Red Giants - Uplift North Hills Prep
... spin. These clouds are called nebula. About 30 million years after the cloud collapsed, its center has reached 15 million kelvin and has become a protostar. As stars continue to go through nuclear fusion from hydrogen gas combining to make deuterons and then two deuterons making helium, the star wil ...
... spin. These clouds are called nebula. About 30 million years after the cloud collapsed, its center has reached 15 million kelvin and has become a protostar. As stars continue to go through nuclear fusion from hydrogen gas combining to make deuterons and then two deuterons making helium, the star wil ...
10.5 The Hertzsprung
... diagram, a pattern begins to form: These are the 80 closest stars to us; note the dashed lines of constant radius. The darkened curve is called the Main Sequence, as this is where most stars are. Also indicated is the white dwarf region; these stars are hot but not very luminous, as they are quite s ...
... diagram, a pattern begins to form: These are the 80 closest stars to us; note the dashed lines of constant radius. The darkened curve is called the Main Sequence, as this is where most stars are. Also indicated is the white dwarf region; these stars are hot but not very luminous, as they are quite s ...
Powerpoint for today
... (as Main Sequence Stars)? A star on Main Sequence has fusion of H to He in its core. How fast depends on mass of H available and rate of fusion. Mass of H in core depends on mass of star. Fusion rate is related to luminosity (fusion reactions make the radiation energy). ...
... (as Main Sequence Stars)? A star on Main Sequence has fusion of H to He in its core. How fast depends on mass of H available and rate of fusion. Mass of H in core depends on mass of star. Fusion rate is related to luminosity (fusion reactions make the radiation energy). ...
Interpreting the HR diagram of stellar clusters
... In fact, it seems that stars are usually born in big groups, as members of a cluster of stars. All the stars in the cluster form at about the same time. So, if we look at a cluster, we see a bunch of stars which are all roughly the same age. However, the stars do not all have the same mass: most ten ...
... In fact, it seems that stars are usually born in big groups, as members of a cluster of stars. All the stars in the cluster form at about the same time. So, if we look at a cluster, we see a bunch of stars which are all roughly the same age. However, the stars do not all have the same mass: most ten ...
Slide 1
... spin. These clouds are called nebula. About 30 million years after the cloud collapsed, its center has reached 15 million kelvin and has become a protostar. As stars continue to go through nuclear fusion from hydrogen gas combining to make deuterons and then two deuterons making helium, the star wil ...
... spin. These clouds are called nebula. About 30 million years after the cloud collapsed, its center has reached 15 million kelvin and has become a protostar. As stars continue to go through nuclear fusion from hydrogen gas combining to make deuterons and then two deuterons making helium, the star wil ...
star
... Life Cycle of a Star (cont.) • When a star’s hydrogen supply is nearly gone, the star leaves the main sequence and begins the next stage of its life cycle. • All stars form in the same way, but stars die in different ways, depending on their masses. • Massive stars eventually become red ...
... Life Cycle of a Star (cont.) • When a star’s hydrogen supply is nearly gone, the star leaves the main sequence and begins the next stage of its life cycle. • All stars form in the same way, but stars die in different ways, depending on their masses. • Massive stars eventually become red ...
l`Astrofilo - Astro Publishing
... (see for example work by Nancy Kiang or John Raven). However, approximately half of the star systems in the galaxy are composed of two or more stars, which leads to the question of how life might evolve differently when presented with two (or more) energy sources, especially if those (i) energy sour ...
... (see for example work by Nancy Kiang or John Raven). However, approximately half of the star systems in the galaxy are composed of two or more stars, which leads to the question of how life might evolve differently when presented with two (or more) energy sources, especially if those (i) energy sour ...
SUMSS - 京都大学
... A typical large galaxy has probably had at least 10 interactions or mergers over its lifetime. Most galaxies are probably ‘assembled’ in this way rather than forming at a single epoch. ...
... A typical large galaxy has probably had at least 10 interactions or mergers over its lifetime. Most galaxies are probably ‘assembled’ in this way rather than forming at a single epoch. ...
