Episodi

  • Nobel Prize 2026: The Science Gets Stranger
    Oct 16 2026

    Can light restore aspects of sight? Can recalling a cold experience change an animal's metabolism? And what can ghost particles and mirror-image molecules tell us about the universe?

    Lester Nare and Krishna Choudhary follow up on our 2026 Nobel Prize episodes with research building on optogenetics, IceCube and molecular handedness. We unpack an early human vision-restoration trial, cold-memory experiments in mice, cosmic neutrino flavors, and a tiny electrical sensor for distinguishing left- and right-handed amino acids.

    Plus: how the Nobels work, our follow-up on the Nobel chemistry illustration, a brief look at neutrino Earth tomography, and why fundamental research matters. Which discovery would you like us to explore next?

    CHAPTERS
    00:00 Cold open: memory, neutrinos and mirror molecules
    00:28 Hello Internet and how the Nobels work
    04:32 Optogenetics recap
    10:23 Restoring aspects of vision
    25:43 Controlling movement in worms
    29:31 Cold memories and metabolism
    41:07 Memory, trauma and ethical questions
    45:44 FFP housekeeping
    48:17 IceCube recap
    56:23 Measuring cosmic neutrino flavors
    1:10:30 A brief look at neutrino Earth tomography
    1:12:20 Why fundamental physics matters
    1:26:58 Chemistry and molecular handedness
    1:29:08 Correcting the Nobel illustration
    1:39:30 Measuring chirality in tiny samples
    1:46:42 Testing the sensor on meteorite and desert samples
    1:51:22 Why these questions matter
    1:57:20 Closing thoughts and signoff

    RESEARCH & FURTHER READING
    Optogenetic therapy for visual function (NEJM, 2026):
    https://doi.org/10.1056/NEJMoa2602215

    Cold memories and thermoregulation (Nature, 2025):
    https://doi.org/10.1038/s41586-025-08902-6

    Three-flavor composition of cosmic neutrinos (PRL, 2026):
    https://doi.org/10.1103/vntd-m133

    Chiral discrimination in meteorite and desert soil extracts (Nature Communications, 2026):
    https://doi.org/10.1038/s41467-026-77947-6

    Further reading, briefly mentioned: neutrino Earth tomography (preprint):
    https://arxiv.org/abs/2607.02644

    EDITORIAL NOTES
    The vision trial was small and exploratory. The cold-memory findings discussed are from mice.

    On-screen clarifications:
    16:53 Both eyes were profoundly visually impaired; the worse-seeing eye was treated.
    19:57 The untreated eye was patched during testing, not a normal-vision control.
    54:41 Neutrino event rates depend on energy and selection, not just detector volume.
    1:05:47 Flavor identification efficiency is distinct from interaction probability; both depend on energy.
    1:13:35 Other astronomy-related Nobels include 2017 (LIGO) and 2019 (cosmology/exoplanets).
    1:18:00 The LHC at CERN enabled the Higgs discovery; CERN itself was founded in 1954.
    1:44:25 Both enantiomers produce current signals; waveform features distinguish them.
    1:46:42 Murchison is a meteorite. Diego de Almagro and North of Antofagasta are soil sites.
    1:47:40 The sensor study reports mixed agreement and limitations, not uniformly negative results.
    1:49:00 Phobos is a Martian moon; a captured-asteroid origin is a hypothesis.

    WATCH & LISTEN
    Full video: https://youtu.be/C9K6onZxyN4
    Episode notes: https://ffppod.com/episodes/ep64
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    Breaking down science news so it makes sense to curious people everywhere.

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    1 ora e 59 min
  • Nobel Prize in Chemistry 2026 Explained: Mirror Molecules (EP 63)
    Oct 7 2026

    Why does life favor one molecular mirror image? The 2026 Nobel Prize in Chemistry honors Henri B. Kagan and Kenso Soai for nonlinear effects and autocatalysis in asymmetric organic synthesis.

    Lester Nare and Krishna Choudhary unpack the science from first principles: chirality, Pasteur's crystals, enantiomeric excess, and how a tiny imbalance can grow into an overwhelming preference for one molecular hand.

    We connect Kagan's catalyst discoveries and the Soai reaction to medicines, the origins of biological handedness, and the serious concerns around hypothetical mirror life. Plus: symmetry in physics, Frances Oldham Kelsey and thalidomide, and our interpretation of a Nobel illustration.

