When did the asteroids become minor planets?
by James L. Hilton
Discovery of the Asteroids
The controversy over whether Pluto should be given a minor planet number
and possibly be demoted from the ranks of the major planets reminds me of a
similar controversy that occurred 150 years ago. This controversy involved
whether or not the bodies discovered between Mars and Jupiter should be
considered equal to the seven other planets known at that time.
Titius von Wittenburg (1766)
discovered that the relative distances of the six known planets from the
Sun almost fit a simple relation. But it had a problem. It predicted there
should be a planet between the orbits of Mars and Jupiter. In 1772 he
published a tract proposing that a planet should exist in the gap.
According to Cunningham
(1988), Johann Bode, director of the Berlin Observatory so popularized
this tract that the relation is now known as Bode's law.
In 1781 Uranus was discovered at just the distance where Bode's Law
predicted a seventh planet (including the gap between Mars and Jupiter)
should occur. This touched off a search for a planet in the gap between
Mars and Jupiter. The search ended, literally before it had begun, on
January 1, 1801 when Guiseppe Piazzi at the Palermo Observatory discovered
a 'star' that had moved from its position the previous night in the
constellation of Taurus (von
Zach 1801). Like Uranus, it was found to be a body at exactly the
distance predicted by Bode's Law. Two consecutive successes for a relation
that has no known physics behind it.
Piazzi named the new planet Ceres Ferdinandea after Ceres, the Roman
goddess of the harvest, and King Ferdinand IV of Naples and Sicily. The
second half of the name was dropped after several years for political
reasons. Thus, the gap was filled and the search ended.
Unexpectedly, on March 28, 1802 Heinrich Olbers discovered another small
body while observing Ceres. Its semi-major axis was nearly the same as
Ceres, and posed problems for the picture of the solar system that had been
emerging over the previous decades. Eventually, this new body was named
Neither of these bodies fit the conventional idea of a planet because
they were so small that their disks were nearly unobservable. Using a
projection system Herschel
(1802) determined 161.6 miles (260.0 km) for the diameter of Ceres and
147 miles (237 km) for Pallas. These results are nearly a factor of four
too small for Ceres and more than a factor of two too small for Pallas.
Because of this starlike appearance, Herschel declared, "From this, their
asteroidal appearance, if I may use that expression, therefore, I shall
take my name, and call them Asteroids; reserving for myself, however, the
liberty of changing that name, if another, more expressive of their nature
should occur." Thus Herschel argued that Ceres and Pallas were not the same
as the other planets.
However, other astronomers of the time thought otherwise. These two new
additions to the solar system were listed along with the rest of the
planets in order of increasing distance from the Sun. They were also given
symbols by their discoverers to be used when recording observations.
The symbols for the planets, shown in Table 1, were and are used as a
shorthand notation by astronomers, and others. To fulfill this role, they
are quick to draw, are easily distinguishable, and do not require much
skill to produce. Many of the symbols have several variants. The ones shown
in Table 1 are those almost universally adopted by the astronomical
Table 1. The Symbols of the Sun, Moon, and Planets.
The discoveries of Juno in 1804 and Vesta in 1807 raised concern in astronomers of
the day that the asteroids were fragments of a planet that had somehow disintegrated.
This theory was first proposed by Olbers upon the discovery of Pallas. However, Juno
and Vesta were added to the catalog of planets along with Ceres, Pallas, and, in
The acceptance of the first four asteroids was so matter-of-fact that introductory
texts such as First Steps to
Astronomy and Geography (1828) lists the planets as, "Eleven: Mercury, Venus, the
Earth, Mars, Vesta, Juno, Ceres, Pallas, Jupiter, Saturn, and Herschel." Herschel was
an alternate name for Uranus (after its discoverer) used in Britain until the 1850's.
The Scene Becomes Complicated
The fifth asteroid, Astraea was discovered near the end of 1845, nearly 39 years
after the discovery of Vesta. The year 1847 saw the discovery of three new asteroids.
