The Day We Found the Universe
... spiraling nebulae were nothing less than separate galaxies. At the same time, a few hundred miles south at Mount Wilson, near Los Angeles, Harlow Shapley resized the Milky Way, measuring it as far larger than previously thought and shoving our Sun o to the side, away from the galaxy's hub. As Shaple ...
... spiraling nebulae were nothing less than separate galaxies. At the same time, a few hundred miles south at Mount Wilson, near Los Angeles, Harlow Shapley resized the Milky Way, measuring it as far larger than previously thought and shoving our Sun o to the side, away from the galaxy's hub. As Shaple ...
TheSkyX - Physics!
... or copied only in accordance with the terms of the agreement (www.bisque.com/eula). It is against the law to copy the software on any medium except as specifically allowed in the license or nondisclosure agreement. The purchaser may make one copy of the software for backup purposes. No part of this ...
... or copied only in accordance with the terms of the agreement (www.bisque.com/eula). It is against the law to copy the software on any medium except as specifically allowed in the license or nondisclosure agreement. The purchaser may make one copy of the software for backup purposes. No part of this ...
FY96
... major common motion groups. The consequence is that the halo is dynamically young, with comingling but identifiable streams of stars of different ages, metallicities and trajectories, presumably from capture of satellite systems by the Milky Way. This "can of worms" model for the halo may explain se ...
... major common motion groups. The consequence is that the halo is dynamically young, with comingling but identifiable streams of stars of different ages, metallicities and trajectories, presumably from capture of satellite systems by the Milky Way. This "can of worms" model for the halo may explain se ...
WFC3 Science White Paper - Space Telescope Science Institute
... Organization Chart 11. Appendix: Acronym List ...
... Organization Chart 11. Appendix: Acronym List ...
W.M. Keck Observatory Annual Report 2009
... initial emphasis on proving whether or not planets exist beyond our own Solar System. With over 400 of these worlds identified within the last fifteen years, modern astronomers continue their hunt for the planets with the lowest possible mass. The Keck I telescope has been the most prolific scientif ...
... initial emphasis on proving whether or not planets exist beyond our own Solar System. With over 400 of these worlds identified within the last fifteen years, modern astronomers continue their hunt for the planets with the lowest possible mass. The Keck I telescope has been the most prolific scientif ...
- Isaac Newton Group of Telescopes
... t gives me great pleasure to write a few words on behalf of the Joint Steering Committee as an introduction to this biennial report of the Isaac Newton Group of telescopes. The two years that this report covers have seen the ING produce results which have advanced astronomical research across a very ...
... t gives me great pleasure to write a few words on behalf of the Joint Steering Committee as an introduction to this biennial report of the Isaac Newton Group of telescopes. The two years that this report covers have seen the ING produce results which have advanced astronomical research across a very ...
Word doc - Infinity Internet
... Adam, M.G. The Changing Face of Astronomy in Oxford (1920-60). Quarterly Journal of the Royal Astronomical Society 37:2 (June 1996) 153-179. Adams, George. Astronomical & geographical essays: containing, I. A full and comprehensive view, on a new plan, of the general principles of astronomy. II. The ...
... Adam, M.G. The Changing Face of Astronomy in Oxford (1920-60). Quarterly Journal of the Royal Astronomical Society 37:2 (June 1996) 153-179. Adams, George. Astronomical & geographical essays: containing, I. A full and comprehensive view, on a new plan, of the general principles of astronomy. II. The ...
The ALMA Universe - ALMA Observatory
... out better observations of objects that are more extended in the sky, such as the giant molecular clouds in the Milky Way or nearby galaxies. ...
... out better observations of objects that are more extended in the sky, such as the giant molecular clouds in the Milky Way or nearby galaxies. ...
solar system
... last motion was made necessary because Copernicus conceptualized the Earth's annual motion as the result of the Earth being embedded in a spherical shell centered on the Sun. Its axis of rotation therefore did not remain parallel to itself with respect to the xed stars. To keep the axis parallel to ...
... last motion was made necessary because Copernicus conceptualized the Earth's annual motion as the result of the Earth being embedded in a spherical shell centered on the Sun. Its axis of rotation therefore did not remain parallel to itself with respect to the xed stars. To keep the axis parallel to ...
Earth Centered Universe Pro V6.0
... If you, the licensee, have purchased a license to use the Earth Centered Universe Pro (ECU) (the “Software”), or upgraded from a previous version of the Software, by sending Nova Astronomics the appropriate fee or by purchasing from a retailer, and you are in possession of a registration number and ...
... If you, the licensee, have purchased a license to use the Earth Centered Universe Pro (ECU) (the “Software”), or upgraded from a previous version of the Software, by sending Nova Astronomics the appropriate fee or by purchasing from a retailer, and you are in possession of a registration number and ...
