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Editor's notes: The following comes from Discovery.com, here. As you read, keep in mind that if this asteroid is on a collision course with Earth, we would expect authorities not to even hint at this possibility until it becomes undeniable. There is plenty of time to move populations around, but that time may, very well, be on the horizon. If my warnings are true, expect to see major headlines as we approach 2020 to 2025, four years before the first "pass by" of this asteroid. My problem is this: I have been reporting on this since 2007. The story never seems to go away. And, now, for some reason, NASA is exploring processes that could change the trajectory of an asteroid. You can see the "why" for my continued interest. Click on the tag, "Apophus, below for other articles.
From Discovery: It’s
little wonder that the name “Apophis” fills people with dread. The name is
Greek for an ancient evil Egyptian god. Also, a potentially hazardous asteroid
was given the ominous name when it was discovered in 2004.
Now,
astronomers using the European Herschel Space Observatory have discovered
something a little unsettling: asteroid 99942 Apophis is actually bigger than
we thought. In fact, it’s been supersized by 20 percent.
Asteroid
Apophis catapulted to fame in 2004 when a study predicted a 2.7 percent chance
of Earth impact in April 2029. Since then, the threat level has been
downgraded. However, the space rock will still make a very close pass with our
planet, coming within 22,364 miles (36,000 kilometers), zooming below the orbit
of geostationary satellites. But Apophis’ orbit is a bit tricky as it will make
yet another close pass in 2036. Although the return trip was also a concern, as of Jan. 9, Apophis’
impact risk in 2036 has been further reduced to a vanishingly small 1 in
7,143,000.
Although
Apophis certainly isn’t a substantial risk, it will likely remain in the
headlines for some years yet.
So,
today, European Space Agency astronomers have announced their findings after
using their orbiting infrared observatory to take a look at Apophis as it raced
toward closest approach to Earth over the weekend. Today, the asteroid flew
safely by at a distance of 9 million miles (14.5 million kilometers, or
one-tenth the Earth-sun distance).
Using
Herschel data, mission scientists have deduced that Apophis is 1,066 feet (325
meters) wide. That’s 20 percent larger than the previous estimate of 885 feet
(270 meters).
“The 20
percent increase in diameter, from 270 to 325 m, translates into a 75 percent
increase in our estimates of the asteroid’s volume or mass,” said Thomas Müller
of the Max Planck Institute for Extraterrestrial Physics in Garching, Germany,
and lead scientist of the study. . . .
Herschel
was also able to map the heat emitted from Apophis’ surface, providing
astronomers with valuable data on the object’s albedo (or reflectivity). It
turns out that the asteroid reflects 23 percent of sunlight that hits it (it
therefore has an albedo of 0.23). 77 percent of the sunlight is absorbed by the
space rock, causing heating. Previous albedo estimates were higher — 0.33 —
meaning Apophis is darker than previously thought.
This
factor is critical. Knowing how much light is absorbed and reflected can
significantly alter orbital models of asteroid orbits. Sunlight imparts a tiny,
yet measurable force on asteroids and heat emitted from the asteroid can do the
same (called the Yarkovsky effect). As an asteroid rotates, it is heated on the
surface facing the sun and cools on the surface facing away. This
heating/cooling cycle can cause changes in the trajectory of the asteroid over
long periods of time.
“These
numbers are first estimates based on the Herschel measurements alone, and other
ongoing ground-based campaigns might produce additional pieces of information
which will allow us to improve our results,” added Müller.
“Although
Apophis initially caught public interest as a possible Earth impactor, which is
now considered highly improbable for the foreseeable future, it is of
considerable interest in its own right, and as an example of the class of Near
Earth Objects,” said Göran Pilbratt, ESA’s Herschel Project Scientist, in a
statement.
“Our
unique Herschel measurements play a key role for the physical characterization
of Apophis, and will improve the long-term prediction of its orbit.”
Note: Apparently the "Apophus" tag does not work. Gee, I wonder how that happened.
Note: Apparently the "Apophus" tag does not work. Gee, I wonder how that happened.
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