By the end of 1851 there were 15 asteroids, still listed by distance from the Sun.
Fourteen of them each had their own symbol; although, the symbol for Irene had never
been drawn, only described (Gould 1852)!
Some of these symbols, in Table 2, were quite fanciful and took significant artistic
skill to draw. Only the symbols for Ceres, Pallas, and Juno kept the same basic
simplicity of the symbols for the larger bodies in the solar system.
Table 2. The Old Symbols of the Asteroids. From
|Asteroid ||Old Symbol
|Egeria ||Never assigned
|Irene ||"A dove carrying an olive-branch, with a star
on its head" (Hind 1852) (never
Encke (1851) made a major change in the
Berliner Astronomisches Jahrbuch, BAJ, for 1854. He said, "Finally, I want
to add that - in view of the complications and difficulties with the recently used
planetary symbols - I took the liberty to introduce the encircled numbers in stead of
symbols," (Translation by Schmaedel,
1999). However, there were some very definite differences from today's scheme. The
asteroids Encke was referring to began with Astrea which was given the number (1) and
went through (11) Eunomia. Ceres, Pallas, Juno, and Vesta continued to be denoted by
their traditional symbols. Not only that, but Ceres through Vesta continued to be listed,
in semi-major axis order along with the ephemerides of the major planets while Astrea
through Eunomia, and Neptune were relegated to a section at the end of the BAJ.
This innovation was immediately seized upon by the astronomical community at large.
American astronomer, B.A. Gould (1852)
As the number of known asteroids increases, the disadvantages of a symbolic notation
analogous to that hitherto in use increase much more rapidly even than the difficulty of
selecting appropriate names from the classic mythology. Not only are many of the symbols
proposed inefficient in suggesting the name of which they are intended to be an
abbreviation; but some of them require for their delineation more artistic accomplishment
than an astronomer is necessarily or generally endowed with.
To simplify this system he proposed a new set of symbols:
To remedy this evil, and not to lose the unquestionable advantage connected with a system
of symbols easily remembered and readily drawn,-it has been agreed upon by several
astronomers in Germany, France, England, and America, to propose for adoption a more
simple system for the group in question,-consisting of a circle containing the number of
the asteroid in the chronological order of its discovery.
The new system of symbols was designed to relieve the growing confusion and restore the
original intent of the symbols, a quick shorthand way of referring to solar system bodies;
not to give the asteroids a different status from the rest of the planets. However, Gould
did state, "...we thus have a symbol ready for every asteroid hereafter to be discovered,
and this remarkable group are distinguished from the larger planets in the character of
In the BAJ for 1855 (Encke, 1852) the numbering of the minor planets at the back
began with (5) Astrea and goes through (15) Eunomia. Ceres through Vesta continued to be
listed in semi-major axis order with the major planets, using their old symbols. This
continued until the BAJ for 1867 (Encke, 1864) where they are listed as (1) Ceres,
(2) Pallas, (3) Juno, and (4) Vesta in order of discovery along with the other asteroids.
The first new asteroid for which the new symbol convention was used was (16) Psyche by
Ferguson (1852) in the publication of a
series of observations at the U.S. Naval Observatory.
However, at least three additional asteroids, (28) Bellona
(Encke, 1854), (35) Leukothea
(Rumker & Peters 1855), and (37)
Fides (Luther 1855), were given the
symbols in Table 3. The symbol for Leukothea, the most complicated of all, is described
by Rumker & Peters as representing an ancient lighthouse. However, there is no
evidence that these symbols were ever used outside of their initial publication in the
Table 3. Symbols for the Asteroids Introduced after 1852.
|(28) Bellona ||
|(35) Leukothea ||
|(37) Fides ||
Cunningham (1988) states that this
set of symbols for the asteroids lasted until 1931 when it was replaced by a number
followed directly by the name; however, I have not been able to find an official notice
of the adoption of the present scheme of numbering asteroids. On the other hand, the
literature shows that several different schemes were used during the latter half of the
nineteenth century. The present form of number name is first found in the
Astronomische Nachrichten (1911).
