John Caister Bennett

Last updated

John Caister "Jack" Bennett (born 6 April 1914 in Estcourt, Natal, died 30 May 1990 in Pretoria), was a South African civil servant and amateur astronomer. [1] His mother was British and his father was from Tasmania. He attended school in Ficksburg and began to work in public service after graduating in 1934, initially in the forestry administration in Elgin before moving to the administration of Transvaal Province in Pretoria. During World War II he served as a soldier in South Africa, Egypt and Italy. In 1974 he retired from the public service. From 1985 he began to suffer from arthritis and soon afterwards his health deteriorated so much that he had to sell his house in Pretoria's Riviera neighborhood and move into a nursing home. He died on 30 May 1990 at the age of 76. [2] [3] [4] [5]

Contents

Amateur astronomer

Bennett's interest in astronomy began early when his mother showed him the starry sky with the Southern Cross and the planets on the way home from evening church visits and told him about her observation of Halley's Comet on its return in 1910.

After the war he started looking for comets with a 60 mm refractor, and from 1958 he observed the new artificial satellites. For this purpose, he bought a light 125 mm refractor with an altazimuth mount in 1961, which later became his favorite instrument. He became a member of the Astronomical Society of Southern Africa and the British Astronomical Association at an early age.

Although he discovered comets as early as the 1960s, he was either not the first discoverer, or the comets he found were short-lived and could not be observed again. During this time (1969 [6] to 1974 [7] ) he systematically compiled a catalog of 152 objects in the southern sky that could be mistaken for a comet. This list, later called the Bennett catalog, [8] is still today a valuable aid for comet hunters, a "southern Messier catalog".

Every year he spent some 150 hours looking for comets in the backyard of his house in Pretoria and by chance discovered on 16 July 1968 an unusual appearance in the galaxy Messier 83 (NGC 5236) in the constellation Hydra. This was recognized shortly afterwards by professional astronomers as a supernova (SN 1968L). Bennett was the first person to visually discover a supernova since the invention of the telescope.

With his 125 mm refractor he finally discovered his first comet, C/1969 Y1 (Bennett), after a search for more than 333 hours on 28 December 1969. This became a "Great Comet" that could be seen with the naked eye the following year. His second comet discovery occurred on 13 November 1974 after a further 482 hours of search. This was the inconspicuous C/1974 V2 (Bennett).

In later years he bought a Celestron C-8, but despite 30 to 40 hours of searching annually for the next 10 years, he had no further success in hunting comets, partially due to increasing light pollution. In addition to comets, he was also interested in meteors and variable stars. In the years before his death, he had to give up observing entirely and donated his famous 125 mm refractor to the University of South Africa. [2] [3] [4] [5]

Discoveries

Honors

After his death, the Pretoria Centre established the ASSA's annual Jack Bennett Award for contributions to astronomy and the Centre.

Related Research Articles

<span class="mw-page-title-main">Crab Nebula</span> Supernova remnant in the constellation Taurus

The Crab Nebula is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The common name comes from William Parsons, 3rd Earl of Rosse, who observed the object in 1842 using a 36-inch (91 cm) telescope and produced a drawing that looked somewhat like a crab. The nebula was discovered by English astronomer John Bevis in 1731, and it corresponds with a bright supernova recorded by Chinese astronomers in 1054. The nebula was the first astronomical object identified that corresponds with a historically-observed supernova explosion.

Boyden Observatory is an astronomical research observatory and science education centre located in Maselspoort, 20 kilometres (12 mi) north-east of the city of Bloemfontein in Free State, South Africa. The observatory is managed by the Physics Department of the University of the Free State (UFS). The Friends of Boyden assist the observatory as a public support group, organising open evenings and protecting its public interest. Boyden also makes use of members of ASSA Bloemfontein Centre, the amateur astronomy club of the city, for presenters and telescope assistants.

Alexander Forbes Irvine Forbes was a South African astronomer, architect and artist, best known for his discovery of periodic comets.

William Stephen FinsenFRAS was a South African astronomer. He discovered a number of double stars and took many photographs of Mars. He developed the Finsen eyepiece interferometer to measure very close double stars. He was the final director of Union Observatory in South Africa from 1957 to 1965.

The Astronomical Society of Southern Africa (ASSA), formed in 1922, is a widespread body consisting of both amateur and professional astronomers. There are eight autonomous centres throughout Southern Africa.

Alan William James Cousins FRAS was a South African astronomer. His career spanned 70 years during which time he concentrated on the measurement of variable stars, including the measurement of the two sinusoidal periods of Gamma Doradus. The UBV photometric system for measuring stellar fluxes he devised in his 1990s became a standard known as the "Cousins system".

