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Longer titles found: Angular diameter distance (view)

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alternate case: angular diameter

119 Tauri (1,353 words) [view diff] exact match in snippet view article find links to article

naked eye under good observing conditions. A semiregular variable, its angular diameter has been measured at about 10 mas. It is a similar star to Betelgeuse
Solar Saros 135 (302 words) [view diff] exact match in snippet view article find links to article
its angular diameter nearly as large as possible). This occurs around January 3. The Moon being nearly exactly at apogee (making its angular diameter as
NGC 3228 (340 words) [view diff] exact match in snippet view article find links to article
its center. Klarchenko et al. mention 53 possible members within the angular diameter of the cluster. The tidal radius of the cluster is 1.4 – 5.5 parsecs
IC 348 (416 words) [view diff] exact match in snippet view article find links to article
associated 2-million-year-old cluster of roughly 400 stars within an angular diameter of 20″. The most massive stars in the cluster are the binary star system
Messier 80 (674 words) [view diff] exact match in snippet view article find links to article
telescopes, appearing as a mottled ball of light. It has an apparent angular diameter of about 10 arcminutes. Since it is 32,600 light-years (10,000 pc)
Messier 38 (520 words) [view diff] exact match in snippet view article find links to article
effort to find a geometrical figure. At its distance of 1066 pc., its angular diameter of about 20 arc minutes corresponds to about 4.0 parsecs (13 light
Shapley 1 (236 words) [view diff] exact match in snippet view article find links to article
center of the nebula is a magnitude 14 white dwarf star. It has an angular diameter of 1.1 arc minutes, which makes it about one-third (.32) of a light
V602 Carinae (831 words) [view diff] exact match in snippet view article find links to article
distance, and a larger radius of 1,050±165 R☉ based on the measured angular diameter and luminosity. An effective temperature of 3,432±280 K was then calculated
Astronomy on Mars (3,565 words) [view diff] exact match in snippet view article find links to article
partial eclipses of the Sun by Phobos, since the angular diameter of Phobos is up to half the angular diameter of the Sun. However, in the case of Deimos the
V5668 Sagittarii (699 words) [view diff] exact match in snippet view article find links to article
and the mass of the entire shell to be 2.7 to 5.4 × 10−5 M☉ . The angular diameter of the dust shell was estimated to be 42 milliarcsec which, along with
Nebula (2,845 words) [view diff] exact match in snippet view article find links to article
Nebula, the brightest nebula in the sky and occupying an area twice the angular diameter of the full Moon, can be viewed with the naked eye but was missed by
3 Geminorum (758 words) [view diff] exact match in snippet view article find links to article
Observations of these occultations can give information about the angular diameter of a star, or about close companions. Occultations of 3 Geminorum have
Intensity interferometer (258 words) [view diff] exact match in snippet view article find links to article
of such an astronomical interferometer is to determine the apparent angular diameter of a radio source or star. If the distance to the object can then be
X Cancri (850 words) [view diff] exact match in snippet view article find links to article
These bands are thought to be very sensitive to temperature. The angular diameter of X Cancri has been measured using both lunar occultations and very
Mu Cephei (2,525 words) [view diff] exact match in snippet view article find links to article
based on its angular diameter and an assumed distance of 2,400 light years gives it a radius of 1,650 R☉, however the angular diameter used later turned
Francis G. Pease (250 words) [view diff] exact match in snippet view article find links to article
to the 100-inch (2,500 mm) telescope at Mt. Wilson to measure the angular diameter of the star Betelgeuse. Their estimate of 0.047" was very close to
Puppis A (298 words) [view diff] exact match in snippet view article find links to article
in diameter and roughly 6500–7000 light-years distant. Its apparent angular diameter is about 1 degree. The light of the supernova explosion reached Earth
Virbhadra–Ellis lens equation (168 words) [view diff] exact match in snippet view article find links to article
angle of light ( α ^ ) {\displaystyle ({\hat {\alpha }})} , and the angular diameter lens-source ( D d s ) {\displaystyle \left(D_{ds}\right)} and observer-source
TX Piscium (1,025 words) [view diff] exact match in snippet view article find links to article
semi-regular or irregular variable which usually pulsate in an overtone. The angular diameter has been measured at around 10 mas, although this varies depending
Gliese 667 (2,571 words) [view diff] exact match in snippet view article find links to article
along the middle of the habitable zone, Gliese 667 C would have an angular diameter of 1.24 degrees—2.3 times larger than the Sun appears from the surface
