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s-process
s-process

... -2.1, when low-mass AGB stars begin to contribute from double shell burning. The s-process then dominates Ba production. The origin of heavy metals at the lowest Galactic metallicity ([Fe/H] = -4) is still not understood, but may be dominated by the weak s-process, or by a separate r-process in mass ...
Magnitudes lesson plan
Magnitudes lesson plan

... that he could see from his latitude into six classes of brightness. His idea of six classes probably came from the Babylonians whose base number was six. The formal introduction of six magnitudes has been credited to Ptolemy (100-150 A.D.) who was a Greek/Egyptian astronomer. He simply advanced the ...
Glossary abiotic factors [AY-bye-aw-tik FAK-turz] the non
Glossary abiotic factors [AY-bye-aw-tik FAK-turz] the non

... electric force ♫ the force exerted by an object with an electric charge; can be a force of attraction or a force of repulsion (p. 468) electrical energy ♫ the energy provided by the flow of electrons in an electric circuit (p. 511) electrical power ♫ the rate at which electrical energy is produced o ...
Spectroscopic confirmation of a galaxy at redshift z=8.6
Spectroscopic confirmation of a galaxy at redshift z=8.6

... is probably surrounded by other sources that contributed to the reionization of the Universe, but which have not yet been discovered or characterized. With the current capabilities of the Wide Field Camera 3 and sensitive spectrographs in the near-infrared on 8–10-m-class telescopes such as SINFONI ...
Celestial Sphere
Celestial Sphere

... more on Constellations (Week 4) ...
Debris disks: dynamics of small particles in
Debris disks: dynamics of small particles in



... We have found internal motions of trapezium systems to be generally small (or even below the observational errors), which is consistent with these systems, being gravitationally bound. However, in a few cases, we found stars to be escaping, some of them with velocities high enough to identify them a ...
Magnitudes - Astronomy @ Walton High School
Magnitudes - Astronomy @ Walton High School

SXDS Highlights : Subaru / FOCAS Spectroscopy
SXDS Highlights : Subaru / FOCAS Spectroscopy

... Natural guide star AO system on Subaru telescope with IRCS. 154 hours of observation in total. 13 FoVs with 36 LBGs , 1 RadioG., and 7 DRGs are observed. Typical on-source effective integration is 5 hours. Typical PSF size at the target position is FWHM=0.2” (~1.5kpc@z=3) ...
A noble record
A noble record

... meteorites reveals a cornucopia of contributing environments. In this account, we will follow the noble gas evidence in meteorites from the early solar system and show how it illuminates different aspect of its history. ...
Effect of the stellar spin history on the tidal evolution of close
Effect of the stellar spin history on the tidal evolution of close

... and very low-mass stars (0.1 M ). We tested two stellar spin evolution profiles, one with fast initial rotation (1.2 day rotation period) and one with slow initial rotation (8 day period). We tested the effect of varying the stellar and planetary dissipations, and the planet’s mass and initial orbit ...
Constellation ARA
Constellation ARA

... planet 12152 Aratus are Hades, and Poseidon. When the named in his honour youngest child, Zeus, was born, his mother Rhea hid him in Crete and gave Cronus a stone to swallow, telling him the stone was Zeus. When Zeus grew up, he made Cronus vomit his brothers and sisters. Once freed, they banded tog ...
Y-band Imaging of Extragalatic Fields and High redshift
Y-band Imaging of Extragalatic Fields and High redshift

... cal Astronomy Observatory (LOAO) and the Maidanak Observatory. The deepest limit magnitude of 260 minutes exposure is Y = 21.5 AB mag in case of LOAO and Y = 22 AB mag for the Maidanak Observatory. Using the Y-band imaging data, we measured photometric calibration parameters of Y-band. We got two ph ...
Discovering Planetary Nebula Geometries: Explorations with a
Discovering Planetary Nebula Geometries: Explorations with a

- University of Manitoba
- University of Manitoba

... We must first convert the images to 32-bit format, subtract the overscan region from each image, crop each image to 520 x 512 pixel size, subtract the master bias frame from each image, subtract the master dark frame from each image, and finally divide each image by the master flat. Select the usabl ...
The extreme ultraviolet and X-ray Sun in Time: High
The extreme ultraviolet and X-ray Sun in Time: High

... decays over time as a result of stellar spin-down. The early Sun’s X-ray (≈1−100 Å) and extreme-ultraviolet (EUV; ≈100−900 Å) emissions could thus have exceeded the present-day Sun’s level by orders of magnitude (Ribas et al. 2005). By driving atmospheric erosion, such extreme radiation levels were ...
@let@token Stellar Oscillations: Pulsations of Stars Throughout the
@let@token Stellar Oscillations: Pulsations of Stars Throughout the

... requires heat/energy, so less energy is radiated out the top of the convection zone than enters at its base. It is possible (but not easy) to show that this energy gain occurs at maximum density during the pulsations, so this naturally leads to driving. This explains the driving in pulsating white d ...
Planet Hunters Education Guide
Planet Hunters Education Guide

... such as Galaxy Zoo, Snapshot Serengeti or Seafloor Explorer, require volunteers to identify objects in images. Other projects, such as Whale FM or Bat Detective need people to identify sounds, while Old Weather and Ancient Lives utilize the human ability to identify words and letters and to decipher ...
The Solar System - Royal Astronomical Society of Canada
The Solar System - Royal Astronomical Society of Canada

... T h at since the discovery of the new planet Pluto the diameter of our system has become about 8,000,000,000 miles. T h at the orbits of the bodies revolving round the sun are not closed ellipses round a sun at rest, as usually described, bu t open helical paths round a sun in motion on its flight t ...
PDF format
PDF format

... What did astronomers debate about the nature of spiral nebulae until the 1920s? ...
Stellar Spectroscopy
Stellar Spectroscopy

... temperature, velocity and composition of an object as well as be used to infer mass, distance and many other pieces of information. Spectroscopy is done at all wavelengths of the electromagnetic spectrum, from radio waves to gamma rays; but here we will focus on optical light. The three types of spe ...
Exercise 11
Exercise 11

... The ability to construct devices to precisely measure angles in the sky occurred before the in­ vention of the telescope. The Dane Tycho Brahe (1561-1626) was recognized for his keen eyesight and for the construction of massive and accurate quadrants. His ability to make and record accurate position ...
14.1 Introduction - University of Cambridge
14.1 Introduction - University of Cambridge

... ure 13.11) following the ejection of the star’s outer layers in the planetary nebula stage. In either case, without an internal source of energy, white dwarfs simply cool off at an essentially constant radius as they slowly deplete their supply of thermal energy. ...
Teacher`s Guide - Cornell Science Inquiry Partnerships
Teacher`s Guide - Cornell Science Inquiry Partnerships

... d. Accuracy of Measurements. Also discuss with the students how well we can measure the above two properties on the pictures. The number of wrinkles might be possible to count, but only if the photograph has high enough resolution. However, the height of each person might be possible to estimate (e. ...
65008_StarFinderPart2
65008_StarFinderPart2

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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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