「Hubble」の共起表現一覧(1語右で並び替え)
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| It was named for the astronomer Edwin | Hubble, a Wheaton native and graduate of Wheaton Cent |
| ven lower value, around 50, corresponding to a | Hubble age of around 20 billion years. |
| of the redshifts associated with the galaxies, | Hubble and Milton Humason discovered a rough proporti |
| you aren't aware already, the Google doodle is | Hubble, and clicking it leads to search results where |
| redshift-distance correlation, nowadays termed | Hubble's law, was formulated by Hubble and Humason in |
| It was discovered in 1949 by Edwin | Hubble and again in 1955 by A. G. Wilson. |
| ngine once used by the famous astronomer Edwin | Hubble at the Mt. |
| The head teacher is Mr. A. E. | Hubble, B.Ed., NPQH. |
| ging to John Buttles and her husband's brother | Hubble Blinn, including a bag of gold coins and a bun |
| ehavi et al. reported evidence in support of a | Hubble bubble. |
| " was later covered by Nick Lowe (Bowi EP) and | Hubble Bubble. |
| named one of the top ten photographs from the | Hubble by Space.com. |
| Land based telescopes and | Hubble capture the first images of exoplanets in the |
| would be to only consider the scale factor and | Hubble constant for a Friedman-Robertson-Walker model |
| matters have resulted in cited values for the | Hubble Constant ranging between 60 km/s/Mpc and 80 km |
| igh estimate was due to an mis-estimate of the | Hubble constant by Alfred Behr, which could not be re |
| Based on the published red shift, ( | Hubble Constant of 62 km/s per Mpc) a rough distance |
| lusters they choose to include or not, on what | Hubble constant they use, etc. 70.51.11.219 (talk) 12 |
| ated on three fields: the determination of the | Hubble constant (H0) using the Tully-Fisher relation, |
| is work led to the precise measurements of the | Hubble Constant H0 and the deceleration parameter q0, |
| The | Hubble Constant measures the current state of expansi |
| es, leading to the precise measurements of the | Hubble constant H0 and the deceleration parameter q0, |
| with the thesis titled "The Anisotropy of the | Hubble Constant". |
| y estimate the expansion rate of the Universe ( | Hubble constant) using the measured time-delay and le |
| The | Hubble Constant, named for astronomer Edwin Hubble, w |
| ere, the coefficient H in the exponential, the | Hubble constant, is |
| 8 he published the first good estimate for the | Hubble constant, revising Hubble's value of 250 down |
| onstrained by supplying a precise value of the | Hubble constant. |
| ly they cannot be used to define points on the | Hubble curve, because of circular reasoning. |
| al models he developed to visible and infrared | Hubble data collected by then Harvard graduate studen |
| In the years since the original | Hubble Deep Field, the Hubble Deep Field South and th |
| en in the image here - in the same vein as the | Hubble Deep Field. |
| The | Hubble Deep Field |
| two fields of 10' by 16'; one centered on the | Hubble Deep Field North (12h 36m 55s, +62° 14m 15s) a |
| WFPC2 was used to image the | Hubble Deep Field in 1995, the Hourglass Nebula and E |
| Hubble docked in the cargo bay of Atlantis. | |
| COSTAR being inserted into | Hubble during First Servicing Mission. |
| ned information from multiple wavelengths from | Hubble, ESO's telescope and NASA's Chandra and used v |
| The | Hubble European Space Agency Information Centre is he |
| the field, Lars Lindberg Christensen from the | Hubble European Space Agency Information Centre offer |
| he died in 1953, and the house remained in the | Hubble family until approximately 1973. |
| entist for education, assistant astronomer and | Hubble Fellow. |
| Edwin | Hubble first thought it to be in the Local Group, but |
| lation of homogeneity) led to the discovery of | Hubble flow, the metric expansion of space that occur |
| e passage of time using clocks moving with the | Hubble flow. |
| ng" observers because they move along with the | Hubble flow. |
| It uses data from the | Hubble Guide Star Catalog II. |
| Hubble had studied the nebula previously at Yerkes an | |
