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More About Individual Term Projects
More About Individual Term Projects

... In this case, you may use the known period of 2.8673 days if your observations do not let you determine the period independently. You will need to observe more than one minimum if you want to independently determine the period of Algol. ...
FROM MOLECULAR CLOUDS TO STARS 1 Star formation and the
FROM MOLECULAR CLOUDS TO STARS 1 Star formation and the

... clouds. CO is the best tracer of the diffuse medium because it is very abundant ([CO]/[ H2], ~ 10-4), it has a relatively high dissociation energy (11.09 eV) and it can be excited from millimetre wavelengths (few Kelvin) to the near infrared (~ 3000 K) in a variety of different physical environments ...
Animated Planets PowerPoint Presentation
Animated Planets PowerPoint Presentation

... Because you asked…….. The next visible comet is Comet Faye. Comet Faye's last perihelion was on November 15, 2006. It reached an apparent magnitude of 9.5 during that orbit. The orbital period of Comet Faye is 7.55 years Its next perihelion will occur on May 29, 2014. During this next appearance, i ...
TE SC.4.E.5.4, 5.3, 5.2, 5.1
TE SC.4.E.5.4, 5.3, 5.2, 5.1

... school. If available, direct students to look at the photograph on p. 3. Ask What is the girl looking at? … thinking about? Encourage students to answer the ?’s on the page. Ask students what other questions they have? Introduce scientists who study space. Ask what tools do astronomers use? That’s r ...
Lab 02: Determining the Solar and Sidereal Days
Lab 02: Determining the Solar and Sidereal Days

... Shown below is Figure 0.5 (page 06) from the textbook. It has been color-inverted so that the sky appears white and the starlight appears gray or black. A long photographic exposure will show the apparent path of the stars as the earth spins. Thus, in exactly one sidereal day, a star would trail out ...
Question paper - Unit 5 (6PH05) - January 2012
Question paper - Unit 5 (6PH05) - January 2012

... young cluster containing a similar number of stars there will be fewer A light main sequence stars. B massive main sequence stars. C red giant stars. D white dwarf stars. (Total for Question 4 = 1 mark) 5 About 25% of the mass of our Universe is thought to consist of dark matter. A key property of d ...
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... This power spectrum is typical for giants. You have a Gaussian envelope of excess power due to the p-mode oscillations, and an exponential rise to low frequencies believed to be due to convection motion. ...
The Death of a Star
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November - Hawaiian Astronomical Society
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Hubble`s Expansion of the Universe
Hubble`s Expansion of the Universe

... a distance indicator as they become too faint. At this point, we use another object known as type Ia supernovae. A supernova marks the end of a star’s life in an extremely energetic explosion. When a supernova explodes, its light intensity brightens to a peak, and then gradually fades over time. For ...
Spiral Galaxies - Astronomy Centre
Spiral Galaxies - Astronomy Centre

... • Our Milky Way Galaxy is just one of Kant’s island universes, which are now referred to as galaxies • The word Universe now refers to the full expanse of space and its contents • While most diffuse nebulae are nearby clouds of gas and dust within the Milky Way, the elliptical and spiral nebulae are ...
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...  Once Kepler’s candidate planetary transit events are identified, a team of ground-based observers perform follow-up observations to rule out false positive events that may mimic a sequence of transits.  The follow-up observations provide additional information about the characteristics of the par ...
Galaxy clusters - University of Iowa Astrophysics
Galaxy clusters - University of Iowa Astrophysics

... • From this, the amount of X-ray emitting gas can be calculated to be 2×1014 M • The mass of X-ray emitting gas is greater than the mass in all the stars in all the galaxies in the cluster and about 10% of the total mass. ...
A-level Physics A Mark scheme Unit 05 - Section 2A
A-level Physics A Mark scheme Unit 05 - Section 2A

... Universe expanding from an extremely dense and hot point over the past 13.6 billion years. The candidate also describes the evidence from, the relative abundances of H and He and the measurement of the microwave background radiation and states they support the big bang theory. Hubble’s Law may also ...
AQA Minutes Template
AQA Minutes Template

... Universe expanding from an extremely dense and hot point over the past 13.6 billion years. The candidate also describes the evidence from, the relative abundances of H and He and the measurement of the microwave background radiation and states they support the big bang theory. Hubble’s Law may also ...


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Targets and their Environments - Pathways Towards Habitable Planets

... However: Earth-like planetary mass in solar system ≈ 2ME  [Fe/H] ≥ -0.3 (Turnbull 08)  requirement: stars in young disk population ...
The Sun is a Star
The Sun is a Star

... Sun. It can damage your eyes. • You can view the Sun by making a small hole in a piece of paper. Then, hold the paper with the hole about a meter from a black piece of paper. You will see an image of the Sun. ...
Physivd Preliminary Module 8.5 The Cosmic Engine
Physivd Preliminary Module 8.5 The Cosmic Engine

...  Barred b) describe some changes that are likely to take place during the life of a star.  State that the life path a star takes depends on its mass.  Briefly describe the main stages and time spent in each stage in a star’s life for the following masses:  <0.1: formation of brown dwarf  0.5-2: ...
Labeling the HR Diagram - Mastering Physics Answers
Labeling the HR Diagram - Mastering Physics Answers

... Spectral type is related to surface temperature, with stars of spectral type O having the highest surface temperature and stars of spectral type M having the lowest surface temperature. In other words, spectral type increases to the left on the H­R diagram. Now proceed to Part E to determine how the ...
neutron star.
neutron star.

... According to conservation of angular momentum, what would happen if a star orbiting in a direction opposite the neutron’s star rotation fell onto a neutron star? A. The neutron star’s rotation would speed up. B. The neutron star’s rotation would slow down. C. Nothing, the directions would cancel eac ...
Celestial Motions
Celestial Motions

... • Their inability to observe stellar parallax was a major factor. ...
Pre-Lab
Pre-Lab

... The word “galaxy,” having been used in English since the fourteenth century, is as old as this language. Galaxy was derived from the French, Greek, and Latin words for milk. To pre-industrial people, lacking bright lights, the Milky Way, a band of diffuse light stretching across the dark sky, would ...
Astronomical Chronicle  for September, 2008
Astronomical Chronicle for September, 2008

... although early autumn may be considered distinct from the last. The length of the day in winter and summer is not differentiated, nor is there a definite concept of the solstices despite the mention of the "turnings of the sun" and "long days" in a line of ...
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Corvus (constellation)



Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.
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