An Etymological Dictionary of Astronomy and Astrophysics
English-French-Persian

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 204
verifiability principle
  پروز ِ راست-جُست-پذیری   
parvaz-e râst-jost-paziri

Fr.: principe de vérifiabilité   

In logical positivism philosophy, the claim that a statement is literally meaningful (it expresses a proposition) if and only if it either actually has been verified or could at least in principle be verified.

Quality noun from → verifiable; → principle.

verifiable
  راست-جُست-پذیر   
râst-jost-pazir

Fr.: vérifiable   

That can be verified. → verify; → verification; → verifiability principle.

verify; → -able.

verification
  راست-جُست   
râst-jost

Fr.: vérification   

The act of verifying. The state of being verified.
The process of research and examination required to establish correctness, authenticity, or validity.

Verbal noun of → verify.

verify
  راست-جُستن، راست-جست کردن   
râst-jostan, râst-jost kardan

Fr.: vérifier   

To ascertain the truth or correctness of, as by examination, research, or comparison.

M.E. verifien, from M.Fr. verifier, from M.L. verificare "to make true," from L. verus "true;" → -fy.

Râst-jostan, literally "to seek the truth, to seek the right," from râst "right, true; just, upright, straight" (Mid.Pers. râst "true, straight, direct;" Soghdian rəšt "right;" O.Pers. rāsta- "straight, true," rās- "to be right, straight, true;" Av. rāz- "to direct, put in line, set," razan- "order;" cf. Skt. raj- "to direct, stretch," rjuyant- "walking straight;" Gk. orektos "stretched out;" L. regere "to lead straight, guide, rule," p.p. rectus "right, straight;" PIE base *reg- "move in a straight line," hence, "to direct, rule") + jostan/juyidan "to seek, strive for" (Proto-Iranian *iud- "to struggle for something, to fight;" Av. yūδ- "to fight, struggle;" Mod.Pers. justan, juy- "to search, seek, ask for;" cf. Mid.Pers. vijuyihitan "to search, seek").

vernal
  بهاری   
bahâri (#)

Fr.: vernal   

Of or pertaining to spring. → vernal equinox.

From L. vernalis "of the spring," from vernus "of spring," from uēr "spring," cognate with Pers. bahâr, as below.

Bahâri of or pertaining to bahâr "spring;" Mid.Pers. wahâr "spring;" O.Pers. vāhara- "spring time," θūra-vāhara- "name of a spring month;" Av. vaηhar "spring;" cf. Skt. vasara- "relating or appearing in the morning;" Gk. ear "spring;" L. uēr "spring," vernus "of spring;" O.N. vār "spring;" Lith. vasara "summer;" O.C.S. vesna "spring."

vernal equinox
  هموگان ِ بهاری   
hamugân-e bahâri

Fr.: équinoxe vernal   

The point of intersection between the ecliptic and the celestial equator at which the Sun passes from south to north of the celestial equator during its apparent annual motion. The instant of this event. It occurs on March 20, 21 or rarely 19. At the vernal equinox, as with the → autumnal equinox, night and day are equal in length world over. Several thousands years ago the vernal equinox was in Aries, but because of precession it has now slid west into Pisces. Right ascension and celestial longitude are measured from the vernal equinox. Also known as spring equinox. → First Point of Aries.

vernal; → equinox.

vernal-equinox year
  سال ِ هموگان ِ بهاری   
sâl-e hamugân-e bahâri

Fr.: année d'équinoxe vernal, année vernale   

The time interval between two successive passages of the Sun, when the true longitude of the Sun is considered. In other words, the interval during which the Sun's true longitude increases by 360 degrees. Its mean length for the epoch J2000.0 is 365.24236460 real solar days (approximately 365.2424 days). The vernal-equinox year, on which the Iranian calender is based, should not be confused with → tropical year. See also: A concise review of the Iranian calendar. → Iranian calendar

vernal; → equinox; → year.

vernier
  ورنیه   
vernier (#)

Fr.: vernier   

A small movable scale running parallel to the main graduated scale in certain measuring instruments, such as the → sextant, used to obtain a fractional reading of one of the divisions on the main scale. Also known as Vernier scale.

After the French mathematician Pierre Vernier (1580-1637), who invented the scale in 1631.

version
  گرداک   
gardâk

Fr.: version   

A particular form or variant of something.
An account of something, given from a specific point of view.

M.E., from M.Fr. version, from M.L. versionem (nominative versio) "a turning," from p.p. stem of L. vertere "to turn;" cognate with Pers. gardidan "to change," as below.

Gardâk, present stem of gardidan "to change, to turn" (Mid.Pers. vartitan "to change, to turn;" Av. varət- "to turn, revolve;" cf. Skt. vrt- "to turn, roll," vartate "it turns round, rolls;" L. vertere "to turn;" O.H.G. werden "to become;" PIE base *wer- "to turn, bend") + -âk noun suffix.

vertex
  تارک   
târak

Fr.: vertex, sommet   

Plural form: vertices.
1) Astro.: A point in the → celestial sphere toward which or from which the common motion of a group of stars is directed.
2) Math.: The → point where two → sides of a → plane figure or an → angle  → intersect.
3) In → graph theory, any of the points of which graphs are formed. Same as → node.

