1 - Quia
... B. Carbon C. Hydrogen D. Nitrogen 16. What is the first stage in the life cycle of a star? (2 points) ...
... B. Carbon C. Hydrogen D. Nitrogen 16. What is the first stage in the life cycle of a star? (2 points) ...
Astronomy Part 2 - Malvern Troop 7
... a) List the names of the five most visible planets. Explain which ones can appear in phases similar to lunar phases and which ones cannot, and explain why. b) Find out when each of the five most visible planets that you identified in requirement 5a will be observable in the evening sky during the ne ...
... a) List the names of the five most visible planets. Explain which ones can appear in phases similar to lunar phases and which ones cannot, and explain why. b) Find out when each of the five most visible planets that you identified in requirement 5a will be observable in the evening sky during the ne ...
observingopenclusters-2-2-1
... to the Sun Slide your scope or binoculars parallel to the dog’s back and then move west of that line. You will pick up a large rich field of stars – Open Cluster M41 Procyon (Canis Minor) Locate next large and (also close) Procyon This points the way to 2 very different open clusters in Monocerous, ...
... to the Sun Slide your scope or binoculars parallel to the dog’s back and then move west of that line. You will pick up a large rich field of stars – Open Cluster M41 Procyon (Canis Minor) Locate next large and (also close) Procyon This points the way to 2 very different open clusters in Monocerous, ...
EX - Uplift North Hills Prep
... (ii) Modern techniques enable the measurement from Earth’s surface of stellar parallax angles as small as 5.0 × 10–3 arcsecond. Calculate the maximum distance that can be measured using the method of stellar parallax. ...
... (ii) Modern techniques enable the measurement from Earth’s surface of stellar parallax angles as small as 5.0 × 10–3 arcsecond. Calculate the maximum distance that can be measured using the method of stellar parallax. ...
Name _________ Date _____________ Period ______ Skills
... COMPOSITION OF STARS _____ 5. The band of colors produced when white light passes through a prism is a(n) a. color wheel. b. emission line. c. ultraviolet light. d. spectrum. _____ 6. A hot, solid object gives off a(n) a. continuous spectrum. b. absorption spectrum. c. emission line. d. partial spec ...
... COMPOSITION OF STARS _____ 5. The band of colors produced when white light passes through a prism is a(n) a. color wheel. b. emission line. c. ultraviolet light. d. spectrum. _____ 6. A hot, solid object gives off a(n) a. continuous spectrum. b. absorption spectrum. c. emission line. d. partial spec ...
Masers and high mass star formation Claire Chandler
... If you know flux density, dust temperature, distance to source, and opacity characteristics of dust, you can get Md. Assume dust to gas ratio and you get total mass of object. ...
... If you know flux density, dust temperature, distance to source, and opacity characteristics of dust, you can get Md. Assume dust to gas ratio and you get total mass of object. ...
Astro 10 Practice Test 2
... d. Mostly iron, similar to the hot iron core of the Earth, with a little bit of helium and some heavier elements. 17. On a clear autumn night, you spend some time examining the glowing HII regions in the galaxy M33, using a large reflecting telescope. If you were IN the galaxy M33, looking at these ...
... d. Mostly iron, similar to the hot iron core of the Earth, with a little bit of helium and some heavier elements. 17. On a clear autumn night, you spend some time examining the glowing HII regions in the galaxy M33, using a large reflecting telescope. If you were IN the galaxy M33, looking at these ...
What is a Scientist? - Cockeysville Middle School
... Stars are giant spheres of glowing gases. A star is powered by nuclear fusion. This is a process whereby hydrogen atoms are fused together to create helium atoms. In the process a tremendous amount of energy is given off in the form of electromagnetic waves and heat. There are billions of stars in a ...
... Stars are giant spheres of glowing gases. A star is powered by nuclear fusion. This is a process whereby hydrogen atoms are fused together to create helium atoms. In the process a tremendous amount of energy is given off in the form of electromagnetic waves and heat. There are billions of stars in a ...
Ages of Star Clusters - Indiana University Astronomy
... sequence sooner. In a cluster in which all the stars formed at the same time, the stars “peel off” the main sequence from the top, leaving only progressively less and less massive stars remaining on the main sequence as time goes by. The main sequence turnoff is the point on the main sequence for wh ...
... sequence sooner. In a cluster in which all the stars formed at the same time, the stars “peel off” the main sequence from the top, leaving only progressively less and less massive stars remaining on the main sequence as time goes by. The main sequence turnoff is the point on the main sequence for wh ...
A-36_SF
... • We learn about star formation by studying groups of stars – Color indicates age: hot, massive, blue stars die quickly – …but not before they blow away the cloud they were born from – Galactic rotation disperses clustered stars ...
... • We learn about star formation by studying groups of stars – Color indicates age: hot, massive, blue stars die quickly – …but not before they blow away the cloud they were born from – Galactic rotation disperses clustered stars ...
Star Basics
... helium. At these temperatures most of the hydrogen is ionized, so the hydrogen lines are weak. Both HeI and HeII (singly ionized helium) are seen in the higher temperature examples. The radiation from O5 stars is so intense that it can ionize hydrogen over a volume of space 1000 light years across. ...
... helium. At these temperatures most of the hydrogen is ionized, so the hydrogen lines are weak. Both HeI and HeII (singly ionized helium) are seen in the higher temperature examples. The radiation from O5 stars is so intense that it can ionize hydrogen over a volume of space 1000 light years across. ...
The magnitude scale
... times fainter again, i.e. 10,000 times fainter than one at the naked eye limit, and so on. ...
... times fainter again, i.e. 10,000 times fainter than one at the naked eye limit, and so on. ...
The Birth of Stars Guiding Questions • Because stars shine by
... 1. Why do astronomers think that stars evolve (bad use of term – this is about the birth, life and death of stars and that is NOT evolution)? 2. What kind of matter exists in the spaces between the stars? 3. In what kind of nebulae do new stars form? 4. What steps are involved in forming a star like ...
... 1. Why do astronomers think that stars evolve (bad use of term – this is about the birth, life and death of stars and that is NOT evolution)? 2. What kind of matter exists in the spaces between the stars? 3. In what kind of nebulae do new stars form? 4. What steps are involved in forming a star like ...