    CHAPTERS
    00:00 Why life has a molecular handedness
    01:33 Hello Internet
    02:49 The 2026 Chemistry laureates
    06:24 Chirality and mirror-image molecules
    12:10 Pasteur and the history of handedness
    19:36 Why is life's chemistry one-handed?
    24:35 Frank and the origin-of-life puzzle
    29:14 Enantiomeric excess explained
    30:30 Kagan and nonlinear effects
    38:58 FFP and symmetry in physics
    42:20 Soai and asymmetric autocatalysis
    51:28 Why chirality matters for medicine
    58:21 What this does and does not explain about life
    1:00:25 Mirror life and biological risk
    1:10:37 Examining the Nobel illustration
    1:14:10 Recap and Nobel week reflections

    RESEARCH & FURTHER READING
    Original papers and supporting context:
    Frank's model (1953): https://doi.org/10.1016/0006-3002(53)90082-1
    Puchot, Kagan et al. (1986): https://doi.org/10.1021/ja00269a036
    Soai et al. (1995): https://doi.org/10.1038/378767a0
    Sato et al., amplification (2003): https://doi.org/10.1002/anie.200390105
    Mirror-life risks (2024): https://doi.org/10.1126/science.ads9158
    Nobel announcement: https://www.nobelprize.org/prizes/chemistry/2026/press-release/

    EDITORIAL NOTES
    Intro: the 50:50 example describes an unbiased synthesis, not all chemistry. The Soai reaction is a clue to amplification, not proof of how life began.

    On-screen clarifications:
    04:38 B-DNA is right-handed; Z-DNA can form a left-handed helix.
    13:56 Pasteur separated sodium ammonium tartrate crystals.
    18:48 L/D configuration does not specify optical rotation.
    19:10 Proteins mainly use L-amino acids; DNA/RNA use D-sugars.
    22:55 Mentos mainly triggers CO2 bubble nucleation.
    27:18 Asymmetric catalysis and autocatalysis are distinct.
    34:07 0.25 × 0.25 = 0.0625 = 6.25%.
    36:31 Inactive mixed catalyst pairs are a simplified model.
    37:55 The normalized product-ratio curve need not be parabolic.
    42:04 Wu: preferential emission opposite spin; antineutrinos also emitted.
    45:30 5-pyrimidyl alkanol; an alkanol is an alcohol.
    47:10 The tiny-imbalance result is Sato et al. (2003), cited above.
    47:40 A demonstration of symmetry breaking by asymmetric autocatalysis.
    49:09 Above 99.5% ee means above 99.75% majority form, not exactly 100%.
    49:57 0.00005% excess is 1 part in 2,000,000.
    52:44 Thalidomide enantiomers interconvert in the body.
    53:36 Merrell applied in the U.S.; Kelsey withheld approval. Trial exposure occurred.
    1:02:09 Mirror-life catastrophe is a serious risk, not an observed outcome.
    1:03:28 Antibodies are adaptive immunity, not innate immunity.
    1:03:53 Impaired recognition does not mean proven total immune invisibility.
    1:04:27 Some treatments might work; ecosystem protection is very difficult.
    1:04:56 No reproducing mirror organism has been reported.
    1:09:19 Chimeras and genetic modification are not interchangeable.
    1:10:37 The Nobel-diagram critique is our interpretation, not an official correction.
    1:11:51 Solid wedge: toward; hashed wedge: away; ordinary line: neither.

    WATCH & FOLLOW
    Full video: https://youtu.be/Wdapv1hFT4w
    Episode notes: https://ffppod.com/episodes/ep63
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    Breaking down science news so it makes sense to curious people everywhere.