Document
... spiral galaxy – 1000,000 light years wide – 10,000 light years thick at the centre – has three distinct spiral arms - Sun is positioned in one of these arms about two-thirds of the way from the galactic center, at a distance of about 30,000 lightyears The Andromeda Galaxy, M31, is the nearest majo ...
... spiral galaxy – 1000,000 light years wide – 10,000 light years thick at the centre – has three distinct spiral arms - Sun is positioned in one of these arms about two-thirds of the way from the galactic center, at a distance of about 30,000 lightyears The Andromeda Galaxy, M31, is the nearest majo ...
Constellations
... Most atlases of today have their origins with those that were derived from Hipparchus and used his “magnitude” system. ...
... Most atlases of today have their origins with those that were derived from Hipparchus and used his “magnitude” system. ...
SHELL H II REGIONS IN NGC 6334
... Not all the stars are in bound orbits… • In the Orion Nebula we found two young massive stars that appear to have been ejected from the same point some 500 years ago (the same age of the University of Valencia). ...
... Not all the stars are in bound orbits… • In the Orion Nebula we found two young massive stars that appear to have been ejected from the same point some 500 years ago (the same age of the University of Valencia). ...
The Next 2-3 Weeks
... • Maser (stimulated emission) when there is long path through gas at same radial velocity (as seen by us). Intense brightening of beam. • Radio VLBI measurements of maser proper motion d/dt and vr ...
... • Maser (stimulated emission) when there is long path through gas at same radial velocity (as seen by us). Intense brightening of beam. • Radio VLBI measurements of maser proper motion d/dt and vr ...
Stars
... ______ 8. The colors that appear when a chemical element emits light are called a. continuous lines. b. absorption lines. c. color lines. d. emission lines. ______ 9. Each element in a hot gas can be identified by a. a unique set of bright emission lines. b. a unique set of bright absorption lines. ...
... ______ 8. The colors that appear when a chemical element emits light are called a. continuous lines. b. absorption lines. c. color lines. d. emission lines. ______ 9. Each element in a hot gas can be identified by a. a unique set of bright emission lines. b. a unique set of bright absorption lines. ...
The Hertzsprung-Russell Diagram
... Most stars lie in the main sequence because if a star is hotter it is brighter. Thus you would expect stars of the same size but different temperatures to form a diagonal line since “hotter means brighter” That Main-Sequence is steeper than a ‘same-size diagonal” shows that larger mass ‘normal’ star ...
... Most stars lie in the main sequence because if a star is hotter it is brighter. Thus you would expect stars of the same size but different temperatures to form a diagonal line since “hotter means brighter” That Main-Sequence is steeper than a ‘same-size diagonal” shows that larger mass ‘normal’ star ...
May 2009 Tz 2
... (d) Alnitak is a main sequence star with a luminosity similar to that of Antares. Use the value quoted in (c)(ii) to deduce that the mass of Alnitak is in the range 16 MS to 40 MS, where MS is the mass of the Sun. ...
... (d) Alnitak is a main sequence star with a luminosity similar to that of Antares. Use the value quoted in (c)(ii) to deduce that the mass of Alnitak is in the range 16 MS to 40 MS, where MS is the mass of the Sun. ...
Galaxies - senwiki
... A galaxy is an immense grouping of stars, planets and dust. The matter in a galaxy is held together by gravitational attraction (i.e. it doesn’t just fall apart and separate) Within galaxies, there are many long cycles of star formation (from dust and gas) and supernovae; more dust and gases. ...
... A galaxy is an immense grouping of stars, planets and dust. The matter in a galaxy is held together by gravitational attraction (i.e. it doesn’t just fall apart and separate) Within galaxies, there are many long cycles of star formation (from dust and gas) and supernovae; more dust and gases. ...
August Skies
... The source of the Perseid meteor shower is actually debris from the comet SwiftTuttle. Every year, the earth passes through the debris stream left by the comet and the earth's atmosphere incinerates the particles into the glowing embers called meteors or “falling stars”. The shower peaks early after ...
