688 Melanie

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688 Melanie (prov. designation: Template:Mp or Template:Mp) is a dark background asteroid from the central regions of the asteroid belt. It was discovered by Austrian astronomer Johann Palisa at the Vienna Observatory on 25 August 1909.[1] The carbonaceous C-type asteroid has a rotation period of 18.9 hours and measures approximately Script error: No such module "convert". in diameter. Any reference to the origin of the asteroid's name is unknown.[2]

Orbit and classification

Melanie is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[3][4][5] It orbits the Sun in the central asteroid belt at a distance of 2.3–3.1 AU once every 4 years and 5 months (1,618 days; semi-major axis of 2.7 AU). Its orbit has an eccentricity of 0.14 and an inclination of 10° with respect to the ecliptic.[6] The body's observation arc begins at Vienna Observatory in July 1913, or four years after its official discovery observation.[1]

Naming

This minor planet was named in 1910, by Otto Prelinger who collaborated with Johann Palisa and Max Wolf on the photographic star charts (AN 186, 15). Any reference of this minor planet's name to a person or occurrence is unknown.[2]

Unknown meaning

Among the many thousands of named minor planets, Melanie is one of 120 asteroids for which Template:MoMP has been published. All of these asteroids with an unknown meaning have low numbers, beginning with Template:Mp and ending with Template:Mp, all discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.[7]

Physical characteristics

In both the Bus-DeMeo classification and the Bus–Binzel SMASS classification, Melanie is a common, carbonaceous C-type asteroid.[6][4]

Rotation period

In September 2011, a rotational lightcurve of Melanie was obtained from photometric observations by Robert Stephens at the Santana Observatory Template:Obscode in California. Lightcurve analysis gave a well-defined rotation period of Script error: No such module "val". hours with a low brightness variation of Script error: No such module "val". magnitude (U=3Script error: No such module "Check for unknown parameters".).[8] The first but unsuccessful attempt to measure the objects period was undertaken by Richard Binzel in June 1984.[9] Other observations by French amateur astronomers Laurent Bernasconi (2005) and René Roy (2011) gave a period of (Script error: No such module "val".) and (Script error: No such module "val".) hours and an amplitude of Script error: No such module "val". and Script error: No such module "val". magnitude, respectively (U=2−/2−Script error: No such module "Check for unknown parameters".).[10] Also in 2011, an ambiguous period of (Script error: No such module "val".) with an alternative period solution of 16.10 hours and an amplitude of (Script error: No such module "val".) magnitude was determined (U=2Script error: No such module "Check for unknown parameters".).[11]

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), and the Japanese Akari satellite, Melanie measures (Script error: No such module "val".), (Script error: No such module "val".) and (Script error: No such module "val".) kilometers in diameter and its surface has an albedo of (Script error: No such module "val".), (Script error: No such module "val".) and (Script error: No such module "val".), respectively.[12][13][14]

The Collaborative Asteroid Lightcurve Link adopts the albedo obtained by IRAS and derives a diameter of 41.38 kilometers using an absolute magnitude of 10.59.[15] Alternative mean-diameters published by the WISE team include (Script error: No such module "val".), (Script error: No such module "val".), (Script error: No such module "val".), (Script error: No such module "val".) and (Script error: No such module "val".) with a corresponding albedo of (Script error: No such module "val".), (Script error: No such module "val".), (Script error: No such module "val".), (Script error: No such module "val".) and (Script error: No such module "val".).[4][15] On 4 August 2002, an asteroid occultation gave a best-fit ellipse dimension of (Script error: No such module "val".) with a low quality rating of 0.[4] These timed observations are taken when the asteroid passes in front of a distant star.[4]

References

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  1. ↑ a b Script error: No such module "citation/CS1".
  2. ↑ a b Script error: No such module "citation/CS1".
  3. ↑ Script error: No such module "citation/CS1".
  4. ↑ a b c d e Script error: No such module "citation/CS1".
  5. ↑ Script error: No such module "Citation/CS1". (PDS main page)
  6. ↑ a b Script error: No such module "citation/CS1".
  7. ↑ Script error: No such module "citation/CS1".
  8. ↑ Script error: No such module "Citation/CS1".
  9. ↑ Script error: No such module "Citation/CS1".
  10. ↑ Script error: No such module "citation/CS1".
  11. ↑ Script error: No such module "Citation/CS1".
  12. ↑ Script error: No such module "Citation/CS1".
  13. ↑ Script error: No such module "Citation/CS1".
  14. ↑ Script error: No such module "Citation/CS1". (online, AcuA catalog p. 153)
  15. ↑ a b Script error: No such module "citation/CS1".

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External links

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