Skip to content
  • For Scientists arrow_outward
NSF Logo Icon
NRAO Logo
  • News
  • Gallery
  • Telescopes
    • VLA
    • ALMA
    • VLBA
    • GBT
    • ngVLA
  • Tech
    • CDL
    • Spectrum Management
    • ngRADAR
    • VLASS
  • Visit Us
    • Visit VLA
    • Visit ALMA
    • Visit GBO
  • Learn
    • What is Radio Astronomy?
    • Black Holes
    • Exoplanets
    • Pulsars Astronomy
    • Eclipse Basics
    • Blogs
    • Outreach Programs & Events
  • Explore
    • Cosmic Coloring Compositor
    • Interferometry Explained
    • NRAO Mission Control
  • Join & Give

physics

Select : asteroid collisionasteroidsastronomical distance scalesatomsbig bangblack holesbright lights in the skybrown dwarfcareerscelestial eventschecker cabscometsconstellationscosmic distancescosmic microwave backgroundcosmic rayscosmologydark energydark matterdwarf planeteartheclipseeclipticeducationexoplanetsexpansion of the universegalaxiesgeneral relativitygravitational lensgravity wavesGreat Red SpotHoaxesHubble Space Telescope (HST)Interferometerinterferometryinterstellar moleculesionosphereJupitermagnetarsmarsmeteorsMH370milky wayMilky Way Galaxymoleculesmoonmoonsneutron starneutron starsNibirunight skyparallaxphysicsplanetsplutoproperties of lightPtolemypulsarsquasarsradar astronomyRadio Astronomyradio frequency interferenceradio interferometersradio recombination line emissionRadio TelescopeSatellite DishSchwarzschild Radiusscientific methodsearch for extraterrestrial intelligenceSETIsolar systemspace probesspacecraftstar formationstarssunsupernovasupernova remnantssupernovaetelescopestime dilationTrans Neptunian Objectstwin paradoxunexplained celestial observationsVenusVery Large ArrayVery Long Baseline Array (VLBA)Voyager 1weather

A Question Regarding Atmospheric Transparency Windows

The link you provided appears to no longer be active.  A more general discussion regarding astronomical observations from ground-based…

What was the Intensity of the Cosmic Background Radiation Just After Recombination?

Since the cosmic microwave background emits as a black body, we start with the spectral radiance of a black…

Why Don’t All Objects in the Milky Way Rotate Around the Black Hole at the Center of our Galaxy?

The gravitational force has a distance dependence to it that makes it decrease as you get further away from…

How Can We See Stars in the Night Sky When They Are So Far Away?

Even though the stars that we see in the night sky are all very far away, we can see…

How to Calculate the Orbital Period of a Comet Given its Closest and Furthest Orbital Distance

Given the minimum and maximum distance of the orbit of a comet in an elliptical orbit, you can use…

Is the Speed of Light Changed by Gravity?

The short answer is no, the speed of light that you measure locally is unchanged by gravity.  In Einstein’s…

Posts navigation

  • « Previous
  • 1
  • …
  • 14
  • 15
  • 16
  • 17
  • 18
  • 19
  • 20
  • …
  • 34
  • Next »

Connect with NRAO

mail
Tweets by TheNRAO
The National Radio Astronomy Observatory is a facility of the U.S. National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Founded in 1956, the NRAO provides state-of-the-art radio telescope facilities for use by the international scientific community. NRAO telescopes are open to all astronomers regardless of institutional or national affiliation. Observing time on NRAO telescopes is available on a competitive basis to qualified scientists after evaluation of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time. NRAO also provides both formal and informal programs in education and public outreach for teachers, students, the general public, and the media.
The U.S. National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 "to promote the progress of science; to advance the national health, prosperity, and welfare; to secure the national defense..."
AUI collaborates with the scientific community and research sponsors to plan, build, and operate cutting-edge facilities. We cultivate excellence, deliver value, enhance education, and engage the public.
  • News
  • Gallery
  • Telescopes
    • VLA
    • ALMA
    • VLBA
    • GBT
    • ngVLA
  • Tech
    • CDL
    • Spectrum Management
    • ngRADAR
    • VLASS
  • Visit Us
    • Visit VLA
    • Visit ALMA
    • Visit GBO
  • Learn
    • What is Radio Astronomy?
    • Black Holes
    • Exoplanets
    • Pulsars Astronomy
    • Eclipse Basics
    • Blogs
    • Outreach Programs & Events
  • Explore
    • Cosmic Coloring Compositor
    • Interferometry Explained
    • NRAO Mission Control
  • Join & Give
  • For Scientists
  • About NRAO
  • Ask an Astronomer
  • Historical Archives
  • Media Use
  • Social Media Policy
  • NRAO Library
  • Central Development Lab
  • Technology Transfer
  • Employee Services
  • Visitor Code of Conduct
  • Careers

Contact Us

NRAO Headquarters
520 Edgemont Road
Charlottesville, VA 22903
434-296-0211
More Information Here

© 2025 The National Radio Astronomy Observatory