Johann Palisa
Relevant Non-Istrians


Johann Palisa
(1848-1925)

Early Asteroid Research in Austria

ohann Palisa, the astronomer, was born on December 6, 1948 in Troppau, Silesia (now Opava, Czech Republic) and died on May 2, 1925 in Vienna, Austria. He is best known for his discovery of 120 asteroids, including 142 Polana and 183 Istria. He also prepared two catalogs containing the positions of almost 4,700 stars. 

Abstract

Johann Palisa discovered the first asteroid (136) Austria in 1874 at the Austrian Naval Observatory in Pola, Istria. After discovering 27 more objects in Pola, Palisa was offered a position in Vienna where he had the new large refractor (at that time the largest telescope in the world) at his disposal. During his career he discovered a total of 121 asteroids, making him the most successful discoverer of minor planets using visual techniques.

Joseph Rheden used the new technology of photography to continue the program. He concentrated on measurements of positions for the purpose of orbit determination. At the same time Theodor Oppolzer introduced a new method of orbit determination which was applied to the observations.

International cooperations resulted among other projects in the production of the Wolf-Palisa charts, and, much later, in a remeasurement of the original plates and use of the data for the improvement of orbit determination.

This successful field of research came to an end because of the deterioration of observing conditions in Vienna, financial problems due to the political and economic decline following World War I and the death of Palisa in 1925.


The science of astronomy has a long tradition at the University of Vienna in Austria. Records show that astronomy has been persued since the middle ages. However, for most of the time the work of the Austrian astronomers was hampered by the lack of suitable telescopes. The largest telescope of the old Vienna Observatory, until the middle of the 19th century located on the roof of the old building of the University near the center of Vienna, had a diameter of only 6 inches. As a consequence astronomers in Vienna turned to other areas of interest; they became specialists in calculating orbits of planets and comets.

During the 19th century Austria was a seafaring nation. To support the navigation of her ships at sea, Austria had, as all seafaring nations had to have, a naval observatory.

The Austro-Hungarian Imperial Naval Observatory in Pola, Istria Photograph courtesy of Österreichisches Staatsarchiv

The oldest astronomical observatory in present-day Croatia was established in Pula in 1871 as part of the Hydrographical Institute of the Imperial and Royal Navy. It was located in Pola (now Pula) near Fiume (now Rijeka) at the south end of the Istria peninsula along the eastern shore of the Adriatic Sea. Pola was the "Kriegshafen" (literally: war harbour) of the Austro-Hungarian Empire.

Palisa briefly was an assistant astronomer at the observatories in Vienna and Geneva before being appointed director (1871 or 1872-80) of the observatory at Pola, a position that carried with it the rank of commander. His main area of responsibility was the "time service", i.e. the determination and maintenance of the precise time. While the time service was a necessary and demanding task it is easy to imagine that it was not totally satisfying for a reasearch-oriented person.

Following a suggestion by his teacher Theodor von Oppolzer (1841-1886), Palisa started to observe Minor Planets. Although the telescope was, at 6 inches of diameter, not any more powerful than the telescope in Vienna, the observing conditions were considerably better.

In 1874 he found his first object and named it in honour of the Empire and according to the prevailing naming conventions, (136) Austria (Palisa 1874). During his tenure in Pola, Palisa discovered a total of 28 objects [including Polana, Adria and Istria]. 

 

ASTEROIDS

No.

Name

Date discovered

136

Austria

Wednesday, March 18, 1874

137

Meliboea

Tuesday, April 21, 1874

140

Siwa

Tuesday, October 13, 1874

142

Polana

Thursday, January 28, 1875 

143

Adria

Tuesday, February 23, 1875

151

Abundantia

Monday, November 01, 1875

153

Hilda

Tuesday, November 02, 1875 

155

Scylla

Monday, November 08, 1875

156

Xanthippe

Monday, November 22, 1875

178

Belisana

Tuesday, November 06, 1877

182

Elsa

Thursday, February 07, 1878 

183

Istria

Friday, February 08, 1878 

184

Dejopeja

Thursday, February 28, 1878 

192

Nausikaa 

Monday, February 17, 1879

195

Eurykleia

Saturday, April 19, 1879 

197

Arete

Wednesday, May 21, 1879 

201

Penelope

Thursday, August 07, 1879

204

Kallisto

Wednesday, October 08, 1879

205

Martha

Monday, October 13, 1879

207

Hedda

Friday, October 17, 1879 

208

Lacrimosa

Tuesday, October 21, 1879

210

Isabella

Wednesday, November 12, 1879

211

Isolda

Wednesday, December 10, 1879 

212

Medea

Friday, February 06, 1880

214

Aschera

Sunday, February 29, 1880

216

Kleopatra

Saturday, April 10, 1880

218

Bianca

Saturday, September 04, 1880

219

Thusnelda

Thursday, September 30, 1880

While the discovery of Minor Planets was important to him, he placed even greater importance on the re-observation of objects which had been discovered by others: this was to make sure that good orbits could be determined.

142 Polana 
(discovered January 28, 1875)

Dimenzije 57,1 km
Velika poluosa 2,471 a.j.
Ekscenticitet orbite 0,137
Nagib orbite prema ekliptici 2°14'
Sidericki period 3,8 godina
Apsolutna magnituda 10,27
Albedo 0,04
Polana
Orbite: Merkur, Venera, Zemlja, Mars, asteroid, Jupiter. V = Vernal equinox

183 Istria
(discovered February 8, 1878)

Dimenzije 36 km
Velika poluosa 2,794 a.j.
Ekscenticitet orbite 0,348
Nagib orbite prema ekliptici 26° 25'
Sidericki period 4,7 godina
Apsolutna magnituda 9,68
Albedo 0,16
Istria

Palisa's mentor von Oppolzer had published a book on orbit calculations (Oppolzer 1870). Based on the "Theoria Motus" (Gauss 1809) he derived useful criteria which allow to decide whether or not an orbit can be determined uniquely from three complete observations (right ascension and declination) at three different epochs. Von Oppolzer calculated orbits and ephemerides for 165 comets and minor planets.