W Orionis (616 words) [view diff] exact match in snippet view article find links to article
A long secondary period of 2,450 days has also been reported. The angular diameter of W Orionis has been measured using interferometry and a value of
HD 32453 (687 words) [view diff] exact match in snippet view article find links to article
has expanded to 10 times the latter's girth (radius detected from an angular diameter of 0.748 mas). It radiates at 50 solar luminosities from its enlarged
ESO 383-76 (1,595 words) [view diff] exact match in snippet view article find links to article
photometric catalogue by Lauberts and Valentijn in 1989 that made the first angular diameter measurements of the galaxy. This includes the D25 and D25.5 B-band
Astronomical seeing (3,902 words) [view diff] exact match in snippet view article find links to article
overcome seeing. The strength of seeing is often characterized by the angular diameter of the long-exposure image of a star (seeing disk) or by the Fried
R Crucis (650 words) [view diff] case mismatch in snippet view article find links to article
Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076
Moons of Pluto (3,706 words) [view diff] exact match in snippet view article find links to article
passes in front of and blocks one of Pluto's satellites. Charon has an angular diameter of 4 degrees of arc as seen from the surface of Pluto; the Sun appears
IC 2395 (651 words) [view diff] exact match in snippet view article find links to article
same cluster is also supported by Clariá et al. who estimated its angular diameter at 19 arcminutes. IC 2395 is an open cluster of poor to moderate richness
S Orionis (550 words) [view diff] exact match in snippet view article find links to article
have been observed using VLTI and VLBA observations which measured an angular diameter varying between 7.9 and 9.7 mas. The mean period of variation has been
History of Mars observation (7,726 words) [view diff] exact match in snippet view article find links to article
geocentric model to explain the planet's motions. Measurements of Mars' angular diameter can be found in ancient Greek and Indian texts. In the 16th century
Canes II Group (136 words) [view diff] case mismatch in snippet view article find links to article
Name Equatorial Coordinates Declination Blue Magnitude Type Angular Diameter arc. Galaxy Diameter (Kly) Recessional Velocity Other Names NGC 4096 12 06
Soap Bubble Nebula (368 words) [view diff] exact match in snippet view article find links to article
imaged PN G75.5+1.7 on July 17, 2008. The nebula measures 260″ in angular diameter with a central star that has a J band magnitude of 19.45. Due to the
Winter solstice (3,175 words) [view diff] exact match in snippet view article find links to article
change in azimuth or elevation less than or equal to about 1/60 of the angular diameter of the Sun. Observing that it occurred within a two-day period is easier
Antares (5,517 words) [view diff] exact match in snippet view article find links to article
in 2010. The linear radius of the star can be calculated from its angular diameter and distance. However, the distance to Antares is not known with the
W Hydrae (447 words) [view diff] exact match in snippet view article find links to article
System). Radius calculated using a distance of 98+30 −18 parsecs and an angular diameter of 41.4 milliarcseconds (0.041 arcsec). 98 • 0.041 = diameter of 4
PKS 2131-021 (508 words) [view diff] exact match in snippet view article find links to article
comoving coordinate distance of PKS 2131−021 is 3.97 Gpc, with an angular diameter distance of 1.74 Gpc, and luminosity distance of 9.08 Gpc. Observations
T Ceti (641 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER". Monthly Notices of the Royal Astronomical
Spirit (rover) (5,063 words) [view diff] exact match in snippet view article
seeing Mercury's 6.1" angular diameter. They were able to observe transits of Deimos across the Sun, but at 2' angular diameter, Deimos is about 20 times
V636 Scorpii (485 words) [view diff] case mismatch in snippet view article find links to article
Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076
72 Tauri (678 words) [view diff] exact match in snippet view article find links to article
-C; Zhu, G. -L.; Fan, Q. -Y. (1987). "The measurements of stellar angular diameter by photoelectric observation of lunar occultation". Acta Astronomica
W Aquilae (986 words) [view diff] exact match in snippet view article find links to article
being accepted for peer-reviewed publication. Radius calculated with angular diameter and distance in Table 1 Vallenari, A.; et al. (Gaia collaboration)
Orders of magnitude (volume) (662 words) [view diff] exact match in snippet view article
core radius r = distance times sin(1⁄2 angular diameter) = 0.2 light year. Distance = 3.3 ± 0.9 kly; angular diameter = 20 arcseconds; expands 10 milliarcseconds
NGC 2244 (549 words) [view diff] exact match in snippet view article find links to article
astronomiques de Strasbourg. Retrieved 2007-04-20. distance × sin( angular diameter / 2 ) "The Rosette Nebula In Hubble Palette". Sky & Telescope. Retrieved
