Gerrit Verschuur

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Gerrit L. Verschuur
Verschuur Gerrit.jpg
Gerrit L. Verschuur in 1999
Born1937
Cape Town
NationalityAmerican
Naturalized 1975
Alma mater Rhodes University
University of Manchester
Scientific career
FieldsRadio astronomy
Institutions University of Memphis

Gerrit L. Verschuur (born in 1937 in Cape Town, South Africa) is an American scientist who is best known for his work in radio astronomy. Though a pioneer in that field, Verschuur is also an author (he has written about astronomy, natural disasters, and earth sciences), inventor, adjunct professor of physics for the University of Memphis, and Astronomer Emeritus - Arecibo Observatory and now semi-retired. He served for a time as the Chief Scientist for Translucent Technologies, LLC; a company which is based in Memphis, Tennessee. [1]

Contents

In 1992 Verschuur became a resident of the City of Lakeland, which is located in Shelby County, Tennessee, northwest of Memphis. In 2001 Verschuur was elected, and served a four-year term as commissioner. In 2007 he was elected again and served for a total of 10 years. In Lakeland, Verschuur was also the President of the Garner Lake Association [ permanent dead link ]. Since 1986 he has been married to Dr. Joan Schmelz, a fellow scientist whose specialty is solar astronomy, specifically coronal loops. [2] Verschuur has one son who lives in England. [1]

During his years living beside the lake in Lakeland he made a fundamental discovery concerning the manner in which light interacts with a so-called Secchi Disk that is used to measure the transparency of lake and ocean waters. The disk had been invented in the mid-nineteenth century by a Jesuit priest (Angela Secchi) but no one before Verschuur had understand the optics underlying the measurement technique. [3]

Verschuur has taught at the University of Manchester, Rhodes University, the universities of Colorado and Maryland, UCLA, and the University of California, Berkeley, among others. [4] He has been an annual speaker at Mid-South Stargaze, "the annual amateur astronomers conference and star party held at Rainwater Observatory in French Camp, Mississippi." [5] In 1971 Verschuur was hired as the first Director of Fiske Planetarium for the University of Colorado at Boulder, [6] and in 1980 he worked with Dr. John C. Lilly. [4]

In his primary field of study Verschuur "pioneered the measurement of the interstellar magnetic field using the 21-cm Zeeman effect technique." [7] A thing which, according to Virginia Trimble, for the first time allowed astronomers to "measure magnetic strengths and their place-to-place variations with some confidence." [8]

Biography

Gerrit L. Verschuur was born in 1937 in Cape Town, South Africa, at the foot of Table Mountain. In 1936, his parents had emigrated from the Netherlands and settled in Cape Town. Two years after he was born—in 1939—his parents moved again, choosing a suburb of Cape Town named Lakeside. While he was living there, Verschuur attended Muizenberg Junior School. Then, when his parents moved to Port Elizabeth in 1950, he attended Grey Junior and subsequently Grey High School.[ citation needed ]

After graduation he began a six-year stint at Rhodes University in Grahamstown where he earned a BSc in 1957—Majors: Math, Physics, & Applied math; a BSc (Hons) of Physics in 1958; and a MSc degree of physics, in 1960.

In December 1960 he sailed for Southampton, England on Edinburgh Castle, a ship owned by the Union Castle Line. [9] It was one of the last passenger mail boats to ply the SA-England route, but was sold for scrap in 1967. [10]

Current research

Verschuur is at the center of a recent debate over the age of the universe. [11] [12] He claimed that images from the Wilkinson Microwave Anisotropy Probe are not pictures of the universe in its early form, but rather hydrogen gas clouds in our own galaxy. If he is shown to be correct, much work relating to the Big Bang theory would be undermined.

On December 10, 2007, his work with respect to COBE, WMAP, and HI, was published in The Astrophysical Journal. [13] However, Land and Slosar [14] claimed that the data did not support the correlation claimed by Verschuur. He subsequently published 4 more papers on the subject backing up his claims. [15] [16] [17] [18]

His current research is conducted in partnership with Joan Schmelz, his wife, and elaborates on the exciting discovery they made that the so-called high-velocity clouds are produced by supernova events that occurred relatively close to the Sun, of order hundreds of light years distant, several hundred thousand years ago. They solved the 60 year-old mystery concerning the distance to certain clouds when they found that neutron stars (left over after the explosion) exists in spectroscopic binary systems, the primary example having been discovered by researchers in Belgium led by Ana Escorza who used GAIA data to identify likely neutron star candidates. [19] [20] [21] [22] [23]

Selected publications

Books

Encyclopaedia articles

Related Research Articles

<span class="mw-page-title-main">Cosmic microwave background</span> Trace radiation from the early universe

The cosmic microwave background is microwave radiation that fills all space in the observable universe. It is sometimes called relic radiation. With a standard optical telescope, the background space between stars and galaxies is almost completely dark. However, a sufficiently sensitive radio telescope detects a faint background glow that is almost uniform and is not associated with any star, galaxy, or other object. This glow is strongest in the microwave region of the radio spectrum. The accidental discovery of the CMB in 1965 by American radio astronomers Arno Penzias and Robert Wilson was the culmination of work initiated in the 1940s.

