Michael William Feast

Last updated
Michael William Feast
Born(1926-12-29)29 December 1926
Deal, Kent, England
Died1 April 2019(2019-04-01) (aged 92)
Cape Town, South Africa
Scientific career
Fields Astronomy

Michael William Feast (29 December 1926 [1] [2] – 1 April 2019) 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. [3]

South African Astronomical Observatory observatory

South African Astronomical Observatory (SAAO) is the national centre for optical and infrared astronomy in South Africa. It was established in 1972. The observatory is run by the National Research Foundation of South Africa. The facility's function is to conduct research in astronomy and astrophysics. The primary telescopes are located in Sutherland, which is 370 kilometres (230 mi) from Observatory, Cape Town, where the headquarters is located.

University of Cape Town university in Cape Town, South Africa

The University of Cape Town (UCT) is a public research university located in Cape Town in the Western Cape province of South Africa. UCT was founded in 1829 as the South African College making it the oldest higher education institute in South Africa. In terms of full university status, it is jointly the oldest university in South Africa and the oldest extant university in Sub-Saharan Africa alongside Stellenbosch University which received full university status on the same day in 1918.

His research focussed on the structure of the Milky Way, the Magellanic Clouds, and the cosmic distance ladder using variable stars. [4] [5]

Milky Way Spiral galaxy containing our Solar System

The Milky Way is the galaxy that contains the Solar System, with the name describing the galaxy's appearance from Earth: a hazy band of light seen in the night sky formed from stars that cannot be individually distinguished by the naked eye. The term Milky Way is a translation of the Latin via lactea, from the Greek γαλαξίας κύκλος. From Earth, the Milky Way appears as a band because its disk-shaped structure is viewed from its outer rim. Galileo Galilei first resolved the band of light into individual stars with his telescope in 1610. Until the early 1920s, most astronomers thought that the Milky Way contained all the stars in the Universe. Following the 1920 Great Debate between the astronomers Harlow Shapley and Heber Curtis, observations by Edwin Hubble showed that the Milky Way is just one of many galaxies.

Magellanic Clouds two irregular dwarf galaxies orbiting the Milky Way galaxy within the Local Galactic Group

The Magellanic Clouds are two irregular dwarf galaxies visible in the Southern Celestial Hemisphere; they are members of the Local Group and are orbiting the Milky Way galaxy. Because both show signs of a bar structure, they are often reclassified as Magellanic spiral galaxies. The two galaxies are:

Cosmic distance ladder succession of methods by which astronomers determine the distances to celestial objects

The cosmic distance ladder is the succession of methods by which astronomers determine the distances to celestial objects. A real direct distance measurement of an astronomical object is possible only for those objects that are "close enough" to Earth. The techniques for determining distances to more distant objects are all based on various measured correlations between methods that work at close distances and methods that work at larger distances. Several methods rely on a standard candle, which is an astronomical object that has a known luminosity.

Career and honours

Feast holds the degrees of BSc (Hons) and PhD from London [6] From 1949 to 1951 he worked with Gerhard Herzberg at the National Research Council in Ottawa, Ontario, Canada, following which from 1952 to 1974 he was at the Radcliffe Observatory, Pretoria [7] He was also director of the South African Astronomical Observatory from 1976 to 1992. [8]

Gerhard Herzberg German-Canadian physicist and physical chemist

Gerhard Heinrich Friedrich Otto Julius Herzberg, was a German-Canadian pioneering physicist and physical chemist, who won the Nobel Prize for Chemistry in 1971, "for his contributions to the knowledge of electronic structure and geometry of molecules, particularly free radicals". Herzberg's main work concerned atomic and molecular spectroscopy. He is well known for using these techniques that determine the structures of diatomic and polyatomic molecules, including free radicals which are difficult to investigate in any other way, and for the chemical analysis of astronomical objects. Herzberg served as Chancellor of Carleton University in Ottawa, Ontario, Canada from 1973 to 1980.

National Research Council (Canada) Primary national research and technology organization of the Government of Canada

The National Research Council is the primary national research and technology organization (RTO) of the Government of Canada, in science and technology research and development. The Minister of Innovation, Science, and Economic Development is responsible for the National Research Council. The transformation of the NRC into an RTO that focuses on "business-led research" was part of the federal government's Economic Action Plan. On 7 May 2013, the NRC launched its new "business approach" in which it offered four business lines: strategic research and development, technical services, management of science and technology infrastructure and NRC-Industrial Research Assistance Program (IRAP). With these services, NRC intended to shorten the gap between early stage research and development and commercialization. At one point, NRC had over 30 approved programs.

Ottawa Federal capital city in Ontario, Canada

Ottawa is the capital city of Canada. It stands on the south bank of the Ottawa River in the eastern portion of southern Ontario. Ottawa borders Gatineau, Quebec; the two form the core of the Ottawa–Gatineau census metropolitan area (CMA) and the National Capital Region (NCR). As of 2016, Ottawa had a city population of 934,243 and a metropolitan population of 1,323,783 making it the fourth-largest city and the fifth-largest CMA in Canada. In June 2019, the City of Ottawa estimated it had surpassed a population of 1 million.