HR 7484 (600 words) [view diff] case mismatch in snippet view article find links to article
Based on Eclipsing Binary Stars: Toward Precision Better than 1% in Angular Diameter Predictions". The Astrophysical Journal. 837 (1): 19. arXiv:1611.09976
SU Persei (688 words) [view diff] exact match in snippet view article find links to article
Observations during 2015 and 2016 with CHARA show that the star has an angular diameter between 3.51 and 3.68 milliarcseconds. Considering its large distance
R Andromedae (1,126 words) [view diff] exact match in snippet view article find links to article
temperature and luminosity but is typically about 2,500 K and 6,300 L☉. The angular diameter of R Andromedae has been measured at 8.63±1.42 mas and 8.32±1.27 mas
BOOMERanG experiment (584 words) [view diff] exact match in snippet view article find links to article
and others, the BOOMERanG data from 1997 and 1998 determined the angular diameter distance to the surface of last scattering with high precision. When
UU Aurigae (1,019 words) [view diff] exact match in snippet view article find links to article
1971 to 1998, the periods are calculated as 439.4 and 233.1 days. The angular diameter of UU Aurigae has been measured at 12.07 ± 0.22 mas using very-long-baseline
Alpha Sagittarii (971 words) [view diff] exact match in snippet view article find links to article
inner solar system on a 250 year orbit. Radius retrieved multiplying angular diameter to distance; 107.5*0.00048 arcseconds*52.1 pc = 2.69 R☉. van Leeuwen
S Crucis (456 words) [view diff] case mismatch in snippet view article find links to article
Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076
Alphard (1,105 words) [view diff] exact match in snippet view article find links to article
with a spectral classification of K3 and luminosity class III. The angular diameter has been measured using interferometry, after correction for limb darkening
Lambda Gruis (435 words) [view diff] exact match in snippet view article find links to article
1134/S1063773712050015, S2CID 119257644. Cruzalèbes, P.; et al. (June 2010), "Angular diameter estimation of interferometric calibrators. Example of λ Gruis, calibrator
CHARA array (978 words) [view diff] exact match in snippet view article find links to article
measured directly, using CHARA. This was achieved by using the observed angular diameter of the star that the planet orbited, and the already known distance
Lambda Boötis (751 words) [view diff] case mismatch in snippet view article find links to article
1051/0004-6361:200810623, S2CID 14972955 Ciardi; et al. (2007), "The Angular Diameter of λ Boötis", The Astrophysical Journal, 659 (2): 1623–1628, arXiv:astro-ph/0612723
RW Cephei (3,415 words) [view diff] exact match in snippet view article find links to article
Images obtained using the SURFING algorithm result in a limb-darkened angular diameter of 2.45 mas, corresponding to a linear radius of 900–1,760 R☉ depending
Chi Cygni (3,728 words) [view diff] exact match in snippet view article find links to article
the angular diameter of the star. The statistical margin of error is about 20%. The distance can also be derived by comparing changes in the angular diameter
Upsilon Capricorni (532 words) [view diff] exact match in snippet view article find links to article
; Evans, D. S.; Silverberg, E. C.; Wiant, J. R. (March 1973), "The angular diameter of Upsilon Capricorni and an occultation of SAO 118655.", Astronomical
AZ Cygni (2,072 words) [view diff] exact match in snippet view article find links to article
unreliable due to a high amount of astrometric noise. By using the angular diameter and Gaia parallax-derived distance in the 2019 Mid-infrared stellar
Eridanus Cluster (282 words) [view diff] exact match in snippet view article find links to article
barred and unbarred); Sm, SBm, Irr=Irregular; (r),(rs)=Ring Structure Angular diameter of the galaxy (arcminutes) Diameter of the galaxy (thousands of light
Heliometer (660 words) [view diff] no match in snippet view article find links to article
The difference in the two micrometer readings so obtained is the (angular) diameter of the Sun. Similarly, a precise measurement of the apparent separation
KW Sagittarii (1,040 words) [view diff] exact match in snippet view article find links to article
000 L☉ and a radius around 1,009 ± 142 R☉ was based on the measured angular diameter and luminosity. VX Sagittarii — another red supergiant (RSG) in the
Sparrow's resolution limit (418 words) [view diff] exact match in snippet view article find links to article
stars that can still be perceived as separate by an observer. The angular diameter of the Airy disk is determined by the aperture of the instrument. Rayleigh's
Fine guidance sensor (715 words) [view diff] exact match in snippet view article find links to article
companion, determine if certain stars really are double stars, measure the angular diameter of stars, galaxies, etc. Due to the sensitivity of the FGS they can
87 Leonis (451 words) [view diff] exact match in snippet view article find links to article
S2CID 14878976. Dunham, D. W.; Evans, D. S.; et al. (April 1974), "The angular diameter of 87 Leonis.", Astronomical Journal, 79: 483–484, Bibcode:1974AJ.