From 1880 to 1919 Palisa was a member of the staff at the Vienna Observatory. It is interesting to speculate why the then emerging photographic technique was not used. One reason is probably that the lens of the large refractor was optimised for the visual wavelength range, which made it not suitable for the blue-sensitive emulsions of the time (Spitaler 1891). Another reason is presumably the small field of view, which would have necessitated a large number of exposures to cover reasonable areas of the sky.

In any case, by 1891 when the photographic plate was first used in astronomy, Palisa had found 83 of the 120 asteroids he eventually identified by visual observation alone. He re-observed many of the objects which had been discovered photographically by Max Wolf in Heidelberg, thus assuring the good quality of the orbital elements. The close collaboration with Heidelberg also resulted in the production of the Wolf-Palisa stellar charts. Deep wide-field survey plates, taken in Heidelberg, were converted to high-precision maps in Vienna by superimposing precise coordinate grids. The practical value of these charts for the asteroid observers was that anything in the field of view which was not on the chart was, in all likelihood, a minor planet, a fact which usually could be substantiated by re-observation during the same night, or during following nights. 

A total of 210 star charts, covering the area around the ecliptic, were published in 1899, 1902, and 1908. Production of the charts was discontinued after the First World War, because the prevailing international conditions made it impossible to sell the product.
Joseph Rheden
Joseph Rheden

In 1907 the "Normalastrograph" (plate scale 1 arcmin per mm, lens optimized for blue sensitive plates) was put in operation at the Vienna Observatory. Joseph Rheden (1873-1946), Palisa's son-in-law, used it to continue the observations of Minor Planets and of comets (Rheden 1913).

He concentrated on the determination of positions for the purpose of orbit determination. Approximately 1000 of the plates taken by Rheden are still in the plate archive of the Observatory. Most of the plates were used for search and discovery, with visual follow-up. Lacking suitable high-precision measuring equipment the plates were not measured at the time. Only in the 1960ies the plates were measured in the framework of a thesis project (Pendl 1969) and the data supplied to the Minor Planet Center (then located in Cincinnati). Accurate determination of positions was carried out and published (Minor Planet Circulars 2698, 2823, 2870, 2907).

As a consequence of the explosive growth of the city of Vienna around the turn of the century the Observatory had been engulfed by the urban environment. Observing conditions further worsened due to rapid industrialisation and increasing light pollution. During and after the First World War the political and economic situation deteriorated, caused by the breakup of the Austro-Hungarian Empire combined with an economic crisis and hyperinflation, and brought most of the astronomical research in Vienna to a standstill.

The last observations of Minor Planets, which still can be considered a continuation of the original programme, were carried out by Alois Purgathofer (1925-1984), at the occasion of the opposition of the Minor Planet (51) Nemausa in 1954 (Purgathofer 1955).

One of the objects discovered by Palisa, the asteroid (719) Albert, was lost after the initial discovery. Considerable search efforts were made at the time (Palisa 1912, Curtis 1913) and later (Kristensen and West 1989), but the object remained lost. In a remarkable coincidence (719) Albert was recovered by J.A Larsen of the Spacewatch Project (Larsen et al. 2000) several days before the presentation of the paper that is the major textual portion of this web page.

Acknowledgements:

Thanks go to Monika Rode-Paunzen and to Lars Lindberg Christensen.

References:

  • Curtis, H. D.,1913. Search for asteroid 1911 MT (719), Albert. Lick Obs. Bull. 249 (8), 47-48
  • Gauss, C. F., 1809, Theoria Motus Corporum Coelestium In Sectionibus Conicis Solem Ambientium, Hamburg
  • Kristensen, L. K., West, R. M., 1989. On the lost minor planet (719) Albert. Astron. Astrophys. 218, 317-324
  • Larsen, J. A. et al., 2000, IAU Circ. 7420
  • Oppolzer, Th., 1870, 1880. Lehrbuch zur Bahnbestimmung von Planeten und Kometen. 2 Vol. Leipzig.
  • Palisa, J., 1874. Entdeckung eines Planeten. Astron. Nachr. 83, 207
  • Palisa, J., 1912. Photographische Beobachtungen des Planeten 1911 MT. Astronomischer Kalender für 1913. Wien, 138-143
  • Pendl, E., 1969. Die Neuvermessung von 140 Aufnahmen Kleiner Planeten sowie ein Programm zur Berechnung vorläufiger Bahnen, Diss. Univ. Wien.
  • Purgathofer, A., 1955. 165 Positionen des kleinen Planeten (51) Nemausa während der Opposition 1954. Mitt. Univ. Stwte Wien 7, 235-258
  • Rheden, J., 1913. Photographische Aufnahmen des Halleyschen Kometen und der Kometen des Jahres 1911, ausgeführt am photographischen Refraktor der k. k. Sternwarte in Wien. Ann. Univ. Stwte Wien, XXIII, 1-28
  • Spitaler, R. 1891, Zeichnungen und Photographien am Grubbschen Refraktor in den Jahren 1885 bis 1890. Ann.Univ. Stwte Wien VII, 183-205

Credits:

*Affiliated to the Astrophysics Division, Space Science Department, European Space Agency

Sources:

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Created: Wednesday, May 15, 2002; Last updated: Thursday, November 24, 2011
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