| Hubble has created photo-collage illustrations for pu | |
| Hubble has also curated and exhibited throughout the | |
| Hubble has provided the visual overview of the underl | |
| eve 15 km/pixel resolution from 4300 km, while | Hubble has taken images of up to 114 km/pixel from 60 |
| Photo of IC 349, taken by NASA and The | Hubble Heritage Team (STScI/AURA) 19 September 1999. |
| Edwin | Hubble House is a National Historic Landmark house lo |
| tington Library and Botanic Gardens, the Edwin | Hubble House, and El Molino Viejo (all National Regis |
| Another | Hubble image shows an infant galaxy forming nearby, w |
| Hubble image of the scar taken on 23 July 2009 showin | |
| This new | Hubble image used filters that only let through light |
| Hubble image of the scar taken on July 23 showing a b | |
| This | Hubble image was recorded using polarizing filters (a |
| With the release of a recent | Hubble image there is currently debate about whether |
| A different | Hubble image |
| Hubble image of NGC 2841. | |
| Its main emphasis is on the exquisite | Hubble images that have enabled astronomers to gain e |
| of a star named V838 Monocerotis, taken by the | Hubble in 2004. |
| t called Ursa Major Dwarf, discovered by Edwin | Hubble in 1949. |
| Although not the first space telescope, | Hubble is one of the largest and most versatile, and |
| 2069 | Hubble is a dark-colored main belt asteroid. |
| people who made the discoveries, such as Edwin | Hubble, Isaac Newton, and Albert Einstein. |
| Credit: image by NASA, ESA, The | Hubble Key Project Team, and The High-Z Supernova Sea |
| Galaxies - The introduction of | Hubble Law and discussions of the classification of g |
| Combined | Hubble Legacy images by Robert Gendler. |
| Hubble Legacy Archive Near-UV image of the jet coming | |
| So the | Hubble limit need not define the cosmological event h |
| then at a later time, some objects within the | Hubble limit no longer will be observed (by us) as th |
| Per | Hubble's law, objects at the Hubble limit have an ave |
| Rockefeller was a 2008 honoree of the Edwin P. | Hubble Medal of Initiative, the city of Marshfield, M |
| en and Betty Hearnes were awarded the Edwin P. | Hubble Medal of Initiative during the Charleston Dogw |
| Hubble Middle School or HMS is a public middle school | |
| timore, Maryland, in 1981, and was head of the | Hubble Missions Office at his death. |
| Hubble moved to New York City in 1944, and by the lat | |
| Hubble observations in 2000 revealed an inner torus-l | |
| vatory's Hale Telescope's first light by Edwin | Hubble on January 26, 1949, some 20 years after the P |
| s discovered by the famous US astronomer Edwin | Hubble on August 30, 1935. |
| Hubble on the payload bay just prior to being release | |
| The | Hubble Origins Probe (HOP) is an orbital telescope pr |
| gnificant, because, in a universe in which the | Hubble parameter was constant, light emitted at the p |
| n these scenarios, precise measurements of the | Hubble parameter as a function of redshift are needed |
| In contrast, the | Hubble parameter seems to be decreasing with time, me |
| case the temperature T is proportional to the | Hubble parameter H, i.e. . |
| The | Hubble parameter, H, is ~70.88 km s−1Mpc−1. |
| Later during her youth she was playing at | Hubble Park, where future Hall of Fame Rogers Hornsby |
| Near the bottom (of the | Hubble photo) is the pinkish glow of atomic hydrogen |
| Hubble Postdoctoral Fellowship 2002-2005 | |
| him a graduate student researcher award and a | Hubble postdoctoral fellowship. |
| mas Gonzalez-Torres, the Lead EVA Officer, and | Hubble Program Manager Preston Burch both explained t |
| The physical size of the | Hubble radius (solid line) as a function of the linea |
| During cosmological inflation, the | Hubble radius is constant. |
| eans length, which is very nearly equal to the | Hubble radius for radiation. |
| quated misnomer used by observers before Edwin | Hubble realized that these spiral shaped nebulae were |
| rt activities, and Operations Assistant to the | Hubble Repair Mission Director. |
| At 1.2" away from the nucleus of the galaxy, | Hubble resolved a compact companion. |