<span class="mw-page-title-main">Galaxy formation and evolution</span>

The study of galaxy formation and evolution is concerned with the processes that formed a heterogeneous universe from a homogeneous beginning, the formation of the first galaxies, the way galaxies change over time, and the processes that have generated the variety of structures observed in nearby galaxies. Galaxy formation is hypothesized to occur from structure formation theories, as a result of tiny quantum fluctuations in the aftermath of the Big Bang. The simplest model in general agreement with observed phenomena is the Lambda-CDM model—that is, clustering and merging allows galaxies to accumulate mass, determining both their shape and structure. Hydrodynamics simulation, which simulates both baryons and dark matter, is widely used to study galaxy formation and evolution.

<span class="mw-page-title-main">Molecular cloud</span> Type of interstellar cloud

A molecular cloud, sometimes called a stellar nursery (if star formation is occurring within), is a type of interstellar cloud, the density and size of which permit absorption nebulae, the formation of molecules (most commonly molecular hydrogen, H2), and the formation of H II regions. This is in contrast to other areas of the interstellar medium that contain predominantly ionized gas.

<span class="mw-page-title-main">Interstellar medium</span> Matter and radiation in the space between the star systems in a galaxy

The interstellar medium (ISM) is the matter and radiation that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space. The energy that occupies the same volume, in the form of electromagnetic radiation, is the interstellar radiation field. Although the density of atoms in the ISM is usually far below that in the best laboratory vacuums, the mean free path between collisions is short compared to typical interstellar lengths, so on these scales the ISM behaves as a gas, responding to pressure forces, and not as a collection of non-interacting particles.

<span class="mw-page-title-main">Reionization</span> Process that caused matter to reionize early in the history of the Universe

In the fields of Big Bang theory and cosmology, reionization is the process that caused electrically neutral atoms in the universe to reionize after the lapse of the "dark ages".

<span class="mw-page-title-main">Rogue planet</span> Planets not gravitationally bound to a star

A rogue planet, also termed a free-floating planet (FFP) or an isolated planetary-mass object (iPMO), is an interstellar object of planetary mass which is not gravitationally bound to any star or brown dwarf.

<span class="mw-page-title-main">Hydrogen line</span> Spectral line of hydrogen state transition in UHF radio frequencies

The hydrogen line, 21 centimeter line, or H I line is a spectral line that is created by a change in the energy state of solitary, electrically neutral hydrogen atoms. It is produced by a spin-flip transition, which means the direction of the electron's spin is reversed relative to the spin of the proton. This is a quantum state change between the two hyperfine levels of the hydrogen 1 s ground state. The electromagnetic radiation producing this line has a frequency of 1420.405751768(2) MHz (1.42 GHz), which is equivalent to a wavelength of 21.106114054160(30) cm in a vacuum. According to the Planck–Einstein relation E = , the photon emitted by this transition has an energy of 5.8743261841116(81) μeV [9.411708152678(13)×10−25 J]. The constant of proportionality, h, is known as the Planck constant.

<span class="mw-page-title-main">Lambda-CDM model</span> Model of Big Bang cosmology

The Lambda-CDM, Lambda cold dark matter, or ΛCDM model is a mathematical model of the Big Bang theory with three major components:

  1. a cosmological constant, denoted by lambda (Λ), associated with dark energy
  2. the postulated cold dark matter, denoted by CDM
  3. ordinary matter
<span class="mw-page-title-main">NGC 5986</span> Globular cluster in the constellation Lupus

NGC 5986 is a globular cluster of stars in the southern constellation of Lupus, located at a distance of approximately 34 kilolight-years from the Sun. It was discovered by Scottish astronomer James Dunlop on May 10, 1826. John L. E. Dreyer described it as, "a remarkable object, a globular cluster, very bright, large, round, very gradually brighter middle, stars of 13th to 15th magnitude". Its prograde–retrograde orbit through the Milky Way galaxy is considered irregular and highly eccentric. It has a mean heliocentric radial velocity of +100 km/s. The galacto-centric distance is 17 kly (5.2 kpc), which puts it in the galaxy's inner halo.

