Old Hubble Images Reveal Neptune’s “Lost” Moon

Hubble Image Reveals Neptunes Lost Inner Moon

Naiad is the encircled point of light just to the left of Neptune. The images were obtained by the High Resolution Channel of the Advanced Camera for Surveys on the telescope. An occulting mask was placed in front of Neptune to reduce the planet’s glare. In the image, a color composite of Neptune, taken one month earlier, has been inserted for context.

Using new techniques to suppress Neptune’s glare, astronomers view Neptune’s innermost moon for the first time since it was discovered by Voyager 1989.

Neptune’s tiny, innermost moon, Naiad, has now been seen for the first time since it was discovered by Voyager’s cameras in 1989. Dr. Mark Showalter, a senior research scientist at the SETI Institute in Mountain View, California, announced the result today in Denver, Colorado, at the annual meeting of the Division for Planetary Sciences of the American Astronomical Society. He and collaborators Dr. Jack Lissauer of the NASA Ames Research Center, Dr. Imke de Pater of UC Berkeley, and Robert French of the SETI Institute, also released a dramatic new image of Neptune’s puzzling rings and ring-arcs, which were first imaged by Voyager.

“Naiad has been an elusive target ever since Voyager left the Neptune system,” said Dr. Showalter. From Earth, Neptune is 2 million times brighter than Naiad, and the two are separated by only one arcsecond. “This is equivalent to the width of a human hair from 50 feet away,” noted collaborator Lissauer. The team of astronomers needed to develop new techniques to suppress Neptune’s glare. Naiad was finally revealed, moving across a sequence of eight images taken during December 2004.

Hubble Image Reveals Naiad

This version of the image identifies all of the bodies visible in the image. Note that even the newly-discovered moon, provisionally identified as S/2004 N 1, is visible here as a faint dot. Only the third moon from the center–Despina–is not shown, because it was positioned behind the occulting mask, along with Neptune, at the time the images were taken.

Strangely, Naiad appears to have veered significantly off course. The astronomers are puzzled by the fact that Naiad is now far ahead of its predicted orbital position. They wonder whether gravitational interactions with one of Neptune’s other moons may have caused it to speed up, although the details remain mysterious. Further observations will be needed in order to understand Naiad’s motion.

In addition to its moons, Neptune hosts a family faint rings and ring-arcs. The arcs have been changing slowly in the years since their discovery. Whereas Voyager saw a set of four closely-spaced arcs, the leading two arcs have been fading away, and are completely absent from the newest images. The trailing arcs, however, are essentially unchanged. This system of arcs is probably confined by the gravitational effects of the nearby moon Galatea, but the reason for the long-term changes is unknown. Dr. de Pater has also been following the ongoing evolution of the arcs from the 10-meter W. M. Keck telescope in Hawaii.

Showalter and his collaborators had previously announced the discovery of a tiny moon of Neptune in July. That moon, which is no more than 20 km (12 miles) across, goes by the provisional designation “S/2004 N 1”. The new results reported today are based on further analysis of the same images, which were all obtained by Hubble between 2004 and 2009. Although 100-km Naiad is much larger than the moon announced in July, it orbits much closer to Neptune and so has proven to be much harder to detect.

Astronomers View Neptunes Innermost Moon

The outer ring, Adams, shows two distinct bright segments or “arcs” to the right of Neptune. At the time of the Voyager flyby, this ring contained four arcs, but two of them subsequently faded away. The arcs are believed to be confined by the gravitational influence of a nearby moon, Galatea, but the scientists do not currently understand why only two of the four arcs have survived for the intervening 15 years. An inner ring, Leverrier, is also visible.

“It is always exciting to find new results in old data,” Showalter remarked. “We keep discovering new ways to push the limit of what information can be gleaned from Hubble’s vast collection of planetary images.”

Download the Press Conference Slides

Support for this work was provided by NASA through grant number from the SPACE TELESCOPE SCIENCE INSTITUTE, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.

More Information about the Images:

Neptune’s innermost moon, Naiad, is clearly seen here for the first time since the Voyager 2 flyby of 1989. The Hubble Space Telescope captured the tiny point of light just off to the side of Neptune in December, 2004. The detection went unnoticed until recently, when the images were re-analyzed using newly developed processing techniques. The new analysis employed special processing to suppress the extensive glare around Neptune, which is more than one million times brighter than the nearly 100-km object shown. The image is composed of eight four-minute exposures, which have been combined to produce the equivalent of a single 32-minute exposure.

The images were obtained by the High Resolution Channel of the Advanced Camera for Surveys on the telescope. An occulting mask was placed in front of Neptune to reduce the planet’s glare. In the image, a color composite of Neptune, taken one month earlier, has been inserted for context.

Source: SETI Institute

Images: SETI Institute

1 Comment on "Old Hubble Images Reveal Neptune’s “Lost” Moon"

  1. Madanagopal.V.C | October 10, 2013 at 8:12 am | Reply

    Neptune has already got four moons and also the ring structure corresponding to all the gas giants like Saturn, Jupiter, Uranus. The small moon Naiad is now discovered in the inner most orbit of Neptune. May be we can find more small moons and stones floating around it as in the case of Saturn where we found and astounding 23 moons and still counting. Thank You.

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