| In 1913, | Hubble returned from England and was admitted to the |
| Hubble: Secrets from Space (1998) (TV) (as Professor | |
| e High Speed Photometer (HSP) during the first | Hubble Servicing Mission in 1993. |
| The debut mission of the SpaceCube 1.0, | Hubble Servicing Mission 4, was the first time Xilinx |
| to support other short-term goals, including a | Hubble servicing mission, Mars Exploration Rover exte |
| Hubble Servicing Mission 4: The SpaceCube was the bra | |
| rease the awareness of European Space Agency's | Hubble share (15%), but the contribution of European |
| reate the arcs seen in this resplendent image ( | Hubble Site). |
| The F-sequence references a | Hubble sky region code. |
| the University of Padua in Italy investigated | Hubble Space Telescope images of NGC 2808 taken in 20 |
| ebula Pillars of Creation photo made by NASA's | Hubble Space Telescope. |
| 1 - STS-109: Space Shuttle Columbia flies the | Hubble Space Telescope service mission, its last befo |
| from NASA's Great Observatories, including the | Hubble Space Telescope and the Spitzer Space Telescop |
| include antique stained glass, images from the | Hubble Space Telescope, and the Discovery Pavilion, a |
| our space walk (EVA) to evaluate tools for the | Hubble Space Telescope servicing mission. |
| The | Hubble Space Telescope has identified classical Cephe |
| of The un-coated backup primary mirror for the | Hubble space telescope showing its honeycomb structur |
| A | Hubble Space Telescope (HST) false-color image/diagra |
| As preparation for the Rosetta mission, | Hubble Space Telescope pictures taken on March 12, 20 |
| Galaxy Survey Treasury (ANGST) program on the | Hubble Space Telescope. |
| l analyzed photos of this event taken from the | Hubble Space Telescope. |
| s a visible galaxy that has been imaged by the | Hubble Space Telescope. |
| ir of overlapping galaxies photographed by the | Hubble Space Telescope. |
| A survey with the | Hubble Space Telescope revealed no visible orbiting c |
| mes Webb Space Telescope, the successor to the | Hubble Space Telescope. |
| RS or HRS) was a spectrograph installed on the | Hubble Space Telescope. |
| owalter and Jack J. Lissauer in 2003 using the | Hubble Space Telescope. |
| by her astronaut cousin's voyage to repair the | Hubble Space Telescope, the BBC later made a document |
| The fabrication error in the | Hubble Space Telescope main mirror is the classic exa |
| ional accomplishments and contributions to the | Hubble Space Telescope", and implementation of the sy |
| ht-hour spacewalk to replace components of the | Hubble Space Telescope. |
| The | Hubble Space Telescope has revealed a wealth of new f |
| e, and he is the principal investigator of the | Hubble space telescope mid-UV bright galaxy survey. |
| as, which has been resolved in images from the | Hubble Space Telescope. |
| g, using the ACS and NICMOS instruments on the | Hubble Space Telescope. |
| A search for a faint companion using the | Hubble Space Telescope Wide Field Planetary Camera re |
| could be nearly as good as those taken by the | Hubble Space Telescope. |
| al Investigator the Nuker Team, which used the | Hubble Space Telescope to search for supermassive bla |
| Image of the Bullet Cluster from the | Hubble Space Telescope with total mass contours (domi |
| ed by telescopes using visible light, like the | Hubble Space Telescope. |
| ison, Denise Stephens and Will Grundy with the | Hubble Space Telescope. |
| team of Spanish and US astronomers used NASA's | Hubble Space Telescope to study how the gas stream ra |
| ared group built the NICMOS instrument for the | Hubble Space Telescope and the MIPS instrument for th |
| This image from NASA's | Hubble Space Telescope shows the galaxy cluster Abell |
| part of a much larger star-forming complex-the | Hubble Space Telescope was used to capture images of |
| bject of a major survey for planets, using the | Hubble Space Telescope to look for partial eclipses o |
| the impact of comet Shoemaker-Levy 9 using the | Hubble Space Telescope. |
| By using the | Hubble Space Telescope, he observed approximately one |
