The Orion Nebula Great Nebula in Orion

Jul 30, 2014

180 likes | 291 Views

The Orion Nebula Great Nebula in Orion. M 42 NGC 1976 1,350 ly away 25 ly wide m +4.0. Nebula Video.

Share Presentation

Embed Code

Link

nebula video
orion
nebulagreat nebula

javier

Download Presentation

The Orion Nebula Great Nebula in Orion

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

The Orion NebulaGreat Nebula in Orion M 42 NGC 1976 1,350 ly away 25 ly wide m +4.0

Nebula Video

Orion Nebula: Star-forming Region

Orion Nebula: Star-forming Region. Solar Nebula. Flattening the Solar Nebula. Disks Around Other Stars. Steps in Planet Formation. Condensation Accretion Nebular Capture (Jovian Planets only) After planets form, the solar wind clears the nebula: gas and dust are blown away.

1.02k views • 25 slides

The Orion Nebula (M42)

The Orion Nebula (M42). THE GLOBULAR CLUSTER M13. Credit: Yuugi Kitahara . Andromeda “Nebula” (M31). Andromeda “Nebula” (M31). Velocity dependence on radius for a planet orbiting the Sun…. Rotation curve of galaxies. Real measurements. This class. Formation and evolution of galaxies

1.02k views • 44 slides

The Orion Nebula from HST

The Orion Nebula from HST. Orion stars from the VLT.  1 Ori C. Orion Trapezium from HST. Orion visible + radio (visible = HST, radio = VLA + GBT). Orion HII region ionization front map (O’Dell 2001). Schematic drawing of Orion, O’Dell+ 2008.

551 views • 9 slides

Region in the Constellation Orion named the Orion Nebula which is the closest star formation region to us.

Region in the Constellation Orion named the Orion Nebula which is the closest star formation region to us. Jets and disks appear to be part of the star birth process.

487 views • 12 slides

Orion

. . . . . . . . . . . Ecliptic . . . . . Celestial Equator. Orion. . . . - brightest of all the constellations. . . . M42. . . . . The Heavens are Telling. 6. THE ORION NEBULA. ARRAT 16. MESSIER 42, (M42) containing “THE TRAPEZIUM CLUSTER”.

1.64k views • 126 slides

The Orion Nebula (M42)

The Orion Nebula (M42). Astronomy By Claire Andrues. Where is it located in our sky?.

244 views • 10 slides

Ages and Age Spreads in The Orion Nebula Cluster Rob Jeffries: Keele University, UK

Ages and Age Spreads in The Orion Nebula Cluster Rob Jeffries: Keele University, UK. Absolute Ages The HR diagram of the ONC Evidence for luminosity and age spreads. Absolute Age Constraints. 3 Myr. 5 Myr. UMS evolution 2.8 - 5.2 Myr (68%) Naylor 2009, MNRAS, 399, 432

410 views • 30 slides

Nebula

Nebula. By: Mckayla Morrison. What is a Nebula?.

343 views • 11 slides

Large Scale CO Emission in the Orion Nebula

Large Scale CO Emission in the Orion Nebula. HST. CO (2-1). Núria Marcelino (NRAO-CV) Olivier Berné (Leiden Obs , The Netherlands) José Cernicharo (CSIC /INTA , Spain). The closest (brightest) massive star forming region Prototypical source: observed at almost all wavelengths

304 views • 19 slides

New results on the giant dark silhouette disk dd114-426 in the Orion Nebula.

August 12 th , 2011. A nna M iotello. Graduated in Physics at University of Milan, Italy (2011). New results on the giant dark silhouette disk dd114-426 in the Orion Nebula. miotello@stsci.edu. Doing Master’s degree in Astrophysics at University of Milan, Italy. Anna Miotello

326 views • 25 slides

NEBULA!

NEBULA!. A nebula is a cloud of gas and dust. Stars are formed in a nebula. The size of a nebula varies depending on the size of the original cloud of dust. http://nssdc.gsfc.nasa.gov/image/astro/hst_pillars_m16.jpg. Protostar !.

