For over a century Pluto was the only known bright object in the
Solar System beyond Neptune, but in the past two decades a large number of such
objects have been discovered. The difficulty in seeing finding such objects
lies not in observing them at all, but rather in detecting their movement,
which is what reveals them to be a part of the Solar System rather than remote
astronomical objects. Typically the movement of a body in the Inner Solar
System can be detected from observations made hours apart, in which Outer Solar
System objects appear effectively motionless. Only with the advent of long-term
wide-field surveys, which enable the tracking of such objects over several
months, has enabled the detection of many more such objects, though once their
orbits and magnitudes were established, it has been possible to locate many of
these objects in photographic plates taken by observatories dating back to the
1950s.
In a paper published on the arXiv database at Cornell University
Library on 6 January 2015, Mike Brown of the California Institute of Technology, Michelle Bannister of the University of Victoria and The Australian National University,
Andrew Drake, George Djorgovski, Matthew Graham, Ashish Mahabal and Ciro Donalek of the California
Institute of Technology, Steve Larson, Eric Christensen and Ed Beshore of the Lunar and PlanetaryLaboratory at The University of Arizona and Rob McNaught of The Australian National University, describe the results of a study of
data collected by the Catalina Sky Survey in the Northern Hemisphere and Siding Spring Survey in the Southern Hemisphere, with the objective of discovering
previously undetected bright objects on the Outer Solar System.
The Catalina Sky and Siding Spring Surveys are designed to search
for Near Earth Objects, but are also capable of detecting other bright objects
in the sky.
The Catalina Sky Survey uses the 0.7 m Catalina Schmidt telescope
at the Catalina Observatory in Arizona. It is capable of detecting objects with
magnitudes of up to about 19.5 (in astronomy larger magnitudes equate to dimmer
objects; the human eye can detect objects with magnitudes of up to about 5,
while the Sun, Moon and inner planets have negative magnitudes, i.e. magnitudes
of less than zero), with each image covering 8.1 square degrees of sky. Brown et al. used data from the Catalina Sky
Survey collected between 6 December 2005 and 21 April 2012, covering
approximately 19700 square degrees of sky between declinations of -25 and +70
(where zero is directly over the equator, +90 is directly over the North Pole
and -90 is directly over the South Pole).
The Siding Spring Survey operates
from the 0.5 m Uppsala Schmidt telescope at Siding Spring Observatory in
Australia, and is capable of detecting objects with magnitudes of 19.0 or less,
with each image covering 4.2 square degrees of sky. Brown et al. used data collected by the Siding Spring Survey between 20
February 2005 and 29 April 2012, covering approximately 14100 square degrees of
sky from declination -80 to 0. Since there is some overlap between the two
surveys, the total area covered is approximately 29700 square degrees, although
it is impossible to survey for objects at galactic latitudes of less than 10
degrees (i.e. within 10 degrees of the plain of the galaxy) due to the density
of the stars in this part of the sky.
(a) Coverage of the Catalina Sky Survey (CSS). The shading
shows the number of opposition seasons in which each field has been covered 4
or more times. The equal area plot is centred at an RA of 180 degrees and a declination
of 0 degrees with grid marks placed every 30 degrees of RA and declination.
Contours of galactic latitude of 10 and 20 degrees are shown as well as a line
showing the ecliptic. (b) Coverage of the Siding Spring Survey (SSS). All
parameters are as in (a) except that the plot is centredat an RA of 0 degrees.
Brown et al. (2015).
The Catalina Sky and Siding Spring Surveys are intended to search
for Near Earth Objects (asteroids and comets whose paths bring them close to
the Earth) as such the data produced by them has already been filtered for
moving objects closer than 25 AU from the Sun (i.e. 25 times as far from the
Sun as the Earth or less). An object
moving in a circular prograde orbit (the same direction as the planets,
forwards) at a distance of 25 AU will appear to be moving in a retrograde orbit
(the opposite direction to the planets, backwards) at a speed of 4.9 arcseconds
per hour (the total sky, imagined as a sphere, is divided into 360 degrees,
each of which can be subdivided into 60 arcminutes, each arcminute comprises 60
arcseconds); objects more distant from the Sun than the Earth appear to be
moving in a retrograde orbits as they are moving more slowly than the Earth.
For this reason Brown et al. looked
for candidate objects sighted four times within a night within 4.9 arcseconds
of one-another, counting these observations as a single sighting.
Some of these sightings were found to repeat at the same location on
subsequent occasions. Such sightings are assumed to have been of undocumented astrophysical
sources outside the Solar System. Objects which were not subsequently resighted
were also excluded, being assumed to be either optical effects or one off
astrophysical events. Objects which were subsequently observed within 4
arcseconds of the original sighting were retained as possible sightings of
bright trans-Neptunian objects. This resulted in 1.2 million candidate objects
in the Catalina Sky Survey Field and 2.3 million candidate objects in the
Siding Spring Survey Field.