Report from the Subaru Telescope for External
... Toshikawa et al. (2012) have discovered the most distant protocluster of galaxies ever found at z = 6.01. The overdensity of the protocluster is significant at the 6σ level, based on the surface number density of i’-dropout galaxies. Follow-up spectroscopy revealed that 8 are clustering in a narrow r ...
... Toshikawa et al. (2012) have discovered the most distant protocluster of galaxies ever found at z = 6.01. The overdensity of the protocluster is significant at the 6σ level, based on the surface number density of i’-dropout galaxies. Follow-up spectroscopy revealed that 8 are clustering in a narrow r ...
Starter Edition Handbook
... constellations will help you find the more distant wonders of the Universe that your binoculars or telescope can reveal. Once you can find you way around the sky you will be able to find bright double stars. The next step is to hunt down your first real deep sky objects: open star clusters. Open st ...
... constellations will help you find the more distant wonders of the Universe that your binoculars or telescope can reveal. Once you can find you way around the sky you will be able to find bright double stars. The next step is to hunt down your first real deep sky objects: open star clusters. Open st ...
Project T-REX: Italian technologies for E
... At the same time, the frontier technologies that will developed and applied within T-REX for the construction of mirrors and instruments to be mounted on E-ELT falls explicitly and naturally also in the domain of Sensory Devices, activities set of high priority and strategic relevance for the Countr ...
... At the same time, the frontier technologies that will developed and applied within T-REX for the construction of mirrors and instruments to be mounted on E-ELT falls explicitly and naturally also in the domain of Sensory Devices, activities set of high priority and strategic relevance for the Countr ...
Astronomers` Observing Guides
... space. Each volume is actually two books in one. The first provides a comprehensive overview of the class of celestial object it treats, including the latest information on both their physical properties and their significance in the grand cosmic scheme of things. The second covers observing technique ...
... space. Each volume is actually two books in one. The first provides a comprehensive overview of the class of celestial object it treats, including the latest information on both their physical properties and their significance in the grand cosmic scheme of things. The second covers observing technique ...
LTBN_Script - Let There Be Night
... did brag about it in your book Starry Messenger. Galileo: (Belly laugh) Aahhh, I have to confess, I didn’t really invent the telescope. A Dutch lens maker named Hans Lippershey and others actually came up with the idea and tried to patent it. I heard about his idea and then crafted a few telescopes ...
... did brag about it in your book Starry Messenger. Galileo: (Belly laugh) Aahhh, I have to confess, I didn’t really invent the telescope. A Dutch lens maker named Hans Lippershey and others actually came up with the idea and tried to patent it. I heard about his idea and then crafted a few telescopes ...
Horace Welcome Babcock - National Academy of Sciences
... In 1930 Horace also began his undergraduate studies at Caltech, a personal goal since childhood. He was well aware that the design and assembly of a 200-inch telescope were under way there. He majored in engineering (as his father did in Berkeley), but also studied physics (electricity and light, w ...
... In 1930 Horace also began his undergraduate studies at Caltech, a personal goal since childhood. He was well aware that the design and assembly of a 200-inch telescope were under way there. He majored in engineering (as his father did in Berkeley), but also studied physics (electricity and light, w ...
SpeX Observing Manual - NASA Infrared Telescope Facility
... We also strongly recommend that observers acquire at least three AB cycles (six spectra) of their targets whatever the brightness. This allows any systematic effects in the data to be removed by applying a median combination to the spectra. The most prominent of these effects are the star-like feat ...
... We also strongly recommend that observers acquire at least three AB cycles (six spectra) of their targets whatever the brightness. This allows any systematic effects in the data to be removed by applying a median combination to the spectra. The most prominent of these effects are the star-like feat ...
Understanding Resolution
... One might make the assumption then it would be much easier to resolve fainter stars as the smaller central disks could be closer making observation of a clean separation apparent before they would overlap. However, the inability of the eye to see fainter light at some point overwhelms the benefit of ...
... One might make the assumption then it would be much easier to resolve fainter stars as the smaller central disks could be closer making observation of a clean separation apparent before they would overlap. However, the inability of the eye to see fainter light at some point overwhelms the benefit of ...
How To Use Plastic Sextants - Starpath School of Navigation
... using the sextant for its full range of functions, the traditional mirror is a better choice. On the other hand, Davis sells the mirrors separately, so one could in principle replace the full view mirror on a Mark 25 with a traditional mirror from a Mark 15. Such a change, however, would be more or ...
... using the sextant for its full range of functions, the traditional mirror is a better choice. On the other hand, Davis sells the mirrors separately, so one could in principle replace the full view mirror on a Mark 25 with a traditional mirror from a Mark 15. Such a change, however, would be more or ...