Kappa Pavonis (972 words) [view diff] exact match in snippet view article find links to article
radius to change by about 3 R☉ above and below the mean size. The angular diameter of the disc has been directly observed to change during the pulsations
S Normae (612 words) [view diff] case mismatch in snippet view article find links to article
Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076
Lacaille 9352 (1,062 words) [view diff] exact match in snippet view article find links to article
known as a red dwarf. This was the first red dwarf star to have its angular diameter measured, with the physical diameter being about 47% of the Sun's radius
Maia (star) (1,699 words) [view diff] exact match in snippet view article
and a mass of 3.8 solar masses. Interferometric measurements give an angular diameter of 0.451±0.006 mas, suggesting a radius of 6.61 R☉ assuming a distance
Scientific information from the Mars Exploration Rover mission (4,464 words) [view diff] exact match in snippet view article find links to article
permit seeing Mercury's 6.1" angular diameter. Transits of Deimos across the Sun were seen, but at 2' angular diameter, Deimos is about 20 times larger
Omicron1 Orionis (727 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER", Monthly Notices of the Royal Astronomical
S Persei (1,627 words) [view diff] exact match in snippet view article find links to article
hypergiant and has a radius over 700 times the sun's radius (R☉). Its angular diameter has been measured directly and found to be somewhat elliptical. Modelled
R Aquilae (739 words) [view diff] exact match in snippet view article find links to article
35) × 10−7 M☉ yr−1, forming a dusty silicate shell. Calculated using angular diameter and distance in Table 1 Brown, A. G. A.; et al. (Gaia collaboration)
Richard Towneley (2,901 words) [view diff] exact match in snippet view article find links to article
observations of the comet of 1664, he devised his own method of computing the angular diameter of the nucleus by comparing it with the apparent diameter of a weather
S Muscae (665 words) [view diff] case mismatch in snippet view article find links to article
Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076
Lambda Aquarii (1,162 words) [view diff] case mismatch in snippet view article find links to article
S2CID 120313180. 10. Nather, R. Edward; et al. (June 1970). "The Angular Diameter of Lambda Aquarii". Astrophysical Journal. 160: L181. Bibcode:1970ApJ
Beta Tauri (1,516 words) [view diff] exact match in snippet view article find links to article
including as a "SrCrEu star" or even an Ap star. Its limb-darkened angular diameter has been measured at 1.090±0.076 mas. At a distance of 41.1 pc, this
HR Carinae (1,509 words) [view diff] exact match in snippet view article find links to article
but much less bright. It is most likely a red supergiant with an angular diameter of 0.85±0.20 mas, translating to a radius about 500±150 R☉, and also
Epsilon Trianguli Australis (448 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER", Monthly Notices of the Royal Astronomical
Gamma Hydri (535 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER", Monthly Notices of the Royal Astronomical
Merak (star) (1,361 words) [view diff] case mismatch in snippet view article
Hanlon, W.; Hinrichs, C. E.; Holder, J.; Jin, W. (2024-04-26). "An Angular Diameter Measurement of β UMa via Stellar Intensity Interferometry with the
List of largest galaxies (661 words) [view diff] exact match in snippet view article find links to article
provided scale "Virgo + GA + Shapley" multiplied with the values for the angular diameter of the cited estimation method. Morphology unlisted; images show an
R Sculptoris (896 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER". Monthly Notices of the Royal Astronomical
James Bradley (1,651 words) [view diff] exact match in snippet view article find links to article
1757. He was survived by one daughter. In 1722, Bradley measured the angular diameter of Venus with a large aerial telescope with an objective focal length
Dirk Reuyl (540 words) [view diff] exact match in snippet view article find links to article
with fellow staff member Alexander N. Vyssotsky. In 1941 he measured angular diameter of Mars using photographic plates. In 1943 he claimed to have discovered
Cosmic distance ladder (8,113 words) [view diff] exact match in snippet view article find links to article
relation (or Σ-D relation), used in elliptical galaxies, relates the angular diameter (D) of the galaxy to its velocity dispersion. It is important to describe
Transit of Phobos from Mars (1,945 words) [view diff] exact match in snippet view article find links to article