(a) The locations of transients in the Catalina Sky
Survey. To allow viewability only every 20th transient is shown. (b)
The locations of transients in the Siding Spring Survey.Every 20thtransient
is shown. Brown et al. (2015).
Such candidate objects were suspiciously common around the edges of
the fields, particularly on the Siding Spring Survey and around the northern
extent of the Catalina Sky Survey, making it likely that a lot of false
sightings were present in these areas, probably stationary stars being recorded
as moving objects. The comparatively high number of sightings in the Siding
Spring Survey also made analysing this data more difficult. However a known
bright Kuiper Belt objects, such as the dwarf planet Makemake, could be
identified within the data, suggesting that the method was capable of detecting
real objects.
Since objects in the Outer Solar System must follow Keplerian
orbits, Brown et al. next looked for
objects for which such orbits could be defined. This required a minimum of
three separate sightings, since three orbital parameters can be derived from
each sighting, and a minimum of seven parameters are needed to define a
Keplerian orbit. Three randomly selected points will not usually resolve to a
Keplerian orbit, ruling out sets of sightings of different objects. In order to
make the data manageable, only groups of sightings made from pairs separated by
less than 120 days were considered. However this resulted in a total of 160
billion potential triplets in the Catalina Sky Survey Data and 18 trillion potential
triplets in the Siding Spring Survey data, which would take a prohibitive
amount of computational time to process.
In order to further reduce the data volume, Brown et al. then looked for triplets which
were moving on linear paths through the solar system perpendicular to the
Earth-object vector. This reduced dataset still included known objects such as
Makemake, and reduced the number of candidate triplets to 140 million in the
Catalina Sky Survey data and 3 billion in the Siding Spring Survey data.
Brown et al. next
calculated Keplerian orbits for these remaining triplets, ruling out those that
could not be resolved. This reduced the number of candidate triplets to 4.8
million triplets in the Catalina Sky Survey data and 235 million in the Siding
Spring Survey data. However this data was still likely to contain a
considerable number of false sightings, requiring further data reduction to be
used.
Brown et al. therefore
decided to use quadruplets (sets of four sightings that could be determined to
be the same object) rather than triplets. This reduced the number of candidate
objects, with 1192 quadruplets detected in the Catalina Sky Survey data and
5515 quadruplets in the Siding Spring Survey data. This was a sufficiently
small number to begin comparisons of the quadruplets, establishing whether the
same objects had been detected multiple times.
The 1192 quadruplets recovered from the Catalina Sky Survey data
yielded eight distinct objects, all of which were previously known (Makemake, Haumea,
Orcus, Eris, 2002 TX300, Nereid, Huya and 2002 VE95). It was therefore
concluded that requiring four observations per opposition season (an opposition
season being the period when an object outside the Earth’s orbit is on the same
side of the Sun as us, and therefore on the opposite side of the Earth to the
Sun, the only time when faint objects visible only from reflected sunlight are
visible) was sufficient to exclude false positives from the data.
The eight objects detected in the Catalina Sky Survey.
Each of theobjects is found to be a previously discovered object in the Outer
Solar System. Brown et al. (2015).
This means that the Catalina Sky Survey data found every object in
the Solar System beyond 25 AU brighter than magnitude 19.1 (though Uranus and
Neptune were very bright objects which swamped observations and were therefore
excluded from the data processing) except Pluto, which is known to have been in
an area of the galactic plane excluded from the study for the entire period and
Quaoar, which was actually observed twice in the first season, but then also
moved into the galactic plane.The detections included seven Kuiper Belt Objects
in heliocentric Keplerian Orbits, plus Nereid, an irregular satellite of
Neptune. This strongly suggests that there were no undetected objects in the
field survey area brighter then magnitude 19.1.
However none of the 5515 quadruplets observed by the Siding Spring
Survey could be resolved to one another, suggesting that for this field raising
the number of detections to four was insufficient to remove the false
positives, probably due to the far larger number of original detections.
Attempting to raise the bar to five detections also resulted in an observation
rate of zero. Thus while it is highly
likely that Siding Spring was observing objects, a way to recover these from
the data was not found.
See also…
The dwarf planet Pluto will reach opposition slightly before 3.00 am GMT
on Friday 4 July 2014; this means that it will be directly opposite the
Sun in the sky when viewed from Earth, on this occasion in the...
The Kuiper Belt is a region of the Solar System extending from the orbit
of Neptune at about 30 AU (i.e. 30 times the distance between the Sun
and the...
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