Heliometer
Encyclopedia
Heliometer is an instrument originally designed for measuring the variation of the sun
's diameter at different season
s of the year, but applied now to the modern form of the instrument which is capable of much wider use.http://www.archive.org/stream/encyclopaediabrit13chisrich#page/224/mode/2up
The basic concept is to introduce a split element into a telescope's optical path so as to produce a double image. If one element is moved using a screw micrometer
, precise angle measurements can be made. The simplest arrangement is to split the object lens in half; with one half fixed and the other attached to the micrometer screw and slid along the cut diameter. To measure the diameter of the sun, for example, the micrometer is adjusted so that the two images of the solar disk just touch each other. Similarly, a precise measurement of the apparent separation between two nearby stars, A and B, is made by adjusting the double image so that A in one image touches B in the other.
The first application of the divided object-glass and the employment of double images in astronomical
measures is due to Servington Savary from Exeter in 1743. Pierre Bouguer
, in 1748, originated the true conception of measurement by double image without the auxiliary aid of a filar micrometer
, that is by changing the distance between two object-glasses of equal focus. John Dollond
, in 1754, combined Savary's idea of the divided object-glass with Bouguer's method of measurement, resulting in the construction of the first really practical heliometers. As far as we can ascertain, Joseph von Fraunhofer
, some time not long before 1820, constructed the first heliometer with an achromatic
divided object-glass, i.e. the first heliometer of the modern type.
The first successful measurements of stellar parallax
(to determine the distance to a star) were made by Friedrich Bessel
in 1838 for the star 61 Cygni
using a Fraunhofer heliometer. This was the 6.2" (157 mm) aperture Fraunhofer heliometer at Königsberg Observatory built by Joseph von Fraunhofer's firm, though he did not live to see it delivered to Bessel. Although the heliometer was difficult to use, it had certain advantages for Bessel including a wider field of view compared to other great refractors of the period, and overcame atmospheric turbulence
in measurements compared to a filar micrometer
.
Sun
The Sun is the star at the center of the Solar System. It is almost perfectly spherical and consists of hot plasma interwoven with magnetic fields...
's diameter at different season
Season
A season is a division of the year, marked by changes in weather, ecology, and hours of daylight.Seasons result from the yearly revolution of the Earth around the Sun and the tilt of the Earth's axis relative to the plane of revolution...
s of the year, but applied now to the modern form of the instrument which is capable of much wider use.http://www.archive.org/stream/encyclopaediabrit13chisrich#page/224/mode/2up
The basic concept is to introduce a split element into a telescope's optical path so as to produce a double image. If one element is moved using a screw micrometer
Micrometer
A micrometer , sometimes known as a micrometer screw gauge, is a device incorporating a calibrated screw used widely for precise measurement of small distances in mechanical engineering and machining as well as most mechanical trades, along with other metrological instruments such as dial, vernier,...
, precise angle measurements can be made. The simplest arrangement is to split the object lens in half; with one half fixed and the other attached to the micrometer screw and slid along the cut diameter. To measure the diameter of the sun, for example, the micrometer is adjusted so that the two images of the solar disk just touch each other. Similarly, a precise measurement of the apparent separation between two nearby stars, A and B, is made by adjusting the double image so that A in one image touches B in the other.
The first application of the divided object-glass and the employment of double images in astronomical
Astronomy
Astronomy is a natural science that deals with the study of celestial objects and phenomena that originate outside the atmosphere of Earth...
measures is due to Servington Savary from Exeter in 1743. Pierre Bouguer
Pierre Bouguer
Pierre Bouguer was a French mathematician, geophysicist, geodesist, and astronomer. He is also known as "the father of naval architecture"....
, in 1748, originated the true conception of measurement by double image without the auxiliary aid of a filar micrometer
Filar micrometer
A filar micrometer is a device used in astronomical telescopes for astrometry measurements. The word filar derives from Latin filum, a thread...
, that is by changing the distance between two object-glasses of equal focus. John Dollond
John Dollond
John Dollond was an English optician, known for his successful optics business and his patenting and commercialization of achromatic doublets.-Biography:...
, in 1754, combined Savary's idea of the divided object-glass with Bouguer's method of measurement, resulting in the construction of the first really practical heliometers. As far as we can ascertain, Joseph von Fraunhofer
Joseph von Fraunhofer
Joseph von Fraunhofer was a German optician. He is known for the discovery of the dark absorption lines known as Fraunhofer lines in the Sun's spectrum, and for making excellent optical glass and achromatic telescope objectives.-Biography:Fraunhofer was born in Straubing, Bavaria...
, some time not long before 1820, constructed the first heliometer with an achromatic
Achromatic lens
An achromatic lens or achromat is a lens that is designed to limit the effects of chromatic and spherical aberration. Achromatic lenses are corrected to bring two wavelengths into focus in the same plane....
divided object-glass, i.e. the first heliometer of the modern type.
The first successful measurements of stellar parallax
Stellar parallax
Stellar parallax is the effect of parallax on distant stars in astronomy. It is parallax on an interstellar scale, and it can be used to determine the distance of Earth to another star directly with accurate astrometry...
(to determine the distance to a star) were made by Friedrich Bessel
Friedrich Bessel
-References:* John Frederick William Herschel, A brief notice of the life, researches, and discoveries of Friedrich Wilhelm Bessel, London: Barclay, 1847 -External links:...
in 1838 for the star 61 Cygni
61 Cygni
61 Cygni,Not to be confused with 16 Cygni, a more distant system containing two G-type stars harboring the gas giant planet 16 Cygni Bb. sometimes called Bessel's Star or Piazzi's Flying Star, is a binary star system in the constellation Cygnus...
using a Fraunhofer heliometer. This was the 6.2" (157 mm) aperture Fraunhofer heliometer at Königsberg Observatory built by Joseph von Fraunhofer's firm, though he did not live to see it delivered to Bessel. Although the heliometer was difficult to use, it had certain advantages for Bessel including a wider field of view compared to other great refractors of the period, and overcame atmospheric turbulence
Astronomical seeing
Astronomical seeing refers to the blurring and twinkling of astronomical objects such as stars caused by turbulent mixing in the Earth's atmosphere varying the optical refractive index...
in measurements compared to a filar micrometer
Filar micrometer
A filar micrometer is a device used in astronomical telescopes for astrometry measurements. The word filar derives from Latin filum, a thread...
.