AstrotalkUK

Not for profit website/blog on astronomy, space and my writing

  • Home
    • FAQ
    • Contact
    • About
    • Privacy Policy
  • Content
    • Podcast
    • All episodes
    • Book Review
    • Cyber Security
  • Events

Episode 112 – Brown Dwarfs, Dark Matter and Dark Energy

By Gurbir Dated: March 15, 2024 Leave a Comment

This episode was recorded in Tenerife with Professor Eduardo L Martín who is based at the Instituto de Astrofísica de Canarias. He is working on the European Space Agency’s mission, Euclid.

In time Euclid will shed light on both dark matter and dark energy. It was launched in July 2023 and arrived in its L2 orbit a month later. It has just two instruments which will produce a high-resolution 3-D map of a third of the sky, stretching back 10 billion years during its initial 6-year operational lifetime.

Professor Martín is not part of the Euclid Consortium the around 2500 scientists and engineers from more than a dozen countries who operate the Euclid Mission. He is one of the two Euclid mission Independent Legacy Scientists. Professor Martín is a specialist in substellar bodies, that is celestial bodies with a size about that of Jupiter but with around 50 times its mass. When initially theorised in the 1960s they were called Black Dwarfs but renamed in the 1970s by Jill Tarter as Brown Dwarfs.

Brown Dwarfs generate energy only through gravitational compression, not nuclear fusion. There is an overlap in surface temperature between young brown dwarfs and old very low-mass stars. Martín and his collaborators have developed spectroscopic methods to distinguish brown dwarfs from stars, in particular the Lithium test. More about this interesting role of Lithium in cosmology in Professor Martín’s book published in 2023 by the Institute of Physics, entitled “Lithium Across the Universe“. You can download several free-to-read chapters – here.

Brown Dwarfs emit mostly in the infrared not optical light as our sun. One of the two instruments on Euclid operates in the infrared and can detect these “dark ultracold objects of substellar mass“. Does Professor Martin think Euclid will find Brown Dwarfs? He told me in this recording, “that is what I put in the proposal so we had better do now”. He is supported by a postdoc Marusa Zerjal and a student Diego Martin, funded by the European Research Council.

The first images were released in November 2023. The spacecraft and its instruments are operating well and sending data. More about the Euclid mission, images released so far and a summary of the attributes of Normal Matter, Dark Matter and Dark Energy below.

Episode112 ESA’s Euclid Mission with Professor Eduardo Martin

Perhaps the most pressing question for astrophysicists is what is the cosmos made of. They have known for a long time that visible matter accounts only for the 5%, Dark Matter, 27% and Dark Energy 68%. Currently, most of the attributes of Dark Matter and Dark Energy remain a mystery. Helping to shed some answers to these questions is Euclid’s primary goal.

The visible matter is something we are surrounded by. It responds to all 4 known forces, electromagnetic, gravitation, and the strong and weak nuclear force. Dark matter is not dark, it’s invisible and is only detected through its gravitational influence on the matter we can see. Gravitational lensing is one manifestation.

Whereas gravity is a force of attraction, Dark Energy is repulsive, powering the expansion of the Universe. Its effects are observed by monitoring type 1a supernovae in distant galaxies. Some scientists consider Dark Energy as the Cosmological Constant that Einstein initially added and then removed from his General Theory of Relativity. The Cosmological Constant is now considered by some as the 5th fundamental force, after gravity, electromagnetism, and strong and weak nuclear forces.