The Change Occurs
The acceptance of the new system of symbols was extremely fast. The Astronomical
Journal, edited by Gould, adopted the new symbols immediately. The journal
Astronomische Nachrichten had
articles sporadically including the new symbols beginning 1854, and adopted them for its
index beginning in 1861. The Royal Greenwich
Observatory began labeling observations of the asteroids with the new symbols
beginning in 1858 with the publication of observations from 1856. The
Paris Observatory used them in its
table of contents in 1858, with the publication of its first volume of observations. And
the U.S. Naval Observatory adopted the use of the new symbols in 1863 with the
publication of its observations from 1852.
The two major almanacs that printed asteroid ephemerides at this time had interesting
reactions to the introduction of the new symbols.
The British The Nautical Almanac and Astronomical Ephemeris had been
publishing ephemerides for Ceres, Pallas, Juno, and Vesta in order of their semi-major
axes between the ephemerides of Mars and Jupiter. In the volume for 1856, published in
1853, it stopped printing asteroid ephemerides altogether.
The BAJ continued to publish the ephemerides of the first four asteroids
discovered in semi-major axis order using the old symbols up through the volume for
1866, published in 1864. The ephemerides of the other asteroids were given in numerical
order in a section a section at the end of the BAJ along with the ephemeris for
Neptune. Beginning in 1852 there was also a table of opposition dates included at the
end of the asteroid ephemerides at the end of the BAJ. This table included the
opposition dates for Ceres through Vesta, indicating sort of a 'dual citizenship' for the
first four asteroids. Ceres through Vesta were not included with the other asteroids
until the edition for 1867, published in 1864. This was the first volume since the
introduction of the new symbols not published under the direction of Encke.
The BAJ evidently went so far as to announce a policy to refer to the asteroids
(60) and higher by their numbers only. This led
Förster (1861) to comment, "As for
naming planets, Berlin defines them by numbers only from planet (60) onwards,"
(Translation by Schmaedel, 1999).
However, the edition for 1864, printed in 1861, and all subsequent of the BAJ
refer to all the known asteroids by both number and name.
However, the advent of the new symbols also brought with it other changes. Except for
the U.S. Naval Observatory, all of the other publications immediately began publishing
their observations in order of their numerical symbol rather than their distance from the
Sun. The Paris Observatory also moved the observations of the asteroids to a section
separate from the observations of the other planets, while the Royal Greenwich
Observatory left the observations, in numerical order, between the observations of Mars
The Asteroids are Called 'Minor Planets'
The British The Nautical Almanac and Astronomical Ephemeris had been producing
the elements of the asteroids under the heading of 'Minor Planets, Elements of' since its
volume for 1845, published in 1841. This is the only instance of the use of the phrase
'minor planet' I have found previous to the introduction of the new symbols for the
asteroids. Strangely, this section was dropped from the almanac along with the
ephemerides of Ceres, Pallas, Juno, and Vesta in the volume for 1856, published in 1853.
The first use of 'Kleine Planeten' after the introduction of the new system of symbols
was as 'kleine Planeten' in a paper by Jahn
(1854) in Astronomische Nachrichten. By 1861, the Astronomische Nachrichten
uses 'kleine Planete' as a subcategory to Planete (planet) in the index to collect the
articles on the asteroids. The Astronomische Nachrichten kept the asteroids as a
subcategory of the planets until it published its general index of volumes 181-210 in
1932 (Astronomische Nachrichten
Prior to 1866 the Paris Observatory
used the numerical symbols only in the table of contents. That year, the Paris
Observatory first uses the description 'petites planetes' in the observations. The
asteroids Ceres through Vesta, however, are conspicuously not included in the
category of 'petites planetes'. The observation of the first four asteroids are tabulated,
in order of discovery, not with the other planets, but in a section immediately before the
section titled 'Petites planetes'. Only beginning in 1868
(Paris Observatory 1868) are these four
bodies included with the rest of the 'petites planetes'. Like the BAJ the Paris
Observatory evidently gave Ceres through Vesta a sort of 'dual citizenship' until the
The U.S. Naval Observatory used the word 'asteroids' to describe the bodies between the
orbits of Mars and Jupiter until 1868. At that time it switched to using the term 'small
planets' (U.S. Naval Observatory 1868).