<span class="mw-page-title-main">Stellar kinematics</span> Study of the movement of stars

In astronomy, stellar kinematics is the observational study or measurement of the kinematics or motions of stars through space.

<span class="mw-page-title-main">SIMP J013656.5+093347</span> Possible exoplanet in the constellation Pisces

SIMP J013656.5+093347 is a brown dwarf or planetary mass object at 19.9 light-years from Earth in the constellation Pisces. It belongs to the spectral class T2.5 and its position shifts due to its proper motion annually by about 1.24 arcsec in the right ascension.

<span class="mw-page-title-main">Hubble bubble (astronomy)</span> Variation in the Hubble constant

In astronomy, a Hubble bubble would be "a departure of the local value of the Hubble constant from its globally averaged value," or, more technically, "a local monopole in the peculiar velocity field, perhaps caused by a local void in the mass density."

<span class="mw-page-title-main">Serpens–Aquila Rift</span> Sky region containing dark interstellar clouds

The Serpens–Aquila Rift (also known as the Aquila Rift) is a region of the sky in the constellations Aquila, Serpens Cauda, and eastern Ophiuchus containing dark interstellar clouds. The region forms part of the Great Rift, the nearby dark cloud of cosmic dust that obscures the middle of the galactic plane of the Milky Way, looking inwards and towards its other radial sectors. The clouds that form this structure are called "molecular clouds", constituting a phase of the interstellar medium which is cold and dense enough for molecules to form, particularly molecular hydrogen (H2). These clouds are opaque to light in the optical part of the spectrum due to the presence of interstellar dust grains mixed with the gaseous component of the clouds. Therefore, the clouds in the Serpens-Aquila Rift block light from background stars in the disk of the Galaxy, forming the dark rift. The complex is located in a direction towards the inner Galaxy, where molecular clouds are common, so it is possible that not all components of the rift are at the same distance and physically associated with each other.

The Goldreich-Kylafis (GK) effect is a quantum mechanical effect with applications in Astrophysics. The theoretical background of the work was published by Peter Goldreich and his at the time postdoc Nick Kylafis in a series of two papers in The Astrophysical Journal.

<span class="mw-page-title-main">Cosmological lithium problem</span> Problem in astronomy

In astronomy, the lithium problem or lithium discrepancy refers to the discrepancy between the primordial abundance of lithium as inferred from observations of metal-poor halo stars in our galaxy and the amount that should theoretically exist due to Big Bang nucleosynthesis+WMAP cosmic baryon density predictions of the CMB. Namely, the most widely accepted models of the Big Bang suggest that three times as much primordial lithium, in particular lithium-7, should exist. This contrasts with the observed abundance of isotopes of hydrogen and helium that are consistent with predictions. The discrepancy is highlighted in a so-called "Schramm plot", named in honor of astrophysicist David Schramm, which depicts these primordial abundances as a function of cosmic baryon content from standard BBN predictions.

Misty C. Bentz is an American astrophysicist and Professor of Physics and Astronomy at Georgia State University. She is best known for her work on supermassive black hole mass measurements and black hole scaling relationships.

<span class="mw-page-title-main">HD 73882</span> Eclipsing binary system in constellation Vela

HD 73882 is a visual binary system with the components separated by 0.6″ and a combined spectral class of O8. One of stars is an eclipsing binary system. The period of variability is listed as both 2.9199 days and 20.6 days, possibly due to the secondary being a spectroscopic binary star.

<span class="mw-page-title-main">NGC 4325</span> Galaxy

NGC 4325 is an elliptical galaxy located about 330 million light-years away in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest on April 15, 1865, who described it as "vF, vS, iR, nf of 2". Despite being listed in the Virgo Cluster catalog as VCC 616, it is not a member of the Virgo Cluster but instead a background galaxy.