| A | Hubble Space Telescope (HST) image of the dust disk i |
| ntended primarily for processing data from the | Hubble Space Telescope. |
| The Cosmic Evolution Survey (COSMOS) is a | Hubble Space Telescope (HST) Treasury Project to surv |
| In 1999, Cole et al. used the | Hubble Space Telescope to find that the dominant popu |
| Hubble Space Telescope photos of the Helix Nebula and | |
| -Infrared Multi-Object Spectrometer aboard the | Hubble Space Telescope indicated that the dust had a |
| 6, more than a dozen telescopes, including the | Hubble Space Telescope and large ground-based observa |
| iable stars, being the most distant galaxy the | Hubble Space Telescope has found to contain Cepheid v |
| thin the NGC 2366 and can be seen below in the | Hubble space telescope image. |
| oronagraphic mode of the ACS instrument on the | Hubble Space Telescope. |
| by the recent observation of camera ACS of the | Hubble space telescope. |
| k encircling the star was discovered using the | Hubble Space Telescope and further investigated by th |
| iden University) on observations done with the | Hubble Space Telescope. |
| ion in Eagle nebula captured in image taken by | Hubble Space Telescope. |
| eres, when viewed from Earth, e.g. through the | Hubble Space Telescope, Ceres has a much larger appar |
| es, including IMAX cameras taken into space on | Hubble Space Telescope Servicing Missions on the Spac |
| of ultraviolet observation (much of it via the | Hubble Space Telescope). |
| rements of weak gravitational lensing with the | Hubble Space Telescope. |
| February 13 - Tune-up and repair work on the | Hubble Space Telescope is started by astronauts from |
| lar resolution of space telescopes such as the | Hubble Space Telescope is often much smaller than a g |
| ga Centauri, based on observations made by the | Hubble Space Telescope and Gemini Observatory on Cerr |
| Its distance long uncertain, the | Hubble Space Telescope's Fine Guidance Sensor was use |
| Further study of the system using | Hubble Space Telescope astrometry revised the mass of |
| rocedure that was later used during the second | Hubble Space Telescope servicing mission to raise the |
| ICMOS Survey, which utilises 180 orbits of the | Hubble Space Telescope to image over 8000 galaxies in |
| ronomers who were permitted to make use of the | Hubble Space Telescope. |
| ument for infrared astronomy, installed on the | Hubble Space Telescope (HST), operating from 1997 to |
| The 2009 impact has been studied by NASA's | Hubble Space Telescope, and the study suggests that t |
| Hubble Space Telescope | |
| The | Hubble Space Telescope reveals many local anomalies i |
| nd the European Space Agency announce that the | Hubble Space Telescope has detected a ring of dark ma |
| e about 30 million light years distant, a 2001 | Hubble Space Telescope survey of the galaxy's Cepheid |
| M49 by | Hubble space telescope |
| In 1999, Mighell & Burke used the | Hubble Space Telescope to confirm that the UMi system |
| rew needs to be rescued from their higher risk | Hubble Space Telescope repair mission. |
| Image from the | Hubble Space Telescope. |
| tsianos was involved with such projects as the | Hubble Space Telescope and was the Deputy Project Man |
| ronomers who were permitted to make use of the | Hubble Space Telescope. |
| NGC 2818 - | Hubble Space Telescope (2008) |
| en with the Advanced Camera for Surveys on the | Hubble Space Telescope, the Very Large Telescope and |
| HCG 31 by | Hubble Space Telescope. |
| NGC 4696 by | Hubble Space Telescope |
| stitute, the science operations center for the | Hubble Space Telescope. |
| In 2007, Bean et al. used the | Hubble Space Telescope (HST) and he found that this b |
| Classifications from the | Hubble Space Telescope Medium Deep Survey". |
| urements with the Fine Guidance Sensors on the | Hubble Space Telescope suggest that the planet's orbi |
| Component B as seen by the | Hubble Space Telescope. |
| The | Hubble Space Telescope extragalactic distance scale k |
| r many years at multiple observatories and the | Hubble Space Telescope, a study obtains the exact mas |
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