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Squeeky-bum-time now less squeeky...
- dmcdona
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15 years 2 months ago #81557
by dmcdona
Squeeky-bum-time now less squeeky... was created by dmcdona
Oct. 7, 2009
Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.brown@nasa.gov
DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov
RELEASE: 09-232
NASA REFINES ASTEROID APOPHIS' PATH TOWARD EARTH
PASADENA, Calif. -- Using updated information, NASA scientists have recalculated the path of a large asteroid. The refined path indicates a significantly reduced likelihood of a hazardous encounter with Earth in 2036.
The Apophis asteroid is approximately the size of two-and-a-half football fields. The new data were documented by near-Earth object scientists Steve Chesley and Paul Chodas at NASA's Jet Propulsion Laboratory in Pasadena, Calif. They will present their updated findings at a meeting of the American Astronomical Society's Division for Planetary Sciences in Puerto Rico on Oct. 8.
"Apophis has been one of those celestial bodies that has captured the public's interest since it was discovered in 2004," said Chesley.
"Updated computational techniques and newly available data indicate the probability of an Earth encounter on April 13, 2036, for Apophis has dropped from one-in-45,000 to about four-in-a million."
A majority of the data that enabled the updated orbit of Apophis came from observations Dave Tholen and collaborators at the University of Hawaii's Institute for Astronomy in Manoa made. Tholen pored over hundreds of previously unreleased images of the night sky made with the University of Hawaii's 88-inch telescope, located near the summit of Mauna Kea.
Tholen made improved measurements of the asteroid's position in the images, enabling him to provide Chesley and Chodas with new data sets more precise than previous measures for Apophis. Measurements from the Steward Observatory's 90-inch Bok telescope on Kitt Peak in Arizona and the Arecibo Observatory on the island of Puerto Rico also were used in Chesley's calculations.
The information provided a more accurate glimpse of Apophis' orbit well into the latter part of this century. Among the findings is another close encounter by the asteroid with Earth in 2068 with chance of impact currently at approximately three-in-a-million. As with earlier orbital estimates where Earth impacts in 2029 and 2036 could not initially be ruled out due to the need for additional data, it is expected that the 2068 encounter will diminish in probability as more information about Apophis is acquired.
Initially, Apophis was thought to have a 2.7 percent chance of impacting Earth in 2029. Additional observations of the asteroid ruled out any possibility of an impact in 2029. However, the asteroid is expected to make a record-setting -- but harmless -- close approach to Earth on Friday, April 13, 2029, when it comes no closer than 18,300 miles above Earth's surface.
"The refined orbital determination further reinforces that Apophis is an asteroid we can look to as an opportunity for exciting science and not something that should be feared," said Don Yeomans, manager of the Near-Earth Object Program Office at JPL. "The public can follow along as we continue to study Apophis and other near-Earth objects by visiting us on our AsteroidWatch Web site and by following us on the @AsteroidWatch Twitter feed."
The science of predicting asteroid orbits is based on a physical model of the solar system which includes the gravitational influence of the sun, moon, other planets and the three largest asteroids.
NASA detects and tracks asteroids and comets passing close to Earth using both ground and space-based telescopes. The Near Earth-Object Observations Program, commonly called "Spaceguard," discovers these objects, characterizes a subset of them and plots their orbits to determine if any could be potentially hazardous to our planet.
JPL manages the Near-Earth Object Program Office for NASA's Science Mission Directorate in Washington. Cornell University operates the Arecibo Observatory under a cooperative agreement with the National Science Foundation in Arlington, Va.
Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.brown@nasa.gov
DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov
RELEASE: 09-232
NASA REFINES ASTEROID APOPHIS' PATH TOWARD EARTH
PASADENA, Calif. -- Using updated information, NASA scientists have recalculated the path of a large asteroid. The refined path indicates a significantly reduced likelihood of a hazardous encounter with Earth in 2036.
The Apophis asteroid is approximately the size of two-and-a-half football fields. The new data were documented by near-Earth object scientists Steve Chesley and Paul Chodas at NASA's Jet Propulsion Laboratory in Pasadena, Calif. They will present their updated findings at a meeting of the American Astronomical Society's Division for Planetary Sciences in Puerto Rico on Oct. 8.
"Apophis has been one of those celestial bodies that has captured the public's interest since it was discovered in 2004," said Chesley.
"Updated computational techniques and newly available data indicate the probability of an Earth encounter on April 13, 2036, for Apophis has dropped from one-in-45,000 to about four-in-a million."
A majority of the data that enabled the updated orbit of Apophis came from observations Dave Tholen and collaborators at the University of Hawaii's Institute for Astronomy in Manoa made. Tholen pored over hundreds of previously unreleased images of the night sky made with the University of Hawaii's 88-inch telescope, located near the summit of Mauna Kea.
Tholen made improved measurements of the asteroid's position in the images, enabling him to provide Chesley and Chodas with new data sets more precise than previous measures for Apophis. Measurements from the Steward Observatory's 90-inch Bok telescope on Kitt Peak in Arizona and the Arecibo Observatory on the island of Puerto Rico also were used in Chesley's calculations.
