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WISE colors in unknowns on Jupiter asteroids

WISE has shown that the two packs of Trojans are strikingly similar and do not harbor any interlopers from other parts of the solar system.
Jupiter-asteroids
New results from NASA's Wide-field Infrared Explorer (WISE) reveal that the Jovian Trojans — asteroids that lap the Sun in the same orbit as Jupiter — are uniformly dark with a hint of burgundy color, and have matte surfaces that reflect little sunlight. // Credit: NASA/JPL-Caltech
Scientists using data from NASA’s Wide-field Infrared Survey Explorer (WISE) have uncovered new clues in the ongoing mystery of Jupiter’s Trojans — asteroids that orbit the Sun on the same path as the giant planet. Like racehorses, the asteroids travel in packs, with one group leading the way in front of the gas giant, and a second group trailing behind.

The observations are the first to get a detailed look at the Trojans’ colors: Both the leading and trailing packs are made up of predominantly dark, reddish rocks with a matte, nonreflecting surface. What’s more, the data verify the previous suspicion that the leading pack of Trojans outnumbers the trailing bunch.

The new results offer clues in the puzzle of the asteroids’ origins. Where did the Trojans come from? What are they made of? WISE has shown that the two packs of rocks are strikingly similar and do not harbor any “out-of-towners,” or interlopers, from other parts of the solar system. The Trojans do not resemble the asteroids from the main belt between Mars and Jupiter, or the Kuiper Belt family of objects from the icier, outer regions near Pluto.

“Jupiter and Saturn are in calm, stable orbits today, but in their past, they rumbled around and disrupted any asteroids that were in orbit with these planets,” said Tommy Grav from the Planetary Science Institute in Tucson, Arizona. “Later, Jupiter recaptured the Trojan asteroids, but we don’t know where they came from. Our results suggest they may have been captured locally. If so, that’s exciting because it means these asteroids could be made of primordial material from this particular part of the solar system, something we don’t know much about.”

German astronomer Max Wolf discovered the first Trojan on February 22, 1906. Christened “Achilles” by the astronomer, the roughly 220-mile-wide (350 kilometers) chunk of space rock was the first of many asteroids detected to be traveling in front of the gas giant. Later, asteroids were also found trailing behind Jupiter. The asteroids were collectively named Trojans after a legend in which Greek soldiers hid inside in a giant horse statue to launch a surprise attack on the Trojan people of the city of Troy.

“The two asteroid camps even have their own ‘spy,’” said Grav. “After having discovered a handful of Trojans, astronomers decided to name the asteroid in the leading camp after the Greek heroes and the ones in the trailing after the heroes of Troy. But each of the camps already had an ‘enemy’ in their midst, with asteroid Hector in the Greek camp and Patroclus in the Trojan camp.”

Other planets were later found to have Trojan asteroids riding along with them, too, such as Mars, Neptune, and even Earth, where WISE recently found the first known Earth Trojan.

Before WISE, the main uncertainty defining the population of Jupiter Trojans was just how many individual chunks were in these clouds of space rock and ice leading Jupiter, and how many were trailing. It is believed that there are as many objects in these two swarms leading and trailing Jupiter as there are in the entirety of the main asteroid belt between Mars and Jupiter.

To put this and other theories to bed requires a well-coordinated, well-executed observational campaign. But there were many things in the way of accurate observations — chiefly, Jupiter itself. The orientation of these jovian asteroid clouds in the sky in the past few decades has been an impediment to observations. One cloud is predominantly in Earth’s northern sky, while the other is in the southern, forcing ground-based optical surveys to use at least two different telescopes. The surveys generated results, but it was unclear whether a particular result was caused by the problems of having to observe the two clouds with different instruments and at different times of the year.

Enter WISE, which roared into orbit December 14, 2009. The spacecraft’s 16-inch (40 centimeters) telescope and infrared cameras scoured the entire sky looking for the glow of celestial heat sources. From January 2010 to February 2011, WISE took about 7,500 images every day. The NEOWISE project used the data to catalog more than 158,000 asteroids and comets throughout the solar system.

“By obtaining accurate diameter and surface reflectivity measurements on 1,750 Jupiter Trojans, we increased by an order of magnitude what we knew about these two gatherings of asteroids,” said Grav. “With this information, we were able to more accurately than ever confirm there are indeed almost 40 percent more objects in the leading cloud.”

Trying to understand the surface or interior of a jovian Trojan is also difficult. The WISE suite of infrared detectors was sensitive to the thermal glow of the objects, unlike visible-light telescopes. This means WISE can provide better estimates of their surface reflectivity, or albedo, in addition to more details about their visible and infrared colors — in astronomy “colors” can refer to types of light beyond the visible spectrum.

“Seeing asteroids with WISE’s many wavelengths is like the scene in The Wizard of Oz where Dorothy goes from her black-and-white world into the technicolor land of Oz,” said Amy Mainzer from NASA’s Jet Propulsion Laboratory in Pasadena, California. “Because we can see farther into the infrared portion of the light spectrum, we can see more details of the asteroids’ colors, or, in essence, more shades or hues.”

The NEOWISE team has analyzed the colors of 400 Trojan asteroids so far, allowing many of these asteroids to be properly sorted according to asteroid classification schemes for the first time.

“We didn’t see any ultra-red asteroids, typical of the main belt and Kuiper Belt populations,” said Grav. “Instead, we find a largely uniform population of what we call D-type asteroids, which are dark burgundy in color, with the rest being C- and P-type, which are more gray-bluish in color. More research is needed, but it’s possible we are looking at the some of the oldest material known in the solar system.”