... The source of the Perseid meteor shower is actually debris from the comet SwiftTuttle. Every year, the earth passes through the debris stream left by the comet and the earth's atmosphere incinerates the particles into the glowing embers called meteors or “falling stars”. The shower peaks early after ...
26.4 Groups of Stars
... explanation involves matter spiraling into a supermassive black hole with the mass of a billion suns. ...
... explanation involves matter spiraling into a supermassive black hole with the mass of a billion suns. ...
GET WORKSHEETS FROM MY ASSIGNMENTS PAGE Mrs
... 4.The most likely star color to have a planet with life would be ____ because: a. b. Consider Life Span and Life Zone size ...
... 4.The most likely star color to have a planet with life would be ____ because: a. b. Consider Life Span and Life Zone size ...
Properties of Stars in general
... • But its mass (= fuel supply) is only ~ 17 times that of our Sun. • So its life cannot be so long: ~ 17/45,000 that of our Sun ************* ...
... • But its mass (= fuel supply) is only ~ 17 times that of our Sun. • So its life cannot be so long: ~ 17/45,000 that of our Sun ************* ...
ref H-R Spectral types
... In this Activity we have had a look at the Balmer series, and how its occurrence in the photospheres of stars will vary with temperature. The temperature, and hence the colour and spectral line strength characteristics of stars, is used to classify them into types O, B, A, F, G, K and M-type stars. ...
... In this Activity we have had a look at the Balmer series, and how its occurrence in the photospheres of stars will vary with temperature. The temperature, and hence the colour and spectral line strength characteristics of stars, is used to classify them into types O, B, A, F, G, K and M-type stars. ...
Lecture 31
... light years--not a star, and L = 1040 watts--1,000 L (MW)!! .8 to 14(?) Billion years--distance range. L = 1038-1042 watts. Energy comes from a region solar system-sized. Radio Jets. A thermal (synchotron) and non-thermal (black-body) continuous spectrum & broad (gas with varying speeds) lines. Foun ...
... light years--not a star, and L = 1040 watts--1,000 L (MW)!! .8 to 14(?) Billion years--distance range. L = 1038-1042 watts. Energy comes from a region solar system-sized. Radio Jets. A thermal (synchotron) and non-thermal (black-body) continuous spectrum & broad (gas with varying speeds) lines. Foun ...
Serpens
Serpens (""the Serpent"", Greek Ὄφις) is a constellation of the northern hemisphere. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations defined by the International Astronomical Union. It is unique among the modern constellations in being split into two non-contiguous parts, Serpens Caput (Serpent's Head) to the west and Serpens Cauda (Serpent's Tail) to the east. Between these two halves lies the constellation of Ophiuchus, the ""Serpent-Bearer"". In figurative representations, the body of the serpent is represented as passing behind Ophiuchus between Mu Serpentis in Serpens Caput and Nu Serpentis in Serpens Cauda.The brightest star in Serpens is the red giant star Alpha Serpentis, or Unukalhai, in Serpens Caput, with an apparent magnitude of 2.63. Also located in Serpens Caput are the naked-eye globular cluster Messier 5 and the naked-eye variables R Serpentis and Tau4 Serpentis. Notable extragalactic objects include Seyfert's Sextet, one of the densest galaxy clusters known; Arp 220, the prototypical ultraluminous infrared galaxy; and Hoag's Object, the most famous of the very rare class of galaxies known as ring galaxies.Part of the Milky Way's galactic plane passes through Serpens Cauda, which is therefore rich in galactic deep-sky objects, such as the Eagle Nebula (IC 4703) and its associated star cluster Messier 16. The nebula measures 70 light-years by 50 light-years and contains the Pillars of Creation, three dust clouds that became famous for the image taken by the Hubble Space Telescope. Other striking objects include the Red Square Nebula, one of the few objects in astronomy to take on a square shape; and Westerhout 40, a massive nearby star-forming region consisting of a molecular cloud and an H II region.