The information provided a more accurate glimpse of Apophis' orbit well into the latter part of this century. Among the findings is another close encounter by the asteroid with Earth in 2068 with chance of impact currently at approximately three-in-a-million. As with earlier orbital estimates where Earth impacts in 2029 and 2036 could not initially be ruled out due to the need for additional data, it is expected that the 2068 encounter will diminish in probability as more information about Apophis is acquired.
Initially, Apophis was thought to have a 2.7 percent chance of impacting Earth in 2029. Additional observations of the asteroid ruled out any possibility of an impact in 2029. However, the asteroid is expected to make a record-setting -- but harmless -- close approach to Earth on Friday, April 13, 2029, when it comes no closer than 18,300 miles above Earth's surface.
"The refined orbital determination further reinforces that Apophis is an asteroid we can look to as an opportunity for exciting science and not something that should be feared," said Don Yeomans, manager of the Near-Earth Object Program Office at JPL. "The public can follow along as we continue to study Apophis and other near-Earth objects by visiting us on our AsteroidWatch Web site and by following us on the @AsteroidWatch Twitter feed."
The science of predicting asteroid orbits is based on a physical model of the solar system which includes the gravitational influence of the sun, moon, other planets and the three largest asteroids.
NASA detects and tracks asteroids and comets passing close to Earth using both ground and space-based telescopes. The Near Earth-Object Observations Program, commonly called "Spaceguard," discovers these objects, characterizes a subset of them and plots their orbits to determine if any could be potentially hazardous to our planet.
JPL manages the Near-Earth Object Program Office for NASA's Science Mission Directorate in Washington. Cornell University operates the Arecibo Observatory under a cooperative agreement with the National Science Foundation in Arlington, Va.
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- mjc
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15 years 2 months ago #81560
by mjc
Replied by mjc on topic Re:Squeeky-bum-time now less squeeky...
Very good.
Bit unfortunate that closest approach is on a "Fri 13th".
18,300 miles distant - two and half football fields - I assume that's American football - don't know how big they are.
Anyone got a ballpark angular size at closest approach?
I think I'll be too old to set-up a scope when that arrives.
Still could have been worse - closest approach could have been such that I would feel the heat on my cheeks as I hold out my hand to ward of the glare...
Mark
Bit unfortunate that closest approach is on a "Fri 13th".
18,300 miles distant - two and half football fields - I assume that's American football - don't know how big they are.
Anyone got a ballpark angular size at closest approach?
I think I'll be too old to set-up a scope when that arrives.
Still could have been worse - closest approach could have been such that I would feel the heat on my cheeks as I hold out my hand to ward of the glare...
Mark
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15 years 2 months ago - 15 years 2 months ago #81565
by michaeloconnell
Replied by michaeloconnell on topic Re:Squeeky-bum-time now less squeeky...
Good to hear that the asteroid is less of a threat.
On a separate note:
On a separate note:
Your personal hygiene is your own business Dave....:ohmy:Squeeky-bum-time now less squeeky...
Last edit: 15 years 2 months ago by michaeloconnell.
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- dmcdona
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15 years 2 months ago #81568
by dmcdona
Replied by dmcdona on topic Re:Squeeky-bum-time now less squeeky...
And with Mark mentioning "cheeks"... This could go downhill rapidly... Mods!
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15 years 2 months ago #81570
by mjc
Replied by mjc on topic Re:Squeeky-bum-time now less squeeky...
If I could piggy back a question here re asteroid work.
Is there an online resource where one can set a celestial coordinate, UTC time, and maybe field of view and determine what known solar system objects are known to be within the field of view - or maybe a list of closest objects.
For you asteroid hunters - how do you know that a suspected object is new or not?
And - no - I haven't got any faint spot on any image that I'm curious about - but maybe something for the future.
Mark
Is there an online resource where one can set a celestial coordinate, UTC time, and maybe field of view and determine what known solar system objects are known to be within the field of view - or maybe a list of closest objects.
For you asteroid hunters - how do you know that a suspected object is new or not?
And - no - I haven't got any faint spot on any image that I'm curious about - but maybe something for the future.
Mark
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15 years 2 months ago #81571
by dmcdona
Replied by dmcdona on topic Re:Squeeky-bum-time now less squeeky...
Mark - I'm not sure if there's an online resource but it seems most "asteroid hunters" use astrometrica (shareware but a lenghty 180 days before you get a nag screen. But its only €25 to buy).
Its takes a wee bit of time to set up the configuration file for your particular imaging setup (focal length, pixel size etc) but once done, you can open an image, specify the time/date if necessary (it'll take the time/date from a FITS header if theose fields are completed) and ask it to check for known objects. If your little dot doesn't show up as a known object, you have a potential candidate...
You just need to make sure to download the latest MPC catalogue of known objects. Astrometrica can be set to use the online USNO-B1.0 catalogue (for comparison star fields)so you don't even need to download that.
www.astrometrica.at/
If you need any help, just shout.
Dave
Its takes a wee bit of time to set up the configuration file for your particular imaging setup (focal length, pixel size etc) but once done, you can open an image, specify the time/date if necessary (it'll take the time/date from a FITS header if theose fields are completed) and ask it to check for known objects. If your little dot doesn't show up as a known object, you have a potential candidate...
You just need to make sure to download the latest MPC catalogue of known objects. Astrometrica can be set to use the online USNO-B1.0 catalogue (for comparison star fields)so you don't even need to download that.
www.astrometrica.at/
If you need any help, just shout.
Dave
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