  • Horse head Nebula. Credit ESA
  • Globular Cluster NGC6397. Credit ESA
  • Irregular Galaxy NGC6822. Credit ESA
  • Spiral galaxy IC342. Credit ESA Credit ESA
  • Perseus Cluster. Credit ESA

Summary of attributes for Normal Matter, Dark Matter and Dark Energy

AttributeNormal MatterDark MatterDark Energy
Formation TimeShortly after the Big BangLikely formed shortly after the Big BangBelieved to have originated with the expansion of the universe
LocationEverything we can see including Galaxies, stars, planets and the interstellar mediumPrimarily in galactic halos, halos around galactic clusters and permeates the universeHomogeneously distributed throughout space, associated with vacuum energy
Observational EvidenceEmission and absorption spectra, visible light, X-rays, cosmic microwave backgroundGravitational effects on visible matter, galaxy rotation curves; Dark matter inferred from galaxy cluster dynamics by Fritz Zwicky, 1933). Galaxy rotation curves suggest dark matter and the work of Vera Rubin from the 1970s.
Observation of gravitational lensing.
Acceleration of cosmic expansion, distant Type 1a supernova observations by Saul Perlmutter, Brian Schmidt, Adam Riess (1998-1999).
In time, it may turn out to be the 5th fundamental force.
Interaction with Electromagnetic ForceStrong interaction, contributes to various spectra and emissionsWeak or non-existent interactions with light and other EM wavesWeak or non-existent interactions with light and other EM waves
Interaction with Gravitational ForceExperiences gravitational attraction with other matterExperiences gravitational attraction, influencing cosmic structures. Exhibits a repulsive gravitational effect, driving cosmic expansion
Percentage Composition in the Universe~4.6% of the total mass-energy content~26.5% of the total mass-energy content~68.9% of the total mass-energy content
https://media.blubrry.com/astrotalkuk_podcast_feed/astrotalkuk.org/wp-content/uploads/2024/03/Episode112_EuclidMission.mp3

Podcast: Play in new window | Download (Duration: 48:53 — 89.5MB) | Embed

Subscribe: Spotify | RSS | More

Share this:

  • Click to share on X (Opens in new window) X
  • Click to share on LinkedIn (Opens in new window) LinkedIn
  • Click to share on Facebook (Opens in new window) Facebook

Episode 107 – SETI’s new tool – Technosignatures

By Gurbir Dated: November 18, 2022 Leave a Comment

Episode 107 – Dr Hector Socas-Navarro

The Great Wall of China can be seen from space. Actually, it can’t but the idea that a civilisation could build something large on a planetary scale that could be detected from interstellar distances was articulated first by author Olaf Stapledon in 1937 and popularised by Freeman Dyson in the 1960s. Known today as a Dyson Sphere, it is a megastructure built by an alien intelligence that captures almost all the energy emitted by its star. In this episode, Dr Hector Socas-Navarro explains we humans are not there yet but the increasing density of the Earth’s geosynchronous orbit will become detectable in a couple of centuries.

So not yet a Dyson sphere but a ring or a belt, he calls the Clarke-Exobelt may allow alien civilisations to detect humanity’s presence over interstellar distances. In this episode, we discuss the opportunities for SETI to detect artificial structures like this at interstellar distances using the JWST and very large Earth-based telescopes coming online soon.

Links to the resources we discuss are on the episode webpage

Podcast – Museum of Science and the Cosmos of Tenerife
NASA Technosignatures: “Moderately advanced” technologies in transit. Youtube video
Instituto de Astrofísica de Canarias
Museum of Tenerife

Scientific papers

  • Concepts for future missions to search for technosignatures
  • Possible Photometric Signatures of Moderately Advanced Civilizations: The Clarke Exobelt
  • Further support and a candidate location for Planet 9

https://media.blubrry.com/astrotalkuk_podcast_feed/astrotalkuk.org/wp-content/uploads/2022/11/Episode107_Hector.mp3

Podcast: Play in new window | Download (Duration: 40:25 — 92.5MB) | Embed

Subscribe: Spotify | RSS | More

Share this:

  • Click to share on X (Opens in new window) X
  • Click to share on LinkedIn (Opens in new window) LinkedIn
  • Click to share on Facebook (Opens in new window) Facebook

Episode 106 – ESA’s new science missions

By Gurbir Dated: November 11, 2022 Leave a Comment

Pau McNamara

European Space Agency’s Dr Paul McNamara was studying low-frequency gravitational waves just before they were discovered in 2015. Now he is the astronomy and astrophysics coordinator for the European Space Agency. In this interview, recorded in Athens during Cospar2022, he speaks about some of the exciting science missions that ESA will be launching later this decade.