high latitudes (but less than 70.4°) will see a noticeably smaller angular diameter for Phobos because they are considerably farther away from it than
Gamma Reticuli (545 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER", Monthly Notices of the Royal Astronomical
R Trianguli Australis (529 words) [view diff] case mismatch in snippet view article find links to article
Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076
The Sand Reckoner (1,903 words) [view diff] exact match in snippet view article find links to article
the Sun was no more than thirty times larger than the Moon. that the angular diameter of the Sun, as seen from the Earth, was greater than 1/200 of a right
Zeta Arae (908 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER", Monthly Notices of the Royal Astronomical
Mu Geminorum (1,486 words) [view diff] case mismatch in snippet view article find links to article
16 December 2017. Mondal, Soumen; Chandrasekhar, T. (August 2005), "Angular Diameter Measurements of Evolved Variables by Lunar Occultations at 2.2 and
Spica (2,475 words) [view diff] exact match in snippet view article find links to article
the pair and to directly measure the orbital characteristics and the angular diameter of the primary, which was found to be (0.90 ± 0.04) × 10−3 arcseconds
Virgo Cluster (2,060 words) [view diff] exact match in snippet view article find links to article
SBa,SBb,SBc,SBd=Barred spiral, Sm,SBm,Irr=Irregular. Column 6: The angular diameter of the galaxy (arcminutes). Column 7: The diameter of the galaxy (thousands
Age of the universe (3,880 words) [view diff] exact match in snippet view article find links to article
on 23 February 2008. Retrieved 23 February 2008. Hu, W. "Animation: Angular diameter distance scaling with curvature and lambda". University of Chicago
IC 443 (1,330 words) [view diff] exact match in snippet view article find links to article
surrounding molecular clouds. IC 443 is an extended source, having an angular diameter of 50 arcmin (by comparison, the full moon is 30 arcmin across). At
Sigma Librae (1,313 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER". Monthly Notices of the Royal Astronomical
SN 1572 (2,233 words) [view diff] exact match in snippet view article find links to article
Tycho's SNR has a roughly spherical morphology and spreads over an angular diameter of about 8 arcminutes. Its physical size corresponds to radius of the
S Sagittae (837 words) [view diff] case mismatch in snippet view article find links to article
Moskalik, P.; Gorynya, N. A. (2005). "Mean Angular Diameters and Angular Diameter Amplitudes of Bright Cepheids". Acta Astronomica. 55: 247. arXiv:astro-ph/0507076
TRAPPIST-1e (2,719 words) [view diff] exact match in snippet view article find links to article
Sun due to the low luminosity of its star. The star would cover an angular diameter of about 2.17 degrees from the surface of the planet, and so would
R Leporis (870 words) [view diff] exact match in snippet view article find links to article
1075 • 𝜃 • d, where R is the radius (in solar radii/R☉), 𝜃 is the angular diameter in arcseconds and d is the distance in parsecs. Angular diameters of
Gliese 667 Cc (1,695 words) [view diff] exact match in snippet view article find links to article
edge of the habitable zone. From its surface, the star would have an angular diameter of 1.24 degrees and would appear to be 2.3 times the visual diameter
R Hydrae (1,101 words) [view diff] exact match in snippet view article find links to article
feature is consistent with the star's proper motion. Calculated with angular diameter and distance in Table 1 VERA Collaboration; Hirota, Tomoya; Nagayama
R Hydrae (1,101 words) [view diff] exact match in snippet view article find links to article
feature is consistent with the star's proper motion. Calculated with angular diameter and distance in Table 1 VERA Collaboration; Hirota, Tomoya; Nagayama
Sirius (10,259 words) [view diff] exact match in snippet view article find links to article
been measured by an astronomical interferometer, giving an estimated angular diameter of 5.936±0.016 mas. The projected rotational velocity is a relatively
Sakurai's Object (2,377 words) [view diff] exact match in snippet view article find links to article
had increased to around 11–15. By investigating the measured fluxes, angular diameter, and mass of the nebula, a distance of 5.5 kpc and luminosity of 38 L☉
Sunyaev–Zeldovich effect (2,203 words) [view diff] exact match in snippet view article find links to article
X-ray data can also be used to determine the Hubble constant using the angular diameter distance of the cluster. These thermal distortions can also be measured
On Sizes and Distances (Hipparchus) (3,021 words) [view diff] exact match in snippet view article