References

  1. 1 2 Uncommonly Lakeland Archived July 5, 2008, at the Wayback Machine
  2. Women in science – Earth and Space – Dr. Joan T. Schmelz Archived December 15, 2007, at the Wayback Machine
  3. Verschuur, Gerrit L. (1997). "Transparency Measurements in Garner Lake, Tennessee: The Relationship between Secchi Depth and Solar Altitude and a Suggestion for Normalization of Secchi Depth Data". Lake and Reservoir Management. 13 (2): 142–153. doi:10.1080/07438149709354305.
  4. 1 2 "Jepson School of Leadership Studies: Jepson Studies in Leadership". Archived from the original on December 2, 2007. Retrieved December 10, 2007. (See: Verschuur)
  5. Mid-South Star Gaze Archived October 9, 2007, at the Wayback Machine
  6. History // Fiske Planetarium Archived June 3, 2010, at the Wayback Machine
  7. "Our Place In Space: The Implications Of Impact Catastrophes On Human Thought And Behaviour". Archived from the original on August 6, 2007. Retrieved October 15, 2017.{{cite web}}: CS1 maint: bot: original URL status unknown (link)
  8. http://www.slac.stanford.edu/pubs/beamline/26/1/26-1-trimble.pdf (Beamline, Spring/Summer 1996, Vol. 26, No. 1, pages 40–41.)
  9. "Union-Castle Line". Maritime Matters. February 28, 2010. Retrieved June 27, 2012.
  10. "Union-Castle Line" . Retrieved June 27, 2012.
  11. "Analysis confronts model of universe's formation – physicsworld.com". Archived from the original on December 19, 2007. Retrieved December 10, 2007.
  12. Big Bang or Big Goof? Astronomer Verschuur Challenges 'Seeds' Proof
  13. "High Galactic Latitude Interstellar Neutral Hydrogen Structure and Associated (WMAP) High‐Frequency Continuum Emission"(Abstract)
  14. Correlation between galactic HI and the cosmic microwave background (Physical Review D, vol. 76, Issue 8, id. 087301)
  15. Verschuur, Gerrit L. (2010). "ON THE APPARENT ASSOCIATIONS BETWEEN INTERSTELLAR NEUTRAL HYDROGEN STRUCTURE AND ( WMAP ) HIGH-FREQUENCY CONTINUUM EMISSION". The Astrophysical Journal. 711 (2): 1208–1228. doi:10.1088/0004-637X/711/2/1208.
  16. Verschuur, Gerrit L. (2013). "Interacting Galactic Neutral Hydrogen Filaments and Associated High-Frequency Continuum Emission". The Astrophysical Journal. 768 (2): 181. doi:10.1088/0004-637X/768/2/181.
  17. Verschuur, Gerrit L. (2015). "ASSOCIATIONS BETWEEN SMALL-SCALE STRUCTURE IN LOCAL GALACTIC NEUTRAL HYDROGEN AND IN THE COSMIC MICROWAVE BACKGROUND OBSERVED BY PLANCK". The Astrophysical Journal. 813: 19. doi:10.1088/0004-637X/813/1/19.
  18. Verschuur, G. L.; Schmelz, J. T. (2016). "On the Nature of the Small-Scale Structure in the Cosmic Microwave Background Observed by Planck and Wmap". The Astrophysical Journal. 832 (2): 98. doi: 10.3847/0004-637X/832/2/98 .
  19. Schmelz, J. T.; Verschuur, G. L. (2022). "The Origin and Distance of the High-velocity Cloud MI". The Astrophysical Journal. 938: 68. doi: 10.3847/1538-4357/ac9412 .
  20. Escorza, A.; Karinkuzhi, D.; Jorissen, A.; Van Eck, S.; Schmelz, J. T.; Verschuur, G. L.; Boffin, H. M. J.; De Rosa, R. J.; Van Winckel, H. (2023). "A neutron star candidate in the long-period binary 56 UMa". Astronomy & Astrophysics. 670: L14. doi:10.1051/0004-6361/202245796.
  21. Verschuur, G. L.; Schmelz, J. T. (2023). "The Distance to High-velocity Cloud Complex M". The Astrophysical Journal. 943 (2): 161. doi: 10.3847/1538-4357/acac2a .
  22. Schmelz, J. T.; Verschuur, G. L. (2023). "Radio and γ-ray Evidence for the Supernova Origin of High-velocity Cloud Complex M". The Astrophysical Journal. 943: 44. doi: 10.3847/1538-4357/acae82 .
  23. Schmelz, J. T.; Verschuur, G. L.; Escorza, A.; Jorissen, A. (2023). "Supernovae Origin for the Low-latitude Intermediate-velocity Arch and the North Celestial Pole Loop". The Astrophysical Journal. 956: 2. doi: 10.3847/1538-4357/acf5e4 .
  24. http://www.reciprocalsystem.com/nfs/references.html Archived February 9, 2012, at the Wayback Machine (See: #65.)
  25. "Jepson School of Leadership Studies: Jepson Studies in Leadership". Archived from the original on December 2, 2007. Retrieved December 10, 2007. (See: Verschuur)
  26. Energy Citations Database (ECD) – - Document #4182195
  27. "Silo.lib.ia.us". Archived from the original on January 6, 2009. Retrieved March 4, 2022.
  28. http://www.reciprocalsystem.com/nfs/references.html Archived February 9, 2012, at the Wayback Machine (See: #74.)