Sample pages 1 PDF
... At about 3◦ in angular width, you need a very wide field of view if you want to see the whole thing in its entirety. In practice very few telescopes other than short focal length refractors or Newtonian reflectors provide anything like the necessary fields of view, and certainly not the popular SCT ...
... At about 3◦ in angular width, you need a very wide field of view if you want to see the whole thing in its entirety. In practice very few telescopes other than short focal length refractors or Newtonian reflectors provide anything like the necessary fields of view, and certainly not the popular SCT ...
Five-Hundred Meter Aperture Spherical Radio
... However, in the course of examples it was discovered that the straight-line model is of no use since it always yields some negative cable tensions over the required FAST workspace. Therefore, two alternative cable-arrangement designs are presented for FAST which overcome the problem of negative cabl ...
... However, in the course of examples it was discovered that the straight-line model is of no use since it always yields some negative cable tensions over the required FAST workspace. Therefore, two alternative cable-arrangement designs are presented for FAST which overcome the problem of negative cabl ...
What To See Telescope(Jul-Sept) v1 - One
... most objects. Sights that benefit from larger-aperture telescopes, and descriptions of what you will see with a 6-inch or 8-inch telescope are included where appropriate. The guide also assumes you are somewhat familiar with the night sky, and that you know how to locate specific major constellation ...
... most objects. Sights that benefit from larger-aperture telescopes, and descriptions of what you will see with a 6-inch or 8-inch telescope are included where appropriate. The guide also assumes you are somewhat familiar with the night sky, and that you know how to locate specific major constellation ...
ATACAMA LARGE MILLIMETER / SUBMILLIMETER ARRAY
... 25, and Japan having contracted for their first three. These antennas are the highest precision radio telescopes ever built. The first antenna arrived at the ALMA OSF on April 27, 2007. Construction of the building on the 5000 m elevation Array Operations Site will be completed soon, and constructio ...
... 25, and Japan having contracted for their first three. These antennas are the highest precision radio telescopes ever built. The first antenna arrived at the ALMA OSF on April 27, 2007. Construction of the building on the 5000 m elevation Array Operations Site will be completed soon, and constructio ...
Astronomy Laboratory Manual
... The problem, of course, is that they don't know the bright stars and major constellations. Unfortunately, many never find the help they need and give up astronomy and stick their telescope in the closet. With proper advice and guidance, anyone can turn into a starhopping skymaster. The first thing y ...
... The problem, of course, is that they don't know the bright stars and major constellations. Unfortunately, many never find the help they need and give up astronomy and stick their telescope in the closet. With proper advice and guidance, anyone can turn into a starhopping skymaster. The first thing y ...
THE PERIOD OF ROTATION OF THE SUN
... digitally and can display the data as a chart record or as sound. VIREO simulates modern astronomical observation by accessing a number of databases, both on-line and in data files provided with the software. The basic VIREO database includes data from the Hubble Guide Star Catalog (about 16 million ...
... digitally and can display the data as a chart record or as sound. VIREO simulates modern astronomical observation by accessing a number of databases, both on-line and in data files provided with the software. The basic VIREO database includes data from the Hubble Guide Star Catalog (about 16 million ...
History of the telescope
The earliest known working telescopes appeared in 1608 and are credited to Hans Lippershey. Among many others who claimed to have made the discovery were Zacharias Janssen, a spectacle-maker in Middelburg, and Jacob Metius of Alkmaar. The design of these early refracting telescopes consisted of a convex objective lens and a concave eyepiece. Galileo used this design the following year. In 1611, Johannes Kepler described how a telescope could be made with a convex objective lens and a convex eyepiece lens and by 1655 astronomers such as Christiaan Huygens were building powerful but unwieldy Keplerian telescopes with compound eyepieces. Hans Lippershey is the earliest person documented to have applied for a patent for the device.Isaac Newton is credited with building the first ""practical"" reflector in 1668 with a design that incorporated a small flat diagonal mirror to reflect the light to an eyepiece mounted on the side of the telescope. Laurent Cassegrain in 1672 described the design of a reflector with a small convex secondary mirror to reflect light through a central hole in the main mirror.The achromatic lens, which greatly reduced color aberrations in objective lenses and allowed for shorter and more functional telescopes, first appeared in a 1733 telescope made by Chester Moore Hall, who did not publicize it. John Dollond learned of Hall's invention and began producing telescopes using it in commercial quantities, starting in 1758.Important developments in reflecting telescopes were John Hadley's production of larger paraboloidal mirrors in 1721; the process of silvering glass mirrors introduced by Léon Foucault in 1857; and the adoption of long lasting aluminized coatings on reflector mirrors in 1932. Almost all of the large optical research telescopes used today are reflectors.The era of radio telescopes (along with radio astronomy) was born with Karl Guthe Jansky's serendipitous discovery of an astronomical radio source in 1931. Many types of telescopes were developed in the 20th century for a wide range of wavelengths from radio to gamma-rays.