<span class="mw-page-title-main">V842 Centauri</span> Nova in the constellation Centaurus seen in 1986

V842 Centauri, also known as Nova Centauri 1986, was a nova which occurred in 1986 in the constellation Centaurus. It was discovered by Robert H. McNaught of Siding Spring Observatory in Australia, on 22 November 1986. At the time of its discovery, it had an apparent magnitude of 5.6. It reached a peak magnitude of 4.6 one and a half days later, making it easily visible to the naked eye.

<span class="mw-page-title-main">Sigma Canis Majoris</span> Variable star in the constellation Canis Major

Sigma Canis Majoris, also named Unurgunite, is a variable star in the southern constellation of Canis Major. It is approximately 1,120 light-years from the Sun and has an average apparent visual magnitude of +3.41.

<span class="mw-page-title-main">Hoba meteorite</span> Largest known intact meteorite

The Hoba meteorite, short for Hoba West, is a meteorite that lies on the farm of the same name, not far from Grootfontein, in the Otjozondjupa Region of Namibia. It has been uncovered, but because of its large mass, has never been moved from where it fell. The main mass is estimated at more than 60 tonnes. It is the largest known intact meteorite and about twice as massive as the largest fragment of either the Cape York meteorite's 31-tonne Ahnighito kept in the American Museum of Natural History or the Campo del Cielo's 31-tonne Gancedo in Argentina. It is also the most massive naturally occurring piece of iron known on Earth's surface. The name "Hoba" comes from a Khoekhoegowab word meaning "gift". Following donation to the government in 1987, a visitor centre was constructed with a circular stone access and seating area.

<span class="mw-page-title-main">Comet Bennett</span> Icy small Solar System body; passed closest to Earth in 1970

Comet Bennett, formally known as C/1969 Y1, was one of the two bright comets observed in the 1970s, along with Comet West and is considered a great comet. The name is also borne by an altogether different comet, C/1974 V2. Discovered by John Caister Bennett on December 28, 1969 while still almost two AUs from the Sun, it reached perihelion on March 20, passing closest to Earth on March 26, 1970 as it receded, peaking at magnitude 0. It was last observed on February 27, 1971.

<span class="mw-page-title-main">Gart Westerhout</span> Dutch-American astronomer (1927–2012)

Gart Westerhout was a Dutch-American astronomer. Well before completing his university studies at Leiden, he had already become well-established internationally as a radio astronomer in the Netherlands, specializing in studies of radio sources and the Milky Way Galaxy based on observations of radio continuum emissions and 21-cm spectral line radiation that originates in interstellar hydrogen. He emigrated to the United States, became a naturalized citizen, and held a number of important scientific and management positions in academic and government institutions.

<span class="mw-page-title-main">Grubb Parsons</span> Historic manufacturer of telescopes

Grubb Parsons was a historic manufacturer of telescopes, active in the 19th and 20th centuries. They built numerous large research telescopes, including several that were the largest in the world of their type.

25 Scorpii is a star in the zodiac constellation of Scorpius, located about 920 light years away from the Sun. Its apparent magnitude is 6.71, so its apparent brightness is at the limit of human eyesight and can only be seen under excellent conditions, according to the Bortle scale. The object is moving closer to the Earth with a heliocentric radial velocity of −1.3 km/s. It is a proposed member of the Scorpius–Centaurus association.

HD 108541, also known by its Bayer designation u Centauri is a star located in the constellation Centaurus, It is also known as HR 4748. The apparent magnitude of the star is about 5.4, meaning it is only visible to the naked eye under excellent viewing conditions. Its distance is about 440 light-years, based on its parallax measured by the Hipparcos astrometry satellite. The spectral type of HD 108541 is B8/9V, meaning it is a late B-type main sequence star. These types of stars are a few times more massive than the Sun, and have effective temperatures of about 10,000 to 30,000 K. HD 108541 is just under 3 times more massive than the Sun and has a temperature of about 11,000 K.

HD 120987 is a star system located in the constellation Centaurus. HD 120987 is a quintuple star system located 50 pc from the Sun. The system has an apparent magnitude of 5.565. Based on the system's parallax, it is located some 172 light-years away.