507 views • 16 slides

ORION

ORION. Sirius. CANIS MAJOR. +6. arc-seconds. 0. -6. 124. 0. 31. 62. 93. arc-seconds. 1850. +6. arc-seconds. 0. -6. 124. 0. 31. 62. 93. arc-seconds. 1855. +6. arc-seconds. 0. -6. 124. 0. 31. 62. 93. arc-seconds. 1860. +6. arc-seconds. 0. -6. 124. 0. 31.

492 views • 24 slides

What have we learned from Eclipsing Binaries in the Orion Nebula?

What have we learned from Eclipsing Binaries in the Orion Nebula?. Keivan Guadalupe Stassun Vanderbilt University. Dynamical Masses of PMS Stars circa 2013. N=33 M < 2 M sun. Single stars Circumstellar disk “rotation curve” Binary stars Astrometric Eclipsing.

365 views • 22 slides

2MASS Image of the Orion Nebula

2MASS Image of the Orion Nebula. Massive Cores in Orion. Di Li NAIC, Cornell University February, 2002. HMSF vs. LMSF. Spatial Distinction LMSF region: Taurus GMCs: Orion “Intermediate”: Ophiuchus Higher Star Forming Efficiency for HMSF “Thermal” vs.“Turbulent” Cores

626 views • 45 slides

HST survey of the Orion Nebula Cluster Team Meeting – 12-13 September 2011

HST survey of the Orion Nebula Cluster Team Meeting – 12-13 September 2011. Mass Accretion Rates from H α measurements. Nino Panagia STScI INAF/CT Supernova Ltd. Main Characters in this study. Nino Panagia (STScI) Nicola Da Rio (ESA) Guido De Marchi (ESA) Massimo Robberto (STScI)

299 views • 22 slides

Crab Nebula

Crab Nebula. Neutrinos in Cosmology, Astro, Particle & Nuclear Physics 16 - 24 September 2009, Erice, Sicily. Physics Opportunities with Supernova Neutrinos. Georg Raffelt, Max-Planck-Institut für Physik, München. Stellar Collapse and Supernova Explosion. Main-sequence star.

781 views • 64 slides

The Radio/X-ray Connection in Young Stellar Objects in the Orion Nebula Cluster

The Radio/X-ray Connection in Young Stellar Objects in the Orion Nebula Cluster. By Scott J. Wolk and Jan Forbrich. Güdel (2002). Classes of Young Stellar Objects (YSOs). “class 0”. “class I”. Greene (2001). “class II”. “class III”. Lada (1987) André et al. (2000). ( (thermal) X-rays,

574 views • 42 slides

The IMF of the Orion Nebula Cluster Across the H-burning Limit

The IMF of the Orion Nebula Cluster Across the H-burning Limit. Nicola Da Rio HST Orion Treasury Science Meeting STScI, Baltimore, September 12 th 13 th 2011. Motivation. In order to derive the properties of PMS stars in Orion we need individual spectral types.

302 views • 17 slides

The Nebula Beginning

The Nebula Beginning. The Nebula Beginning. The Nebula Beginning. M17. The Nebula Beginning. M1 – The Orion Nebula. The Nebula Beginning. OXYGEN-RICH SUPERNOVA REMNANT IN THE LARGE MAGELLANIC CLOUD

345 views • 13 slides

Orion

Orion. Constellation: The Hunter. Orion. Orionis Abbreviation Ori 5 stars with known planets 3 Messier Objects M42, M43, M78 2 meteor showers Orionids October Halley’s Comet χ Orionids. Orion. Astride the celestial equator Visible from all over the world

388 views • 11 slides

Nebula

Nebula. A cloud of gas and dust; the first stage in a stars life (where stars are “born”). en.wikipedia.org/wiki/Image:Orion_Nebula_-_Hubble_2006. Protostar. A star during its first contraction (a “baby” star). http://www.celestiamotherlode.net/catalog/images/screenshots/fictional/protostar.

684 views • 13 slides

The Birth of Stars and Planets in the Orion Nebula

The Birth of Stars and Planets in the Orion Nebula. K. Smith (STScI). Orion (the hunter). Why Orion?. Closest massive star forming region (450pc) (there are closer low mass star forming regions) Relatively young (1Myr) Now believed that our Sun started life in such an environment.

861 views • 49 slides

More Related