From L. vertex "highest point," literally "the turning point," originally "whirlpool," from vertere "to turn," cognate with Pers. vartidan, gardidan, → version.

Târak, variant târ "top, vertex, head, the middle of the head;" cf. Sogd. târ "summit, forehead;" Yaghnobi tôr(k) "the back of the head;" Yazghulami tur "summit, head;" Proto-Ir. *starH- "to spread," → expand; PIE *ster- "spread, extend."

vertical
  هجین   
hajin (#)

Fr.: vertical   

1) The apparent → direction of → gravity at the point of observation.
2) Being in a position or direction → perpendicular to the → plane of the → horizon. See also → normal.

Vertical, literally "of or at the vertex, directly overhead," from M.Fr. vertical, from L.L. verticalis "overhead," from L. vertex (genitive verticis) "highest point"

Hajin, from haj, variant hac "anything held vertical, erected in the manner of a spear" (Dehxodâ), may be from Proto-Ir. *hac- "to follow;" cf. Av. (+ *ā-) hac- "to stick to;" Mid.Pers. hâz- "to lead, guide;" → associate.

vertical circle
  پرهون ِ هجین، دایره‌ی ِ ~   
parhun-e hajin, dâyere-ye ~

Fr.: cercle vertical   

The greater circle on the celestial sphere which passes through → zenith, → nadir, and the star and whose plane is perpendicular to the plane of horizon. Same as → azimuth circle.

vertical; → circle.

vertical scaling
  مرپلش ِ هجین   
marpeleš-e hajin

Fr.:   

In computer science, a scaling in which the processing power of the same node/system is increased by increasing/decreasing its resources (CPU, memory, etc.). See also → horizontal scaling.

vertical; → scaling.

vertices
  تارکها   
târakhâ

Fr.: sommets, vertex   

Plural of → vertex.

vertex.

very
  بسیار   
besyâr (#)

Fr.: très   

In a high degree. → Very Large Telescope (VLT); → very massive star; → very high frequencies (VHF).

M.E.; O.Fr verai "true;" L. verax (genitive veracis) "truthful," from verus "true."

Besyâr, from bas "many, much" (Mid.Pers. vas "many, much;" O.Pers. vasiy "at will, greatly, utterly;" Av. varəmi "I wish," vasô, vasə "at one's pleasure or will," from vas- "to will, desire, wish").

very high frequencies (VHF)
  بسامدهای ِ بسیار بالا   
basâmadhâ-ye besyâr bâlâ

Fr.: très hautes fréquences   

Radio frequencies in the range 30 to 300 mega Hz.

very; → high; → frequency.

Very Large Array (VLA)
  آرست ِ بسیار بزرگ   
ârast-e besyâr bozorg

Fr.: Very Large Array (VLA)   

A radio interferometer consisting of 27 antennas, each 25 m in diameter, in a Y-shaped configuration. It is located about 100 km west of Socorro, New Mexico, and is operated by the United States National Radio Astronomy Observatory. The VLA has the resolution of a single antenna 36 km wide and the sensitivity of a dish 130 m across.

very; → large; → array.

Very Large Baseline Array (VLBA)
  آرست با پایه-خط ِ بسیار بزرگ   
ârast bâ pâye-xatt-e besyâr bozorg

Fr.: Very Large Baseline Array (VLBA)   

A network of ten 25-m radio telescopes for → very-long-baseline interferometry (VLBI), operated by the U.S. National Radio Astronomy Observatory. Eight of the VLBA telescopes are distributed across the continental United States, while the other two are in Hawaii and the Virgin Islands, giving a maximum baseline of about 8,000 km and a resolution better than a milliarcsecond at its shortest wavelength.

very; → large; → baseline; → array.

Very Large Telescope (VLT)
  تلسکوپ ِ بسیار بزرگ   
tleskop-e besyâr bozorg

Fr.: Très Grand Télescope, VLT   

An observing facility consisting of four 8.2 m telescopes, with the combined collecting area of a 16 m mirror, owned and operated by the European Southern Observatory at an altitude of 2635 m at the Paranal Observatory in Chile. The four reflecting unit telescopes are called Antu "Sun" in the language of Chile's indigenous Mapuche people, Kueyen "Moon," Melipal "Southern Cross," and Yepun "Venus." Each unit is equipped with several sophisticated instruments. The light of the individual telescopes can be combined using interferometric techniques to achieve superior resolution. → VLT Interferometer (VLTI). The wavelength range covered by the VLT is extremely wide, ranging from deep ultraviolet to mid-infrared.

very; → large; → telescope.

very late thermal pulse (VLTP)
  تپه‌ی ِ گرمای ِ بسیار دیر   
tape-ye garmâyi-ye besyâr dir

Fr.: flash de l'hélium très tardif   

In evolutionary models of → post-asymptotic giant branch stars, the occurrence of the helium shell burning when the star has reached the → white dwarf cooling track. This leads to the possibility of a violent → helium shell flash and expansion on a time-scale of ≤ 10 years. The rapid expansion and prompt change in surface composition observed in → Sakurai's Object are thought to be due to such a very late thermal pulse.

very; → late; → thermal; → pulse.

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