposures made by the ACS instrument on the Hubble Space Telescope. A single ramp filter was used to sample several wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: FR782N @750 nm blue FR782N @770 nm green FR782N @790 nm red Orientation/Scale: Uranus and Ariel - 2006 - Annotated [ http://imgsrc.hubbl…]
Fast_Facts
Technical facts about this news release:
About the Object Object Name: Uranus Object Description: Planet Distance: The semi-major axis of Uranus's orbit about the sun is 19.18 Astronomical Units (A.U.) or roughly 2.9 billion km. Dimensions: Uranus (without rings) has a diameter of roughly 32,000 miles (51,000 km) at the equator. About the Data Data Description: This image was created from HST data from the following proposal 10805: PI: L. Sromovsky (University of Wisconsin, Madison), H. Hammel (Space Science Institute), and K. Rages (SETI Institute). Instrument: ACS/WFC Exposure Date(s): July 26, 2006 Filters: FR782N at 750nm, 770 nm, and 790 nm About the Image Image Credit: NASA, ESA, and L. Sromovsky (University of Wisconsin, Madison) Release Date: August 31, 2006 Colors This image is a composite of many separate exposures made by the ACS instrument on the Hubble Space Telescope. A single ramp filter was used to sample several wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: FR782N @750 nm blue FR782N @770 nm green FR782N @790 nm red Orientation/Scale: Uranus and Ariel - 2006 - Annotated [ http://imgsrc.hubbl…]
Fast Facts
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*Image Type:*: Astronomical
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*Image Type:*: Astronomical
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*Release Date*:August 31, 2006 01:00 PM (EDT)
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*Release Date*:August 31, 2006 01:00 PM (EDT)
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*News Release Number:*: STScI-2006-42a
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*News Release Number:*: STScI-2006-42a
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*Title*:Hubble Captures a Rare Eclipse on Uranus
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*Title*:Hubble Captures a Rare Eclipse on Uranus
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*Description*:
This image is a never-before-seen astronomical alignment of a moon traversing the face of Uranus, and its accompanying shadow. The white dot near the center of Uranus' blue-green disk is the icy moon Ariel. The 700-mile-diameter satellite is casting a shadow onto the cloud tops of Uranus. To an observer on Uranus, this would appear as a solar eclipse, where the moon briefly blocks out the Sun as its shadow races across Uranus's cloud tops.
Though such "transits" by moons across the disks of their parents are commonplace for some other gas giant planets, such as Jupiter, the satellites of Uranus orbit the planet in such a way that they rarely cast shadows on the planet's surface. Uranus is tilted so that its spin axis lies nearly in its orbital plane. The planet is essentially tipped over on its side. During the course of its orbit around the Sun, first one pole and then the other is alternately illuminated. As a result, Uranus has extreme seasons during its 84-year orbit around the Sun. The moons of Uranus orbit the planet above the equator, so their paths align edge-on to the Sun only every 42 years.
This transit has never been observed before because Uranus is just now approaching its 2007 equinox when the Sun will shine directly over the giant planet's equator. The last time a Uranian equinox occurred, when transits could have been observed, was in 1965. However, telescopes of that era did not have the image sharpness required to view satellite transits on Uranus. When Hubble was launched in 1990, the Sun was shining over Uranus's far northern latitudes. Over the past decade Hubble astronomers have seen the Sun's direct illumination creep toward equatorial latitudes and the moons' orbits approach an edge-on configuration.
Ariel, named for a mischievous airy spirit in Shakespeare's "The Tempest," is only one-third the size of Earth's moon. Ariel is the nearest large satellite to Uranus. As Uranus approaches equinox, there will be additional eclipses by the large moons Umbriel, Titania, and Oberon, and by many smaller moons.
Lawrence A. Sromovsky of the University of Wisconsin-Madison, Heidi B. Hammel of the Space Science Institute, Boulder, Colorado, and Kathy A. Rages of the SETI Institute, Mountain View, California, created this color composite image from images at three wavelengths in near infrared light obtained with Hubble's Advanced Camera for Surveys on July 26, 2006.
For more information, contact:
Ray Villard Space Telescope Science Institute, Baltimore, Md. (Phone: 410-338-4514; E-mail: villard@stsci.edu)
Terry Devitt University of Wisconsin, Madison, Wis. (Phone: 608-262-8282; trdevitt@wisc.edu)
Lawrence Sromovsky University of Wisconsin, Madison, Wis. (Phone: 608-263-6785; lsromovsky@ssec.wisc .edu)
Heidi Hammel Space Science Institute, Boulder, Colo. (Phone: 203-438-3506; hbh@alum.mit.edu)
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*Description*:
This image is a never-before-seen astronomical alignment of a moon traversing the face of Uranus, and its accompanying shadow. The white dot near the center of Uranus' blue-green disk is the icy moon Ariel. The 700-mile-diameter satellite is casting a shadow onto the cloud tops of Uranus. To an observer on Uranus, this would appear as a solar eclipse, where the moon briefly blocks out the Sun as its shadow races across Uranus's cloud tops.
Though such "transits" by moons across the disks of their parents are commonplace for some other gas giant planets, such as Jupiter, the satellites of Uranus orbit the planet in such a way that they rarely cast shadows on the planet's surface. Uranus is tilted so that its spin axis lies nearly in its orbital plane. The planet is essentially tipped over on its side. During the course of its orbit around the Sun, first one pole and then the other is alternately illuminated. As a result, Uranus has extreme seasons during its 84-year orbit around the Sun. The moons of Uranus orbit the planet above the equator, so their paths align edge-on to the Sun only every 42 years.
This transit has never been observed before because Uranus is just now approaching its 2007 equinox when the Sun will shine directly over the giant planet's equator. The last time a Uranian equinox occurred, when transits could have been observed, was in 1965. However, telescopes of that era did not have the image sharpness required to view satellite transits on Uranus. When Hubble was launched in 1990, the Sun was shining over Uranus's far northern latitudes. Over the past decade Hubble astronomers have seen the Sun's direct illumination creep toward equatorial latitudes and the moons' orbits approach an edge-on configuration.
Ariel, named for a mischievous airy spirit in Shakespeare's "The Tempest," is only one-third the size of Earth's moon. Ariel is the nearest large satellite to Uranus. As Uranus approaches equinox, there will be additional eclipses by the large moons Umbriel, Titania, and Oberon, and by many smaller moons.
Lawrence A. Sromovsky of the University of Wisconsin-Madison, Heidi B. Hammel of the Space Science Institute, Boulder, Colorado, and Kathy A. Rages of the SETI Institute, Mountain View, California, created this color composite image from images at three wavelengths in near infrared light obtained with Hubble's Advanced Camera for Surveys on July 26, 2006.
For more information, contact:
Ray Villard Space Telescope Science Institute, Baltimore, Md. (Phone: 410-338-4514; E-mail: villard@stsci.edu)
Terry Devitt University of Wisconsin, Madison, Wis. (Phone: 608-262-8282; trdevitt@wisc.edu)
Lawrence Sromovsky University of Wisconsin, Madison, Wis. (Phone: 608-263-6785; lsromovsky@ssec.wisc .edu)
Heidi Hammel Space Science Institute, Boulder, Colo. (Phone: 203-438-3506; hbh@alum.mit.edu)