In 1892 it switched back to 'asteroid' (U.S.
Naval Observatory 1892) then to 'minor planet' in 1900
(Harkness & Skinner 1900), and
finally back to 'asteroid' in 1929 (Peters
The U.S. Nautical Almanac Office, an institution independent of the U.S. Naval
Observatory in the nineteenth century, generally mirrored the usage of the U.S. Naval
Observatory. Aside from a single usage of the term 'minor planet' in 1866, the
communications of the U.S. Nautical Almanac Office always referred to the asteroids as
either 'asteroids' or 'planets.' It is also clear that the Office desired to produce a
full set of ephemerides during a time in which it was struggling to establish itself and
produce its first volumes (Report of the
Nautical Almanac Office 1849-1896).
B.A. Gould at The Astronomical Journal never used the term 'minor planet,'
always opting for 'asteroid'. However, the asteroids were listed separately from the other
planets. Only with the publication of the index to volume 90 in 1985 of the Astronomical
Journal ( Astronomical Journal
1985), long after Gould's death, was the term 'minor planets' used. In December 1998,
the index of volume 116 of the Astronomical Journal uses the puzzling category of
'Minor Planets, Asteroids' ( Astronomical
The Royal Greenwich Observatory appears to have held out until after the turn of the
century. It continued to publish the observations of the asteroids between the observations
of Mars and Jupiter. However, they are listed in numerical order rather than in order of
semi-major axis. The title of the section was 'Observations of the Sun, the Moon, and the
Planets'. The Royal Greenwich Observatory never used either the word 'minor' or 'asteroid'
in regard to any of its observations of solar system bodies until the publication of its
1905 observations (Royal Greenwich Observatory
Thus, the term 'minor planet' was quickly adopted by the astronomical community. But,
its acceptance was not universal.
The Sizes of the first three asteroids shrink
At the time the description 'minor planet' began to be used, the most widely
disseminated values for the diameters of the first four asteroids discovered were Ceres,
2613 km; Pallas, 3380 km; Juno, 2290 km; and Vesta, "not more than 383 km"
(Hughes 1994). The diameters of the first
three asteroids were derived from direct estimates of the sizes of their disks by
Schroter (1811) and are directly comparable
to the 2390 km of Pluto. The pre-1855 asteroid diameters, shown in Figure 1, are grossly too
Fig.1. The diameters determined for the four largest asteroids at different
times. The diameter of Pluto is included for purposes of comparison.
Conversely, the first determination of the diameters of the asteroids after the use of
the term minor planets began to be used were too small.
Stampfer (1856) produced diameters of 350,
270, 200, and 400 km for Ceres, Pallas, Juno, and Vesta respectively. These diameters were
based on photometry rather than trying to measure the angular diameter directly. However,
the albedos chosen were more like that of an icy body in the outer solar system rather than a
rocky body of the inner solar system which these asteroids more closely resemble.
Just as the earlier diameters determinations made as 'planets' were way too large, the
first 'minor planet' diameters were way too small. In both cases the size determined depended
on the assumptions that went into interpreting the data. The question that can not be
answered is, "How much were these assumptions colored by how the observers thought of the
bodies they were observing?" In either case, the assumptions made were not necessarily
Finally, the use of the numbers as part of a symbolic shorthand for the asteroid names
appears to have lost its symbolism shortly after it was introduced.
Here again The Astronomical Journal
(1858) led the way. Beginning in 1858 it marked newly discovered asteroids by enclosing
their number in parentheses rather than a circle. Once the asteroid's orbit was firmly
established, the symbol was then changed to the number enclosed by a circle. This format
lasted only until 1888 when it switched to the number followed by the name separated by a
comma (Astronomical Journal 1888).