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    1 ora e 21 min
  • Nobel Prize in Physics 2026 Explained: IceCube & Neutrinos
    Oct 6 2026
    Why build a telescope inside a billion tons of Antarctic ice? The 2026 Nobel Prize in Physics recognizes Francis Halzen's work on IceCube and the discovery of high-energy neutrinos from the cosmos.In Episode 62 of From First Principles, Lester Nare and Krishna Choudhary explain neutrinos from the ground up: why these elusive particles make powerful cosmic messengers, how faint flashes of Cherenkov light reveal their interactions, and why detecting them requires an observatory buried deep beneath the South Pole.We follow the path from beta decay and the first neutrino experiments to AMANDA, IceCube's construction, the 2013 astrophysical breakthrough, a distant blazar, and a neutrino map of the Milky Way. Along the way: cosmic rays, the Oh-My-God particle, tracks versus cascades, and the international collaboration behind the discovery.CHAPTERS00:00 Hunting ghost particles beneath Antarctica01:16 Hello Internet and Nobel Prize05:30 What are neutrinos?10:00 Neutrinos as cosmic messengers15:02 The Oh-My-God particle16:21 Cosmic-ray energies19:07 Cosmic particle accelerators22:28 Why look for neutrinos?25:52 How to detect a neutrino29:23 Cherenkov light33:13 Building a neutrino observatory37:17 From Antarctic ice to AMANDA42:21 Building IceCube44:59 Reading tracks and cascades49:30 Backgrounds and the 2013 discovery52:46 Tracing cosmic neutrino sources54:16 Mapping the Milky Way58:23 IceCube collaboration and Gen21:01:05 Closing and Nobel weekRESEARCH & FURTHER READINGAMANDA in Antarctic ice (2001): https://doi.org/10.1038/35068509IceCube detector and instrumentation (2017): https://doi.org/10.1088/1748-0221/12/03/P03012First PeV neutrinos (2013): https://doi.org/10.1103/PhysRevLett.111.021103Astrophysical neutrino evidence (2013): https://doi.org/10.1126/science.1242856Blazar TXS 0506+056 (2018): https://doi.org/10.1126/science.aat1378Archival blazar neutrino emission (2018): https://doi.org/10.1126/science.aat2890Milky Way neutrino map (2023): https://doi.org/10.1126/science.adc9818Gamma-ray burst constraints (2012): https://doi.org/10.1038/nature11068IceCube overview: https://icecube.wisc.edu/science/icecube/EDITORIAL NOTESIntro: the 2013 breakthrough was high-energy astrophysical neutrinos. Lower-energy supernova neutrinos were detected in 1987.On-screen clarifications:06:45 Beta-minus decay produces a proton, electron and electron antineutrino.11:10 Davis studied solar neutrinos; Koshiba's team detected SN 1987A neutrinos.17:50 The cosmic-ray knee and ankle are not fixed distance boundaries.19:38 Required accelerator size depends on magnetic-field strength.24:18 Ground-based telescopes also detect gamma rays through air showers.27:48 W interactions produce charged leptons; Z scattering preserves neutrino flavor.34:06 The underwater concept dates to 1960; DUMAND developed in the 1970s.36:09 Baikal holds about one-fifth of unfrozen surface freshwater.38:53 Earth filters muons but also absorbs many very-high-energy neutrinos.41:26 Pressure converts air bubbles into clathrates, reducing light scattering.42:28 Construction finished in December 2010; full operations began in May 2011.44:27 Sensors are DOMs; DeepCore is a densely instrumented detector region.45:47 Timing gives direction; light yield and pattern help estimate energy.49:44 Upgoing events can still be atmospheric neutrinos.53:12 TXS 0506+056 is about 3.7 billion light-years away.56:38 Long GRBs often involve collapsing stars; short GRBs often involve mergers.WATCH & FOLLOWFull video: https://youtu.be/eMahxeBj5k0Episode notes: https://ffppod.com/episodes/ep62Medicine Nobel explained: https://youtu.be/PKAYqhy8xf8Follow @FFPPod on Instagram, TikTok, X and Facebook.From First Principles: Breaking down science news so it makes sense to curious people everywhere.
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    1 ora e 2 min
  • Nobel Prize in Medicine 2026 Explained: Optogenetics (EP 61)
    Oct 5 2026

    How do you prove what a brain cell actually does? The 2026 Nobel Prize in Medicine celebrates a remarkable answer: give cells a light-sensitive protein, then switch their activity on or off with light.


    In Episode 61 of From First Principles, Lester Nare and Krishna Choudhary explain optogenetics from the ground up and trace the discoveries of Peter Hegemann, Georg Nagel and Karl Deisseroth. We follow the story from algae swimming toward light to channelrhodopsins, precisely controlled neurons, and experiments probing memory, reward and behavior. Then we explore heart-brain connections, early attempts to restore vision, and what these experiments can and cannot tell us.