<span class="mw-page-title-main">Pi Piscis Austrini</span> Star in the constellation Piscis Austrinus

Pi Piscis Austrini, Latinized from π Piscis Austrini, is binary star system in the southern constellation of Piscis Austrinus, near the eastern constellation border with Sculptor. It has a yellow-white hue and is visible to the naked eye as a dim point of light with an apparent visual magnitude of 5.12. The system is located at a distance of 92 light-years from the Sun based on parallax. Its radial velocity is poorly constrained, but it appears to be drifting closer at a rate of around −6 km/s. Pi Piscis Austrini is moving through the galaxy at a velocity of 16.3 km/s relative to the Sun. Its projected galactic orbit carries it between 24,000 and 37,500 light-years from the center of the galaxy.

Michael William Feast was a British-South African astronomer. He served as Director of the South African Astronomical Observatory from 1976–1992, then became a professor at the University of Cape Town.

<span class="mw-page-title-main">NGC 1288</span> Barred spiral galaxy in the constellation Fornax

NGC 1288 is an intermediate barred spiral galaxy located about 196 million light years away in the constellation Fornax. In the nineteenth century, English astronomer John Herschel described it as "very faint, large, round, very gradually little brighter middle." The morphological classification of SABc(rs) indicates weak bar structure across the nucleus (SAB), an incomplete inner ring orbiting outside the bar (rs), and the multiple spiral arms are moderately wound (c). The spiral arms branch at intervals of 120° at a radius of 30″ from the nucleus. The galaxy is most likely surrounded by a dark matter halo, giving it a mass-to-light ratio of 14 M/L.

<span class="mw-page-title-main">Royal Observatory, Cape of Good Hope</span> Observatory

The Royal Observatory, Cape of Good Hope, is the oldest continuously existing scientific institution in South Africa. Founded by the British Board of Longitude in 1820, it now forms the headquarters building of the South African Astronomical Observatory.

<span class="mw-page-title-main">U Microscopii</span> Star in the constellation Microscopium

U Microscopii is a Mira variable star in the constellation Microscopium. It ranges from magnitude 7 to 14.4 over a period of 334 days. The Astronomical Society of Southern Africa in 2003 reported that observations of U Microscopii were very urgently needed as data on its light curve was incomplete.

References

  1. "J. C. Bennett (amateur astronomer)". Astronomical Society of Southern Africa. Retrieved 12 September 2021.
  2. 1 2 Jones, John Spencer (1994). "Obituary J. C. Bennett (1914-1990)". Quarterly Journal of the Royal Astronomical Society. 35: 353. Bibcode:1994QJRAS..35..353J . Retrieved 12 September 2021.
  3. 1 2 Fleet, Richard (1991). "John Caister Bennett 1914-1990". Journal of the British Astronomical Association. 101 (6): 367. Bibcode:1991JBAA..101..367F . Retrieved 12 September 2021.
  4. 1 2 da S. Campos, J. A. (1990). "Obituary John Caister Bennett (1914-1990)" (PDF). Monthly Notes of the Astron. Soc. Southern Africa. 49 (9&10): 113–115. Bibcode:1990MNSSA..49..113C . Retrieved 12 September 2021.
  5. 1 2 Marsden, Brian (1990). "Jack Bennett – An Appreciation" (PDF). Monthly Notes of the Astron. Soc. Southern Africa. 49 (9&10): 115. Bibcode:1990MNSSA..49..113C . Retrieved 12 September 2021.
  6. Bennett, J. C. (1969). "Comet-Hunting in Southern Skies". Monthly Notes of the Astron. Soc. Southern Africa. 28 (8): 80–88. Bibcode:1969MNSSA..28...80B . Retrieved 12 September 2021.
  7. Bennett, J. C. (1974). "Some Objects of Interest in the Southern Sky". Monthly Notes of the Astron. Soc. Southern Africa. 33 (8): 107–108. Bibcode:1974MNSSA..33..107B . Retrieved 12 September 2021.
  8. "Jack Bennett's catalogue of deep sky objects". Astronomical Society of Southern Africa. Retrieved 12 September 2021.
  9. Smith, R. F. (1970). "Presentation of the Gill Medal to Mr. J. C. Bennett". Monthly Notes of the Astron. Soc. Southern Africa. 29 (9): 123. Bibcode:1970MNSSA..29..123S . Retrieved 12 September 2021.
  10. "About the BAA: Awards and Medals". British Astronomical Association. Archived from the original on 11 May 2020. Retrieved 12 September 2021.
  11. "Honours for Jack Bennett". Monthly Notes of the Astron. Soc. Southern Africa. 48 (11&12): 113. 1989. Bibcode:1989MNSSA..48..113. Retrieved 12 September 2021.
  12. "(4093) Bennett = 1981 UG21 = 1981 UG9 = 1986 VD". Minor Planet Center. IAU. Retrieved 12 September 2021.