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Finding Neptune’s Smallest Moon

What a lively place Neptune used to be, at least back in the days when the planet captured Triton, doubtless a Kuiper Belt Object now in a retrograde orbit around the primary. Recent work led by Mark Showalter (SETI Institute) puts the Hubble Space Telescope to work in studying one result of the sudden acquisition of so massive an object. A first generation of small satellites was likely scattered and rearranged, its debris becoming the Neptunian moons we see today.

Among them is Hippocamp, once known as S/2004 N 1, which appears to be a fragment from Neptune’s second largest moon Proteus. What an interesting set of observations we have here. Discovered in 2013, Hippocamp is the outermost of the planet’s inner moons, and it orbits a scant 12,000 kilometers from Proteus. We can relate the 2013 discovery with what Voyager 2 found at Neptune in 1989: A large impact crater on Proteus.

“The first thing we realised was that you wouldn’t expect to find such a tiny moon right next to Neptune’s biggest inner moon,” saysd Mark Showalter. “In 1989, we thought the crater was the end of the story. With Hubble, now we know that a little piece of Proteus got left behind and we see it today as Hippocamp.”

Image: This artist’s impression shows the outermost planet of the Solar System, Neptune, and its small moon Hippocamp. Hippocamp was discovered in images taken with the NASA/ESA Hubble Space Telescope. Whilst the images taken with Hubble allowed astronomers to discover the moon and also to measure its diameter, about 34 kilometres, these images do not allow us to see surface structures. Credit: ESA/Hubble, NASA, L. Calçada.

The likely cause of the Proteus impact is a comet, striking long after the havoc created by Triton’s appearance. Jack Lissauer (NASA Ames) is a co-author of the new work:

“Based on estimates of comet populations, we know that other moons in the outer Solar System have been hit by comets, smashed apart, and re-accreted multiple times. This pair of satellites provides a dramatic illustration that moons are sometimes broken apart by comets.”

Image: This composite image shows the location of Neptune’s moon Hippocamp, formerly known just as S/2004 N 1, orbiting the giant planet Neptune, about 4.8 billion kilometres from Earth. The moon is only about 34 kilometres in diameter and dim, and was therefore missed by NASA’s Voyager 2 spacecraft cameras when the probe flew by Neptune in 1989. Several other moons that were discovered by Voyager appear in this 2009 image, along with a circumplanetary structure known as ring arcs. Mark Showalter of the SETI Institute discovered Hippocamp in July 2013 when analysing over 150 archival images of Neptune taken by Hubble from 2004 to 2009. The black-and-white image was taken in 2009 with Hubble’s Wide Field Camera 3 in visible light. Hubble took the colour inset of Neptune on August 19, 2009. Credit: NASA, ESA, and M. Showalter (SETI Institute).

Just 1/1000th the mass of Proteus, Hippocamp shouldn’t be where we see it, but that large impact crater Voyager found on Proteus tells the tale. It alone explains why Proteus didn’t assimilate or sweep aside Hippocamp long ago, thanks to an impact sufficient to have all but shattered Proteus while leaving Hippocamp behind. That cometary bombardment makes Hippocamp a third-generation satellite.

Image: This diagram shows the orbital positions of Neptune’s inner moons, which range in size from 17 to 420 kilometres in diameter. The outer moon Triton was captured from the Kuiper belt many billions of years ago. This tore apart Neptune’s original satellite system. After Triton settled into a circular orbit the debris from shattered moons re-coalesced into the second generation of inner satellites seen today. However, comet bombardment continued, leading to the birth of Hippocamp, which is a broken-off piece of Proteus. Therefore, Hippocamp is considered to be a third-generation satellite. Neither the size of the moons and Neptune, nor the orbits are to scale. Credit: NASA, ESA, and A. Feild (STScI).

Yesterday we looked at an exoplanet scenario for a massive planetary collision. The collision of Proteus with a comet is much smaller in scale, but powerful in its effects. From the paper:

We cannot rule out the possibility that Hippocamp formed in situ and has no connection to Proteus. However, its tiny size and peculiar location lead us to favour the proposed formation scenario, which illustrates the roles that collisions and orbital migration have played in shaping the Neptune system that we see today

The paper is Showalter et al., “The Seventh Inner Moon of Neptune,” Nature 566, pp. 350–353 (20 February 2019). Abstract.

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Comments on this entry are closed.

  • Charley February 21, 2019, 18:48

    Hippocamp, what a funny name for a moon! Is this some type of Latin or Greek derived name ? Does it have some type of meaning in ancient times?

    • Paul Gilster February 21, 2019, 20:57

      Hippocamp comes from Greek ‘hippos’ (‘horse’) and ‘kampos (‘sea monster’). Think of a horse-like sea-monster — a seahorse will do — or else the part of the brain called the hippocampus. I’m afraid I haven’t delved into why the researchers are calling this object Hippocamp, however. Google can pull word derivations like these pretty swiftly, which is how I looked this up.

    • Alex Tolley February 22, 2019, 13:30

      From Wikipedia:

      The discovery team decided to submit a name proposal to the International Astronomical Union based on a figure from Greco-Roman mythology with a relationship to Poseidon or Neptune, the god of the sea,[12] consistent with the naming of other moons of Neptune.[25] Among the names considered was Polyphemus, the gigantic one-eyed son of Poseidon and Thoosa.[26] Showalter, the lead of the discovery team, chose the name Hippocamp partly in acknowledgement of the seahorse genus, Hippocampus, and the mythological creature that is aptly part horse and part fish.[3] In 2019, the IAU accepted the name Hippocamp.[7]

      Mythology:
      Hippocampus (mythology)

  • Robin Datta February 22, 2019, 16:02
  • Antonio February 24, 2019, 10:36

    Time is long due for a Neptune orbiter!

    • Bruce D. Mayfield February 26, 2019, 3:14

      Three planets in need of Cassini type orbiters: Uranus, Neptune and even Jupiter. They have 27, 14 and 57 moons respectively that need to be investigated.

  • Harry R Ray February 27, 2019, 11:41

    Konstantin Batygin tweeted this 14 hours ago: “…we did thousands of new P9 simulations and realized that P9 is smaller(~5Mearth), closer(~400-500 AU), more circular(e~0.2), and visually brighter(V~23)than we originally thought…”. Does this mean that they have been looking in the WRONG PLACE for it? ALSO: Big bummer here – unless Planet Nine is at the EXACT UPPER LIMIT of their AU estimate,it CANNOT be used as an orbital platform for microlensing.

  • ljk March 9, 2019, 14:31

    Hubble solves puzzle of Neptune mystery moon

    By Paul Scott Anderson in SPACE | March 2, 2019

    Meet Hippocamp, the smallest known moon of the planet Neptune. Scientists have puzzled over its origin, and over why we see it orbiting where we do. Now, new Hubble data has shed light on these mysteries.

    https://earthsky.org/space/hubble-solves-mystery-neptune-moon-hippocamp