Hubble Finds Smallest Kuiper Belt Object Ever Seen

Article written: 16 Dec , 2009
Updated: 24 Dec , 2015
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Artists impression of a small KBO detected by Hubble as it transited a star. Credit: NASA, ESA, and G. Bacon (STScI)

Like finding a needle in a haystack, the Hubble Space Telescope has discovered the smallest object ever seen in visible light in the Kuiper Belt. While Hubble didn’t image this KBO directly, its detection is still quite impressive. The object is only 975 meters (3,200 feet) across and a whopping 6.7 billion kilometers (4.2 billion miles) away. The smallest Kuiper Belt Object (KBO) seen previously in reflected light is roughly 48 km (30 miles) across, or 50 times larger. This provides the first observational evidence for a population of comet-sized bodies in the Kuiper Belt.

The object detected by Hubble is so faint — at 35th magnitude — it is 100 times dimmer than what Hubble can see directly.

So then how did the space telescope uncover such a small body? The telltale signature of the small vagabond was extracted from Hubble’s pointing data, not by direct imaging. When the object passed in front a of star, Hubble’s instruments picked up the occulation.

Hubble has three optical instruments called Fine Guidance Sensors (FGS). The FGSs provide high-precision navigational information to the space observatory’s attitude control systems by looking at select guide stars for pointing. The sensors exploit the wavelike nature of light to make precise measurement of the location of stars.

Illustration of how Hubble found a tiny KBO. Credit: NASA, ESA, and A. Feild (STScI)

Illustration of how Hubble found a tiny KBO. Credit: NASA, ESA, and A. Feild (STScI)


In details of a paper published in the December 17th issue of the journal Nature, Hilke Schlichting of the California Institute of Technology in Pasadena, Calif., and her collaborators determined that the FGS instruments are so good that they can see the effects of a small object passing in front of a star. This would cause a brief occultation and diffraction signature in the FGS data as the light from the background guide star was bent around the intervening foreground KBO.

They selected 4.5 years of FGS observations for analysis. Hubble spent a total of 12,000 hours during this period looking along a strip of sky within 20 degrees of the solar system’s ecliptic plane, where the majority of KBOs should dwell. The team analyzed the FGS observations of 50,000 guide stars in total.

Scouring the huge database, Schlichting and her team found a single 0.3-second-long occultation event. This was only possible because the FGS instruments sample changes in starlight 40 times a second. The duration of the occultation was short largely because of the Earth’s orbital motion around the Sun.

They assumed the KBO was in a circular orbit and inclined 14 degrees to the ecliptic. The KBO’s distance was estimated from the duration of the occultation, and the amount of dimming was used to calculate the size of the object. “I was very thrilled to find this in the data,” says Schlichting.

Hubble observations of nearby stars show that a number of them have Kuiper Belt–like disks of icy debris encircling them. These disks are the remnants of planetary formation. The prediction is that over billions of years the debris should collide, grinding the KBO-type objects down to ever smaller pieces that were not part of the original Kuiper Belt population. The Kuiper Belt is therefore collisionally evolving, meaning that the region’s icy content has been modified over the past 4.5 billion years.

The finding is a powerful illustration of the capability of archived Hubble data to produce important new discoveries. In an effort to uncover additional small KBOs, the team plans to analyze the remaining FGS data for nearly the full duration of Hubble operations since its launch in 1990.

Source: HubbleSite

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3 Responses

  1. SuperKevin says

    This is good to hear, hopefully one day we will be able to track everything floating around out there in our system.

  2. Lawrence B. Crowell says

    I have this distant hope that a rough black hole comes within .1 light years of the sun. We would detect it by measuring how it is perturbing zodiacal light or Kuiper belt objects. If we find such a rough black hole that close we could potentially send a VASIMR propelled probe to it to perform some experiments.

    LC

  3. Jon Hanford says

    I like to think of objects in the Kuiper Belt and the vastly larger Oort Cloud as possible stepping stones from our solar system into the Intergalactic Medium. Estimates put the outer edge of the Oort Cloud at nearly 50,000 AU, nearly a quarter of the distance to Proxima Centauri. These bodies would most likely be rich in raw materials that could be utilized for fuel and sustenance. Small steps, for sure, but headed in the right direction.

    A nearby black hole would be very cool, too. 🙂

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