Finally, in 1895 it switched back to using parentheses for all asteroids and always followed
by the asteroid's name (Astronomical Journal
The U.S. Naval Observatory (1868) adopted
the parentheses followed by the name for the asteroids in 1868. In 1872 it replaced the
parentheses with a circle, but kept the name
(U.S. Naval Observatory 1895). It used this
convention until 1949. At this time only the first four asteroids, Ceres, Pallas, Juno, and
Vesta, which it referred to by name only, were observed
(Watts & Adams 1949).
The Astronomische Nachrichten (1872)
started using parentheses followed by the name for all asteroid numbers in 1872. And then
switched to the present day format of number and name without circle, parentheses, or comma
in 1911 (Astronomische Nachrichten 1911).
The Paris Observatory kept the number within a circle symbol right up to 1908, but always
gave the name along with the symbol.
Cunningham (1988) asserts that the
symbol of a number enclosed by a circle was the official designation for asteroids until 1931
when the current nomenclature of the number, sometimes enclosed in parentheses in paper titles
and indices, followed by the name without a separating comma was adopted. However, I do not
know of any agreement codifying this. It is also clear that the number name designation had
become the de facto standard in the literature by evolution over the 73 years between 1858 and
1931. The number in a circle for an asteroid had quickly lost its nature as a symbol and
merely become an accounting tool for the ordering of the asteroids.
Along with the adoption of a new set of symbols that easily separated the asteroids from
the other planets, it appears that the change from planet to minor planet happened very
quickly. It was recognized from the beginning that these bodies did not fit along with the
rest of the planets, but during the years in which the number of known asteroids was small,
they were included on the list of solar system bodies just as if they were regular planets.
However, once their numbers grew too large to fit the existing scheme of classification, their
uniqueness was quickly recognized and a new class of solar system objects was created.
The event that appears to have triggered this reevaluation of the asteroids was the
introduction of a new set of symbols to use as a shorthand notation for them. The new set of
symbols had nothing to do with judging whether or not the asteroids were planets. They were
designed to restore the reason for having the symbols in the first place, a quick convenient
method of referring to a body. Nor is it clear that the name 'minor planet' was meant to
separate the asteroids from the other planets. However, the introduction of the new system of
symbols had the unintended consequence of reordering the asteroids from the traditional
ordering of the planets, by semi-major axis, to numerical order and setting them apart from
the other planets. This separation allowed a new category of solar system objects to be
The BAJ and the Paris Observatory accorded Ceres through Vesta a form of 'dual
citizenship' with both the planets and the asteroids through the mid-1860's. The failure of
this dual categorization is noteworthy because Ceres, the first asteroid discovered, is
estimated to contain 30-40% of the mass of the asteroid belt, while Pallas and Vesta combined
are nearly as massive as Ceres. Because they fit the mold of a minor planet better than that
of a regular planet, even these largest asteroids are considered minor planets after more
than 50 years of being accepted as planets like Jupiter, Saturn, and Mercury.
The label of 'minor planet' also appears to have had almost immediate consequences in
terms of assumptions made in determining their diameters. Almost immediately after the term
'minor planet' was adopted a new determination of the diameters of the first three asteroid
produced values only 10% of those previously adopted, and much smaller than today's accepted
values. Although the methods used in the different eras changed radically, they both required
that the observer make assumptions in reducing the data. These assumptions may have been
colored by how the observers thought of the asteroids.
Acknowledgments I would like to acknowledge the works of
C.J. Cunningham (1988) and
D.W. Hughes (1994). They were both invaluable
in finding starting points for the primary sources on the history of the discovery of the
asteroids and their diameters, respectively. I also would like to acknowledge R.A. Kowalski
(1999, private communication) whose talk "A Brief History of Minor Planet Research," describes
a somewhat different picture than the one I first formed on this subject.
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