He received the DeBeers Medal [9] from the South African Institute of Physics in 1992 and the Gill Medal from the Astronomical Society of Southern Africa in 1983. [10] [11] Feast was an Honorary Fellow of the Royal Astronomical Society, [1] Fellow of the Royal Society of South Africa. [12] The University of Cape Town awarded him an honorary Doctor of Science degree in 1993. [13] Feast was an editor of the journal Monthly Notices of the Royal Astronomical Society . [14]

Royal Astronomical Society learned society

The Royal Astronomical Society (RAS) is a learned society and charity that encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. Its headquarters are in Burlington House, on Piccadilly in London. The society has over 4,000 members ("Fellows"), most of them professional researchers or postgraduate students. Around a quarter of Fellows live outside the UK.

The Royal Society of South Africa is a learned society composed of eminent South African scientists and academics. The Society was granted its royal charter by King Edward VII in 1908, nearly a century after Capetonians first began to conceive of a national scholarly society. The 1877 founder and first President of the Society was Sir Bartle Frere (1815–1884).

<i>Monthly Notices of the Royal Astronomical Society</i> journal

Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal covering research in astronomy and astrophysics. It has been in continuous existence since 1827 and publishes letters and papers reporting original research in relevant fields. Despite the name, the journal is no longer monthly, nor does it carry the notices of the Royal Astronomical Society.

His most frequently cited paper (440 times [15] ) relates to his pioneering study of the brightest stars in the Magellanic Clouds with Thackeray and Wesselink; [16] see, for example, Hodge (1999). [17]

Much of his work has related to the Cepheid period-luminosity relation, [18] for example that on its zero-point as determined via the Hipparcos satellite [19]

Period-luminosity relation

In astronomy, a period-luminosity relation is a relationship linking the luminosity of pulsating variable stars with their pulsation period. The best-known relation, for Classical Cepheid variables, is sometimes called Leavitt's law. Discovered in 1908 by Henrietta Swan Leavitt, the relation established Cepheids as foundational indicators of cosmic benchmarks for scaling galactic and extragalactic distances.

He died in his sleep on 1 April 2019, aged 92. [1]

Related Research Articles

Large Magellanic Cloud irregular galaxy, satellite of the Milky Way

The Large Magellanic Cloud (LMC) is a satellite galaxy of the Milky Way. At a distance of about 50 kiloparsecs, the LMC is the second- or third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal and the possible dwarf irregular galaxy known as the Canis Major Overdensity. Based on readily visible stars and a mass of approximately 10 billion solar masses, the diameter of the LMC is about 14,000 light-years (4.3 kpc), making it roughly one one-hundredth as massive as the Milky Way. This makes the LMC the fourth-largest galaxy in the Local Group, after the Andromeda Galaxy (M31), the Milky Way, and the Triangulum Galaxy (M33).

Cepheid variable type of variable star

A Cepheid variable is a type of star that pulsates radially, varying in both diameter and temperature and producing changes in brightness with a well-defined stable period and amplitude.

S Doradus variable star in the Large Magellanic Cloud

S Doradus is located 160,000 light-years away, and is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite of the Milky Way. It is a luminous blue variable and one of the most luminous stars known, but so far away that it is invisible to the naked eye.

Andrew David Thackeray, was an astronomer trained at Cambridge University. He served as director of the Radcliffe Observatory for 23 years.

IC 2944 H II region and open cluster in the constellation Centaurus

IC 2944, also known as the Running Chicken Nebula or the λ Centauri Nebula, is an open cluster with an associated emission nebula found in the constellation Centaurus, near the star λ Centauri. It features Bok globules, which are frequently a site of active star formation. However, no evidence for star formation has been found in any of the globules in IC 2944.

R136 super star cluster

R136 is the central concentration of stars in the NGC 2070 star cluster, which lies at the centre of the Tarantula Nebula in the Large Magellanic Cloud. When originally named it was an unresolved stellar object but is now known to include 72 class O and Wolf–Rayet stars within 5 parsecs of the centre of the cluster. The extreme number and concentration of young massive stars in this part of the LMC qualifies it as a starburst region.

HD 95109 star

HD 95109 is a Classical Cepheid variable, a type of variable star, in the constellation Carina. Its apparent magnitude is 6.86.

HD 37974 star

HD 37974 a variable B[e] hypergiant in the Large Magellanic Cloud. It is surrounded by an unexpected dust disk.

V598 Puppis is the name given to a nova in the Milky Way Galaxy. USNO-A2.0 0450-03360039, the catalog number for the star, was discovered to be much brighter than normal in X-ray emissions on October 9, 2007, by the European Space Agency's XMM-Newton telescope. Ultimately, the star was confirmed to 600 times brighter than normal by the Magellan-Clay telescope Magellan-Clay telescope at Las Campanas Observatory in Chile.