    CHAPTERS

    00:00 The discovery that put brain cells under light control

    02:34 Hello Internet

    03:28 2026 Medicine Nobel and optogenetics

    05:38 Understanding the brain

    08:42 From correlation to causation

    18:13 Controlling neurons with light

    21:25 Early optogenetics and the chARGe system

    24:17 Light-sensitive microbial proteins

    26:26 Algae and phototaxis

    31:42 Discovering channelrhodopsins

    34:42 Nagel and light-gated ion channels

    40:55 Controlling mammalian neurons

    50:19 Expanding the optogenetic toolkit

    56:10 Neural circuits and behavior

    59:02 Memory, reward and reinforcement

    1:02:53 Heart rhythm and emotion

    1:04:02 Beyond the brain and toward medical treatments

    1:06:56 Implications and limits

    1:09:10 Closing and Nobel week


    RESEARCH & FURTHER READING

    Full paper list: https://ffppod.com/episodes/ep61

    Nobel Prize announcement and background:

    https://www.nobelprize.org/prizes/medicine/2026/summary/

    Optical control of neurons: https://doi.org/10.1038/nn1525

    Memory recall in mice: https://doi.org/10.1038/nature11028

    Partial visual recovery: https://doi.org/10.1038/s41591-021-01351-4


    EDITORIAL NOTES

    On-screen clarifications are included at these timestamps:

    13:46 The Jennifer Aniston neuron was recorded in human patients. Selective firing alone did not establish that it causes recognition.

    30:34 Vertebrate rhodopsin is a GPCR. In rods and cones, light closes cGMP-gated channels and causes hyperpolarization.

    35:12 Xenopus oocytes are immature frog egg cells, not embryos.

    39:52 Calcium entry triggers neurotransmitter release; neurotransmitters carry the signal across the synapse. ChR2 conducts several positive ions, not just calcium.

    52:17 Halorhodopsin is a light-driven chloride pump, not a channel.

    1:03:18 The heart-pacing study expressed ChRmine in mouse heart muscle cells, not neurons.

    Animal studies and early clinical results are distinguished from established treatments.


    WATCH & LISTEN

    Watch this episode: https://youtu.be/PKAYqhy8xf8

    Our Nobel predictions: https://open.spotify.com/episode/4xuoH7WhM5svq8vEJPL3Ce

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    Breaking down science news so it makes sense to curious people everywhere.

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    1 ora e 11 min
  • 2026 Nobel Prize Predictions: Medicine, Physics & Chemistry (EP 60)
    Oct 3 2026

    Who could win the 2026 Nobel Prizes? From the science behind Ozempic to quantum interference and droplets inside living cells, Lester Nare and Krishna Choudhary make their picks for Medicine, Physics and Chemistry, and explain the discoveries behind them.


    In Episode 60 of From First Principles, we explore seven research areas with a case for Nobel recognition: GLP-1, optogenetics, optical coherence tomography, the Aharonov–Bohm effect, atomic force microscopy, biomolecular condensates and Buchwald–Hartwig coupling. We also discuss Michael Berry’s geometric phase and the awkward question of how a prize limited to three people recognizes discoveries built by larger teams.


    These are our predictions, recorded before the 2026 announcements. Medicine, Physics and Chemistry will be announced October 5–7. Which discovery, and which researchers, would you pick? Tell us in the comments, then join us for our Nobel week breakdowns.


    CHAPTERS

    00:00 The science that could win a Nobel Prize

    00:57 Hello Internet: our 2026 predictions

    02:03 Medicine: GLP-1 and the science behind Ozempic

    07:41 Medicine: optogenetics and controlling neurons with light

    13:16 Medicine: optical coherence tomography

    16:28 Golden Goose Awards and FFP updates

    18:39 Physics: the Aharonov–Bohm effect and geometric phase

    27:37 Physics: atomic force microscopy

    32:04 Chemistry: biomolecular condensates

    36:36 Chemistry: Buchwald–Hartwig coupling

    38:42 Your predictions and our Nobel week plans


    RESEARCH & FURTHER READING

    Foundational papers and background for the discoveries discussed:


    GLP-1: Mojsov, Weir & Habener (1987)

    https://doi.org/10.1172/JCI112855

    Optogenetics: Boyden et al. (2005)

    https://doi.org/10.1038/nn1525

    Optical coherence tomography: Huang et al. (1991)

    https://doi.org/10.1126/science.1957169

    Aharonov–Bohm effect (1959)

    https://doi.org/10.1103/PhysRev.115.485

    Berry’s geometric phase (1984)

    https://doi.org/10.1098/rspa.1984.0023

    Atomic force microscopy: Binnig, Quate & Gerber (1986)

    https://doi.org/10.1103/PhysRevLett.56.930

    Biomolecular condensates: Brangwynne et al. (2009); Li et al. (2012)

    https://doi.org/10.1126/science.1172046

    https://doi.org/10.1038/nature10879

    Buchwald–Hartwig coupling: Paul et al. (1994); Guram et al. (1995)

    https://doi.org/10.1021/ja00092a058

    https://doi.org/10.1002/anie.199513481


    Official Nobel announcement schedule:

    https://www.nobelprize.org/prizes/about/prize-announcement-dates/


    EDITORIAL NOTES

    19:30 David Bohm later held a professorship at Birkbeck, University of London (1961–1987); he did not spend the rest of his career in Brazil.

    33:23 The ribosome-producing compartment discussed is the nucleolus, not the nucleosome. These corrections also appear on screen.


    WATCH & EXPLORE

    YouTube: https://youtu.be/MgOpbh5VUGE

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    Breaking down science news so it makes sense to curious people everywhere.

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    41 min
  • Golden Goose Awards 2026: The Science Behind the Winners (Part 1) (EP 59)
    Sep 29 2026

    What connects a noise complaint, holiday lights seen from space, and the physics of a coffee stain? Three unexpected paths from basic research to discoveries with real-world impact.


    Krishna Choudhary and Lester Nare explore the science behind the 2026 Golden Goose Awards: Zhen Xu's work on histotripsy, NASA's Black Marble nighttime satellite data, and Sidney Nagel's discoveries in soft matter physics.


    We start with focused ultrasound and the tiny bubbles that can break apart targeted tissue, tracing the journey from early laboratory experiments to clinical research on liver tumors. Then we look at how Earth's nighttime lights reveal power outages, disaster recovery, and changing human activity. Finally, falling drops, coffee stains, and jammed grains open up a world of robotic grippers and materials that can be trained and retrained.


    The thread connecting all three stories is the unexpected value of federally funded basic research. Part 2 will feature conversations with the award-winning researchers and AAAS CEO Sudip Parikh.


    CHAPTERS

    00:00 Golden Goose Awards trailer

    01:19 Introducing our Golden Goose special

    02:42 Zhen Xu: From a noise complaint to histotripsy

    05:57 The early ultrasound experiments

    13:42 Controlling cavitation with microtripsy

    20:29 Tumor destruction and the immune response

    28:33 Histotripsy through the skull

    37:23 The HOPE4LIVER clinical trial

    43:55 Why basic research needs time

    47:17 FFP updates and supporting the show

    49:20 NASA Black Marble: Holiday lights from space

    55:29 Turning night lights into reliable data

    1:01:36 Hurricane Maria and unequal recovery

    1:08:12 COVID-19 and changing nighttime activity

    1:10:16 Mapping access to electricity

    1:15:20 Where Earth is brightening and dimming

    1:32:57 Sidney Nagel and the physics of everyday life

    1:37:07 The science of a falling drop

    1:46:02 Why coffee leaves a ring

    1:51:04 Jamming: When grains become rigid

    1:53:35 A robotic gripper filled with grains

    1:55:39 Why air pressure changes a splash

    1:58:55 Materials that can be trained and retrained

    2:03:26 The payoff from curiosity

    2:05:29 Coming in Part 2

    2:07:06 Outro


    FEATURED RESEARCH

    Histotripsy: The #HOPE4LIVER single-arm pivotal trial (Radiology, 2024)

    https://doi.org/10.1148/radiol.233051


    NASA's Black Marble nighttime lights product suite (Remote Sensing of Environment, 2018)

    https://doi.org/10.1016/j.rse.2018.03.017


    Training and retraining liquid crystal elastomer metamaterials for pluripotent functionality (PNAS, 2025)

    https://doi.org/10.1073/pnas.2504304122


    WATCH ON YOUTUBE

    https://youtu.be/rDInUEtTojg


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    2 ore e 7 min
  • What OpenAI Actually Did to Navier-Stokes (EP 58)
    Sep 24 2026

    What does it mean to solve an equation that describes almost every fluid around us, from the air over a wing to the water swirling down a drain?

    In Episode 58 of From First Principles, Lester Nare and Krishna Choudhary build the Navier-Stokes equations from the ground up before digging into OpenAI’s claimed breakthrough and the debate surrounding it.