Scientists have proposed a future space mission to the Jupiter Trojans that will gather the data needed to determine their age and origins.

Scientists using data from NASA’s Wide-field Infrared Survey Explorer (WISE) have uncovered new clues in the ongoing mystery of Jupiter’s Trojans — asteroids that orbit the Sun on the same path as the giant planet. Like racehorses, the asteroids travel in packs, with one group leading the way in front of the gas giant, and a second group trailing behind.

The observations are the first to get a detailed look at the Trojans’ colors: Both the leading and trailing packs are made up of predominantly dark, reddish rocks with a matte, nonreflecting surface. What’s more, the data verify the previous suspicion that the leading pack of Trojans outnumbers the trailing bunch.

The new results offer clues in the puzzle of the asteroids’ origins. Where did the Trojans come from? What are they made of? WISE has shown that the two packs of rocks are strikingly similar and do not harbor any “out-of-towners,” or interlopers, from other parts of the solar system. The Trojans do not resemble the asteroids from the main belt between Mars and Jupiter, or the Kuiper Belt family of objects from the icier, outer regions near Pluto.

“Jupiter and Saturn are in calm, stable orbits today, but in their past, they rumbled around and disrupted any asteroids that were in orbit with these planets,” said Tommy Grav from the Planetary Science Institute in Tucson, Arizona. “Later, Jupiter recaptured the Trojan asteroids, but we don’t know where they came from. Our results suggest they may have been captured locally. If so, that’s exciting because it means these asteroids could be made of primordial material from this particular part of the solar system, something we don’t know much about.”

German astronomer Max Wolf discovered the first Trojan on February 22, 1906. Christened “Achilles” by the astronomer, the roughly 220-mile-wide (350 kilometers) chunk of space rock was the first of many asteroids detected to be traveling in front of the gas giant. Later, asteroids were also found trailing behind Jupiter. The asteroids were collectively named Trojans after a legend in which Greek soldiers hid inside in a giant horse statue to launch a surprise attack on the Trojan people of the city of Troy.

“The two asteroid camps even have their own ‘spy,’” said Grav. “After having discovered a handful of Trojans, astronomers decided to name the asteroid in the leading camp after the Greek heroes and the ones in the trailing after the heroes of Troy. But each of the camps already had an ‘enemy’ in their midst, with asteroid Hector in the Greek camp and Patroclus in the Trojan camp.”

Other planets were later found to have Trojan asteroids riding along with them, too, such as Mars, Neptune, and even Earth, where WISE recently found the first known Earth Trojan.

Before WISE, the main uncertainty defining the population of Jupiter Trojans was just how many individual chunks were in these clouds of space rock and ice leading Jupiter, and how many were trailing. It is believed that there are as many objects in these two swarms leading and trailing Jupiter as there are in the entirety of the main asteroid belt between Mars and Jupiter.

To put this and other theories to bed requires a well-coordinated, well-executed observational campaign. But there were many things in the way of accurate observations — chiefly, Jupiter itself. The orientation of these jovian asteroid clouds in the sky in the past few decades has been an impediment to observations. One cloud is predominantly in Earth’s northern sky, while the other is in the southern, forcing ground-based optical surveys to use at least two different telescopes. The surveys generated results, but it was unclear whether a particular result was caused by the problems of having to observe the two clouds with different instruments and at different times of the year.

Enter WISE, which roared into orbit December 14, 2009. The spacecraft’s 16-inch (40 centimeters) telescope and infrared cameras scoured the entire sky looking for the glow of celestial heat sources. From January 2010 to February 2011, WISE took about 7,500 images every day. The NEOWISE project used the data to catalog more than 158,000 asteroids and comets throughout the solar system.

“By obtaining accurate diameter and surface reflectivity measurements on 1,750 Jupiter Trojans, we increased by an order of magnitude what we knew about these two gatherings of asteroids,” said Grav. “With this information, we were able to more accurately than ever confirm there are indeed almost 40 percent more objects in the leading cloud.”

Trying to understand the surface or interior of a jovian Trojan is also difficult. The WISE suite of infrared detectors was sensitive to the thermal glow of the objects, unlike visible-light telescopes. This means WISE can provide better estimates of their surface reflectivity, or albedo, in addition to more details about their visible and infrared colors — in astronomy “colors” can refer to types of light beyond the visible spectrum.

“Seeing asteroids with WISE’s many wavelengths is like the scene in The Wizard of Oz where Dorothy goes from her black-and-white world into the technicolor land of Oz,” said Amy Mainzer from NASA’s Jet Propulsion Laboratory in Pasadena, California. “Because we can see farther into the infrared portion of the light spectrum, we can see more details of the asteroids’ colors, or, in essence, more shades or hues.”

The NEOWISE team has analyzed the colors of 400 Trojan asteroids so far, allowing many of these asteroids to be properly sorted according to asteroid classification schemes for the first time.

“We didn’t see any ultra-red asteroids, typical of the main belt and Kuiper Belt populations,” said Grav. “Instead, we find a largely uniform population of what we call D-type asteroids, which are dark burgundy in color, with the rest being C- and P-type, which are more gray-bluish in color. More research is needed, but it’s possible we are looking at the some of the oldest material known in the solar system.”

Scientists have proposed a future space mission to the Jupiter Trojans that will gather the data needed to determine their age and origins.

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