the Moon measured its own circle close to 650 times, and that the angular diameter of Earth's shadow is 2.5 times that of the Moon. Pappus tells us that
Ara (constellation) (3,229 words) [view diff] exact match in snippet view article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER". Monthly Notices of the Royal Astronomical
Eta Telescopii (1,512 words) [view diff] exact match in snippet view article find links to article
Jupiter, while its radius is 2.3 times the radius of Jupiter. From angular diameter and distance Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia
Alpha Reticuli (967 words) [view diff] exact match in snippet view article find links to article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER". Monthly Notices of the Royal Astronomical
Mensa (constellation) (4,071 words) [view diff] case mismatch in snippet view article
Based on Eclipsing Binary Stars: Toward Precision Better than 1% in Angular Diameter Predictions". The Astrophysical Journal. 837 (1): 19. arXiv:1611.09976
Zeta Geminorum (2,222 words) [view diff] exact match in snippet view article find links to article
1051/0004-6361/200811464, S2CID 18283579 Kervella, P.; et al. (March 2001), "The angular diameter and distance of the Cepheid ? Geminorum", Astronomy and Astrophysics
Eta Corvi (1,909 words) [view diff] exact match in snippet view article find links to article
already designated for β Corvi (Kraz) by R.H. Allen. Calculated using angular diameter and distance. van Leeuwen, F. (2007). "Validation of the new Hipparcos
Conjunction (astronomy) (3,701 words) [view diff] exact match in snippet view article
1953, BC, Mercury, Venus, Mars and Saturn formed a group with an angular diameter of 26.45 arc minutes. Jupiter was on the same day only a few degrees
(31345) 1998 PG (1,004 words) [view diff] exact match in snippet view article
4 kilometers. From the surface of 1998 PG, the moon would have an angular diameter of about 16.3°. For comparison, the Sun appears to be 0.5° from Earth
HR 5171 (3,397 words) [view diff] exact match in snippet view article find links to article
possible S Doradus variable, as well as an eclipsing variable. The angular diameter of HR 5171A has been published three times using measurements from
Transit of Mercury (3,512 words) [view diff] exact match in snippet view article find links to article
May 8 (descending node) and November 10 (ascending node), with the angular diameter of Mercury being about 12″ for May transits, and 10″ for November transits
Orbit of the Moon (4,678 words) [view diff] exact match in snippet view article find links to article
Minimum, mean and maximum distances of the Moon from Earth with its angular diameter as seen from Earth's surface, to scale. Scroll to right to see the
Eclipse cycle (10,447 words) [view diff] exact match in snippet view article find links to article
misses Earth's shadow. Also, at most solar eclipses, the apparent angular diameter of the Moon is insufficient to fully occlude the solar disc, unless
Acrux (2,331 words) [view diff] exact match in snippet view article find links to article
{\text{AU}}/R_{\bigodot }}}\\&11.073\cdot R_{\bigodot }\end{aligned}}} The angular diameter used (0.52 milliarcseconds) is from CADARS. Distance (99 parsecs) is
Altair (2,781 words) [view diff] exact match in snippet view article find links to article
may be due to convection cells forming at the cooler equator. The angular diameter of Altair was measured interferometrically by R. Hanbury Brown and
Orders of magnitude (length) (17,804 words) [view diff] exact match in snippet view article
217P. radius = distance times sin(angular diameter/2) = 0.2 light-year. Distance = 3.3 ± 0.9 kly; angular diameter = 20 arcseconds (Reed et al. 1999)
Arcturus (5,405 words) [view diff] exact match in snippet view article find links to article
Bibcode:1998Obs...118..299G. Quirrenbach, A.; et al. (August 1996), "Angular diameter and limb darkening of Arcturus.", Astronomy and Astrophysics, 312:
Length contraction (5,075 words) [view diff] exact match in snippet view article find links to article
Victor Weisskopf in a Physics Today article. For instance, for a small angular diameter, a moving sphere remains circular and is rotated. This kind of visual
Hollow Moon (3,085 words) [view diff] exact match in snippet view article find links to article
with such a satellite: Saturn's moon Prometheus has roughly the same angular diameter as the Sun when viewed from Saturn. Some scholars have claimed that
List of nearest giant stars (4,068 words) [view diff] exact match in snippet view article find links to article
Calculated using an angular diameter of 5.99 mas. Calculated using an angular diameter of 5.25 mas. Calculated using an angular diameter of 3.99 mas.
