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...e-radiates it as [[thermal radiation]]. The [[luminosity]] of the zodiacal dust in the Solar System is about <math>10^{-7}</math> relative to the luminosit *[[Cosmic dust]] ...

{{Short description|Cosmic stream of charged particles}} ...date=2016-09-28}}</ref> Because new stars and planets form from gases, the cosmic winds that push the gases away are preventing new stars from forming and ar ...

...{cite journal | last=Corasaniti | first=P. S. | title=The impact of cosmic dust on supernova cosmology | journal=Monthly Notices of the Royal Astronomical ...

...and is defined by a region of low [[H I region|neutral hydrogen gas]] and dust [[column density]].<ref name=Lockman>{{ cite journal |vauthors=Lockman FJ, ...itle=Maps of dust infrared emission for use in estimation of reddening and cosmic microwave background radiation foregrounds |journal=Astrophys. J. |date=Jun ...

{{Short description|Series of cosmic microwave background experiments at the South Pole}} ...k Array''' are a series of [[cosmic microwave background]] (CMB) [[List of cosmic microwave background experiments|experiments]]. They aim to measure the [[P ...

...le universe]] is a shade of yellowish-white that has been given the name [[Cosmic Latte]]. ...nearly polarized]] by scattering from elongated [[Cosmic dust|interstellar dust]] grains whose long axes tend to be oriented perpendicular to the galactic ...

..."/><ref name="Zhang"/> Absorption and re-radiation of the starlight by the dust makes the object far brighter in the infrared than it is in visible light.< ''[[Hubble Space Telescope|HST]]'' images show that the dust component of the innermost region of CIT 6's CSE has developed the bipolar ...

...> Hence, [[Neutrino decoupling#Indirect evidence from phase changes to the Cosmic Microwave Background (CMB)]] theorises that the decoupled neutrinos should == Cosmic Background Radiation Polarization == ...

...l= https://www.quantamagazine.org/the-case-for-spectral-distortions-in-the-cosmic-microwave-background-20150630/ |magazine= Quanta|publisher= Simons Foundati ...th>). The spectral distortions also interplay with distinguished epochs of cosmic history such as [[reionization]], [[Recombination (cosmology)|recombination ...

...f their measured data. Comet or meteoroid streams, and even [[interstellar dust]] were identified in the data. ...o determine the three-dimensional spatial distribution of [[interplanetary dust]].<ref>{{cite journal |last1=Leinert |first1=Ch. |last2=Link |first2=H. |la ...

...after the [[Big Bang]] and from more recent epochs. Observations of the [[cosmic microwave background]] and [[Big Bang nucleosynthesis]] studies have set co ...isotropies) in the [[cosmic microwave background]] (CMB), especially the [[Cosmic microwave background#Data reduction and analysis|second peak of the CMB pow ...

..., "The super-massive black hole itself is dark but it has a disc of gas or dust around it that has become so hot that it will outshine an entire galaxy of ...process, which marked the end of the [[Timeline of the Big Bang#Dark Ages|cosmic Dark Ages]], so observing a quasar from before the transition is of major i ...

...shaped [[accretion disk]] of [[matter]] composed of [[gas]], [[Cosmic dust|dust]], [[planetesimal]]s, [[asteroid]]s, or collision fragments in [[orbit]] ar ...otating star. The former is a rotating circumstellar disc of dense gas and dust that continues to feed the central star. It may contain a few percent of th ...

If one considers a pressure-free [[perfect fluid]] (also known as a [[dust solution]]), the effective material Lagrangian becomes <math>\mathcal{L}_m ...2014119>{{cite journal|author=Minazzoli O. |date=July 2014 |title= On the cosmic convergence mechanism of the massless dilaton|journal=Physics Letters B |vo ...

{{Short description|Space dust measurements}}[[File:LunarMicrocraters.jpg|thumb|Small glassy lunar sample ...icles to spacecraft and other space-borne assets. The measurement of space dust requires the use of advanced scientific techniques such as [[secondary ion ...

...= P. G. | title = The search for protostars using millimetre/submillimeter dust emission as a tracer | journal = Planetary Systems: Formation, Evolution an ...cloud by radiation pressure from the star, and will remain mixed with the dust.<ref>{{Cite journal | last = Morrison | first = D. | title = Sizes and albe ...

...e]] and is heavily obscured by the Milky Way's [[star]]s and [[cosmic dust|dust]]. If it were not obscured, it would be one of the largest (about {{frac|3| ...

...he fractional abundances of cyanopolyyne are less affected by changes in [[cosmic ray|radiation field]] intensity past time 1&nbsp;million years because the ...ast1=Van Dishoeck|first1=E. F.|date=2004|title=ISO spectroscopy of gas and dust: From molecular clouds to protoplanetary disks|journal=Annual Review of Ast ...

...h we can see; the [[star]]s, [[interstellar medium|gas]] and [[cosmic dust|dust]] that makes up [[galaxy|galaxies]] and [[galaxy cluster]]s. ...

...astern Meeting], p. 6. Retrieved on 2010-01-26.</ref><ref>E.J. Applewhite, Cosmic Fishing: An Account of Writing Synergetics With Buckminster Fuller. Macmill ...nstream endorsements such as the prologue by [[Arthur Loeb]], and positive dust cover blurbs by [[U Thant]] and [[Arthur C. Clarke]], along with the posthu ...