    Summary

    • How Newton’s laws become equations for a moving fluid
    • Velocity fields, incompressibility, pressure and the nonlinear convective term
    • Why viscosity smooths a fluid while nonlinear motion can create finer structure
    • What finite-time blowup means, and why simulation is different from proof
    • How forced and unforced equations differ, and why those assumptions matter
    • Earlier work on Euler, Boussinesq and related fluid equations
    • OpenAI’s claimed result, Lean verification and the scope of the theorem
    • The dispute over scientific credit and the human research behind AI-assisted work
    • The METR investigation of the Hugging Face incident
    • Emergence World and long-running multi-agent experiments
    • AI-assisted biological discovery, oversight and recursive self-improvement
    • Separating demonstrated capabilities from claims and future scenarios

    Chapters

    00:00 Can AI solve Navier-Stokes?
    00:34 Episode introduction
    02:20 Navier-Stokes: Mathematics Meets AI
    10:20 Building the Equations of Fluid Motion
    21:34 Velocity fields, divergence and incompressibility
    34:33 Acceleration and the convective term
    52:18 Why Fluid Motion Is Nonlinear
    1:02:08 Pressure, Euler and the Missing Physics
    1:14:50 How Viscosity Changes Everything
    1:33:36 Solving Equations vs. Simulating Fluids
    1:44:59 Can a Smooth Fluid Blow Up?
    2:13:52 The Road to the Claimed Breakthrough
    2:31:13 Inside the Claimed Navier-Stokes Proof
    2:48:26 The Dispute Over Scientific Credit
    3:07:23 From Chatbots to Agents
    3:08:57 The METR report and Hugging Face incident
    3:23:23 AI Risk, Oversight and the Race Ahead
    3:38:51 AI Discovery Beyond Mathematics
    3:52:47 Why “just turn it off” gets complicated
    4:06:47 Closing thoughts and what comes next
    4:08:46 Outro

    Featured Research

    OpenAI’s Navier-Stokes announcement
    Tristan Buckmaster’s statement
    METR investigation
    Emergence World
    AI-assisted enzyme discovery

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    4 ore e 9 min
  • What’s Next in Science? Nobel Prizes, Space Missions & More (EP 57)
    Sep 14 2026

    What science should you be watching this fall? From Nobel Prize season to NASA’s Roman Space Telescope, Mars’ moons and Mercury, Lester Nare and Krishna Choudhary take a relaxed tour of the discoveries and missions on their radar.

    In Episode 57 of From First Principles, we explore why curiosity-driven research matters, what the Golden Goose Awards celebrate, and how questions that once sounded impractical can lead to unexpected breakthroughs. Then we turn to space: Roman’s search for dark energy and exoplanets, JAXA’s Martian Moons eXploration (MMX) mission, and the mysteries ESA and JAXA’s BepiColombo mission will investigate at Mercury.

    Along the way, we tour the updated FFP website, revisit some favorite episodes, and ask which stories you want us to cover in depth next.

    A note before we begin: the main conversation was recorded before Labor Day weekend. The opening announcement addresses your requests for a separate episode on OpenAI, Navier–Stokes and the wider AI conversation. This episode is our fall science rundown; that deep dive is still to come.

    CHAPTERS
    00:00 Update on our upcoming Navier–Stokes and AI coverage
    03:43 Episode intro and football banter
    05:47 FFP intro
    06:01 Nobel Prize season and our coverage plans
    10:45 Golden Goose Awards: why basic research matters
    21:02 FFP website tour and favorite episodes
    42:24 Nancy Grace Roman Space Telescope
    46:20 Microlensing, exoplanets and dark matter
    51:25 MMX: where did Mars’ moons come from?
    54:40 BepiColombo and the mysteries of Mercury
    1:02:17 Your questions, future deep dives and sign-off
    1:05:40 Outro

    SHOW NOTES
    NASA’s Nancy Grace Roman Space Telescope:
    https://science.nasa.gov/mission/roman-space-telescope/

    JAXA’s Martian Moons eXploration (MMX):
    https://www.mmx.jaxa.jp/en/mission/

    ESA / JAXA BepiColombo:
    https://www.esa.int/Science_Exploration/Space_Science/BepiColombo

    Explore the research and episodes we cover:
    https://ffppod.com

    Science R&D Funding Tracker:
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    WATCH ON YOUTUBE
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    Breaking down science news so it makes sense to curious people everywhere.

    Which mission or research story deserves a full FFP deep dive? Tell us in the comments.

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    1 ora e 4 min