U Aquilae is a binary star system in the constellation Aquila, Located approximately 614 parsecs (2,000 ly) away from Earth.

Type II Cepheid

Type II Cepheids are variable stars which pulsate with periods typically between 1 and 50 days. They are population II stars: old, typically metal-poor, low mass objects.

Classical Cepheid variable type of variable star

Classical Cepheids are a type of Cepheid variable star. They are population I variable stars that exhibit regular radial pulsations with periods of a few days to a few weeks and visual amplitudes from a few tenths of a magnitude to about 2 magnitudes.


R136a2 is a Wolf-Rayet star residing near the center of the R136, the central concentration of stars of the large NGC 2070 open cluster in the Tarantula Nebula, a massive H II region in the Large Magellanic Cloud which is a nearby satellite galaxy of the Milky Way. It has one of the highest confirmed masses and luminosities of any known star, at about 195 M and 4.3 million L respectively.

Ian Stewart Glass is an infrared astronomer and scientific historian living in Cape Town, South Africa.

U Vulpeculae is a variable and binary star in the constellation Vulpecula.

Adriaan Jan Wesselink (1909–1995) was a Dutch astronomer who worked successively in the Netherlands, South Africa and the United States. He specialised in observing and understanding the characteristics of stars, particularly variable stars.

R145 star

R145 is a spectroscopic binary star in the Tarantula Nebula in the Large Magellanic Cloud located in the constellation Dorado. Both components are amongst the most luminous known.

R85 star

R85 is a candidate luminous blue variable located in the LH-41 OB association in the Large Magellanic Cloud.

R71 is a star in the Large Magellanic Cloud (LMC) in the constellation Mensa. It is classified as a luminous blue variable and is one of the most luminous stars in the LMC.


  1. 1 2 3 Whitelock, Patricia (1 June 2019). "Michael William Feast 1926–2019". Astronomy & Geophysics . 60 (3): 3.12. Bibcode:2019A&G....60c3.12W. doi: 10.1093/astrogeo/atz143 .
  2. Uwechue, Raph (1991). Africa Who's who. Africa Journal Limited. p. 665. ISBN   978-0-903274-17-3.
  3. "Honorary Professor Michael W. Feast". Department of Astronomy, University of Cape Town. Retrieved March 18, 2013.
  4. Warner, Brian (1999). Warner, B. (ed.). Introduction. Variable Stars and Galaxies, a Symposium in Honour of Professor Michael W. Feast ..., Conference Series Vol. 30. Astronomical Society of the Pacific.
  5. Webb, Stephen (1999). Measuring the Universe: The Cosmological Distance Ladder. Springer. p. 155.
  6. Feast, Michael. On the Spectra of Gases Exhibited in the High Voltage Arc (PhD). University of London.
  7. Thackeray, A.D. (1972). The Radcliffe Observatory. The Radcliffe Trust..
  8. "South African Astronomical Observatory". Archived from the original on 2013-09-28.
  9. "Past winners of the De Beers Gold Medal". South African Institute of Physics. Retrieved March 18, 2013.
  10. Anon (1983). "Citation". Monthly Notes of the Astronomical Society of Southern Africa. 42: 16. Bibcode:1983MNSSA..42...16.
  11. "Gill Medal". Astronomical Society of South Africa. Archived from the original on May 3, 2012. Retrieved March 18, 2013.
  12. "Royal Society of SA Fellows". Royal Society of South Africa. Archived from the original on August 14, 2012. Retrieved March 18, 2013.
  13. "Honorary degrees awarded". University of Cape Town. Archived from the original on March 4, 2013. Retrieved March 18, 2013.
  14. "RAS Committee Members". RAS website. Royal Astronomical Society . Retrieved 3 September 2013.
  15. "SAO/NASA ADS Custom Query Form Mon Mar 18 14:32:27 2013". Adsabs.harvard.edu. Retrieved 2013-03-18.
  16. Feast, M.W.; Thackeray, A.D.; Wesselink, A.J. (1960). "The Brightest Stars in the Magellanic Clouds". Monthly Notices of the Royal Astronomical Society. 121: 337–385. Bibcode:1960MNRAS.121..337F. doi:10.1093/mnras/121.4.337.
  17. Hodge, Paul (1999). Chu, Y.H.; et al. (eds.). Magellanic Cloud Studies, Past and Future. New Views of the Magellanic Clouds, IAU Symposium 190. 190. IAU. pp. 3–7.
  18. Feast, M.W.; Walker, A.R. (1987). "Cepheids as Distance Indicators". Annual Review of Astronomy and Astrophysics. Annual Reviews Inc. 25: 345–375. Bibcode:1987ARA&A..25..345F. doi:10.1146/annurev.aa.25.090187.002021.
  19. Feast, M.W.; Catchpole, R.M. (1997). "The Cepheid period-luminosity zero-point from HIPPARCOS trigonometrical parallaxes". Monthly Notices of the Royal Astronomical Society. 286: L1. Bibcode:1997MNRAS.286L...1F. doi:10.1093/mnras/286.1.L1.