These missions include

  • Juice – JUpiter ICy moons Explorer
  • Euclid – To explore dark matter and dark energy
  • Plato – The next-generation planet-hunting mission
  • Ariel – A UK-led mission to explore the atmospheres of exoplanets

He also talks about ESA’s publicly available resources especially useful to science educators. Planetary Science Archive and ESA Sky. They are available to anyone, in or outside Europe and without charge. Links are available on this episode’s web page.


Dr Paul McNamara

https://media.blubrry.com/astrotalkuk_podcast_feed/astrotalkuk.org/wp-content/uploads/2022/11/Episode106.mp3

Podcast: Play in new window | Download (Duration: 43:00 — 98.4MB) | Embed

Subscribe: Spotify | RSS | More

Share this:

  • Click to share on X (Opens in new window) X
  • Click to share on LinkedIn (Opens in new window) LinkedIn
  • Click to share on Facebook (Opens in new window) Facebook

Episode 100 Sandra Benitez Herrera – ESA Education Outreach

By Gurbir Dated: September 18, 2022 Leave a Comment

Astrophysicist Sandra Benitez-Herrera  talks about the opportunities for teachers and students made available by the European Space Agency‘s CESAR (Cooperation through Education in Science and Astronomy Research) program. This episode was recorded in Athens in July during Cospar 2022.

If you are a student or a teacher in Europe or beyond, Sandra explains how you make use of CESAR’s resources – optical, solar and radio telescopes, online seminars, face-to-face training and an enormous quantity of space data from ESA and other space agencies. All in one place and with no charge. She starts with an explanation of what CESAR is – in audio and Youtube video below.


https://media.blubrry.com/astrotalkuk_podcast_feed/astrotalkuk.org/wp-content/uploads/2022/09/Episode100_Sandra_HB.mp3

Podcast: Play in new window | Download (Duration: 27:08 — 31.2MB) | Embed

Subscribe: Spotify | RSS | More

Share this:

  • Click to share on X (Opens in new window) X
  • Click to share on LinkedIn (Opens in new window) LinkedIn
  • Click to share on Facebook (Opens in new window) Facebook
Next Page »

Find me online here

  • E-mail
  • Facebook
  • LinkedIn
  • Twitter
  • Vimeo
  • YouTube

subscribe to mailing list and newsletter

  • This field is for validation purposes and should be left unchanged.

Browse by category

Recent Comments

  • Frank Pleszak on Episode 117 – Early Aviation in Manchester
  • Gurbir Singh on Episode 111 – Chandrayaan-3
  • Lunar Polar Exploration Mission: Difference between revisions – भोजपुरी on Episode 82: Jaxa and International Collaboration with Professor Fujimoto Masaki
  • Gurbir on Public Event. Anglo Indian Stephen Smith – India’s forgotten Rocketeer
  • Sandip Kumar Chakrabarti on Public Event. Anglo Indian Stephen Smith – India’s forgotten Rocketeer

Archives

Select posts by topic

apollo astrobiology Astrophotography BIS Book Review Carl Sagan CCD CCSK China Cloud Computing cnsa commercial Cosmology curiosity Education ESA Gagarin History India Infosec ISRO jaxa Jodrell Bank Mars Media Moon NASA podcast radio astronomy Rakesh Sharma rocket Rockets Roscosmos Science Science Fiction seti Solar System soviet space space spaceflight titan USSR video Vostok Yuri Gagarin

Copyright © 2008–2025 Gurbir Singh - AstrotalkUK Publications Log in