Barnard's Star (5,351 words) [view diff] exact match in snippet view article find links to article
amount to a quarter of a degree in a human lifetime, roughly half the angular diameter of the full Moon. The radial velocity of Barnard's Star is −110 km/s
Albireo (3,008 words) [view diff] exact match in snippet view article find links to article
interferometry from the Navy Precision Optical Interferometer. A limb-darkened angular diameter of 4.904 mas was measured. At the parallax-derived distance of 111
Dark Energy Survey (5,466 words) [view diff] exact match in snippet view article find links to article
correlations and spherical harmonics to constrain the ratio of comoving angular diameter distance D m ( Z e f f = 0.835 ) / r d = 18.92 ± 0.51 {\displaystyle
HR 8799 (4,455 words) [view diff] case mismatch in snippet view article find links to article
Ireland, Michael; von Braun, Kaspar (21 November 2012). "The CHARA Array Angular Diameter of HR 8799 Favors Planetary Masses for Its Imaged Companions". The
Orders of magnitude (power) (2,726 words) [view diff] exact match in snippet view article
"Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER". Monthly Notices of the Royal Astronomical
Lunar theory (6,854 words) [view diff] exact match in snippet view article find links to article
factor of about 2, which is clearly not seen in reality. (The apparent angular diameter of the Moon does vary monthly, but only over a much narrower range
Atmosphere of Uranus (6,387 words) [view diff] exact match in snippet view article find links to article
frustration. Uranus is a relatively faint object, and its visible angular diameter is smaller than 5″. The first spectra of Uranus were observed through
BM Scorpii (819 words) [view diff] exact match in snippet view article find links to article
of 129 R☉, BM Scorpii has a bolometric luminosity of 3,388 L☉. Its angular diameter has been measured at 2.5 mas. In 1920 Annie Cannon discovered that
Total internal reflection (13,479 words) [view diff] exact match in snippet view article find links to article
is compressed into a conical field known as Snell's window, whose angular diameter is twice the critical angle (cf. Fig. 6).  The field of view above
PKS 1741-03 (962 words) [view diff] exact match in snippet view article find links to article
weeks to months. During its ESE period, there was an increase in its angular diameter by 0.7 milliarcsecond. When observed on timescales of few months, PKS
Solar eclipse of July 16, 2186 (1,585 words) [view diff] exact match in snippet view article find links to article
its angular diameter nearly as small as possible). This occurs around July 6th. The Moon being almost exactly at perigee (making its angular diameter as
WASP-178b (1,491 words) [view diff] case mismatch in snippet view article find links to article
1086/319000. S2CID 122558713. Davis, J.; et al. (October 2010). "The Angular Diameter and Fundamental Parameters of Sirius A". Publications of the Astronomical
List of instrument-resolved minor planets (2,527 words) [view diff] exact match in snippet view article find links to article
2012-02-25, retrieved 2011-07-29 Worden, S. P.; et al. (January 1979), "Angular diameter of the asteroids Vesta and Pallas determined from speckle observations"
List of nearest supergiants (4,976 words) [view diff] exact match in snippet view article find links to article
{(5772/4,150)^{4}*5,500}}=143.46\ R\odot } Using Alpha Aquarii's measured angular diameter at 3.066±0.036 milliarcseconds (mas), together with its distance to
List of nearest stars by spectral type (15,778 words) [view diff] exact match in snippet view article find links to article
retrieved multiplying angular diameter to distance; 107.5*0.00048 arcseconds*52.1 pc = 2.69 R☉. Calculated using an angular diameter of 0.801 Milliarcseconds