Discovery News | Ian O'Neill | 2013 Jan 09
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.”
Herschel Spacecraft Eyes Asteroid Apophis
NASA JPL-Caltech | 2013 Jan 09
Herschel Intercepts Asteroid Apophis
ESA Space Science | 2013 Jan 09
