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Q&A 53: How Many Planets Can We Detect? And More... Featuring Professor David Kipping

17.7K views
•
April 19, 2018
by
Fraser Cain
YouTube video player
Q&A 53: How Many Planets Can We Detect? And More... Featuring Professor David Kipping

TL;DR

Answering viewer questions on space exploration, Fermi Paradox, and exoplanets, with a special guest appearance.

Transcript

all right another week time for your questions your questions my answers that's a Steller's Jay wherever you are on my channel done go ahead question pops into your brain just type it in I will gather a bunch of them up and I'll answer them here I got another special guest answer er so please stick around to the end I think you'll really enjoy it a... Read More

Key Insights

  • 🤩 Neutron star collisions may not solve the Fermi Paradox due to the vast age of the universe.
  • ❓ Language differences like Canadian pronunciation variations discussed in a humorous context.
  • 📽️ NASA's active role in supporting innovative projects like the BFR highlights the agency's adaptability.
  • 🥺 The unique dynamics of white dwarfs under extreme rotation settings explained, leading to potential self-destruction.
  • 🎟️ Potential future missions to Europa and Jupiter illustrate the importance of comprehensive exploration strategies.
  • 👾 Continued advancements in space exploration present both exciting discoveries and longer planning timescales.
  • 🥺 Possibility of infinite repeats in an infinite universe could lead to exact Earth copies in distant locations.

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Questions & Answers

Q: Could neutron star collisions explain the Fermi paradox?

Although heavy elements are created in collisions, the universe's age suggests other civilizations could have evolved and explored space billions of years ago.

Q: Why drill through ice on Europa when there are water vents on the surface?

Probes may first sample surface water but directly accessing the ocean could reveal deeper insights, highlighting the importance of both exploration methods.

Q: How would NASA respond to innovative projects like SpaceX's BFR?

NASA collaborates with private companies like SpaceX, enhancing mission viability and reducing costs for further scientific endeavors.

Q: Can white dwarfs spin so fast they tear themselves apart?

Extreme rotation speeds can lead to white dwarf destruction, showcasing the immense forces and speeds present in celestial bodies.

Q: When will Jupiter lose its atmosphere and what will it look like?

Jupiter will remain a gas giant, cooling over time without losing its hydrogen and helium atmosphere, becoming a colder version of itself.

Q: Do you think we live in an exciting yet challenging era for space exploration?

Despite longer timelines for missions, advancements like the BFR and upcoming missions signal continued progress and discoveries in space exploration.

Q: Can you meet an exact Earth copy in an infinite universe by traveling far enough?

In an infinite universe, repeats of configurations will occur, meaning Earth-like planets and inhabitants could exist an infinite number of times.

Q: What factors determine the percentage of exoplanets transiting in front of their star?

The transit probability depends on the star size, planet separation, and angles, with varying rates based on planet properties and star systems.

Summary & Key Takeaways

  • Addressing questions about neutron star collisions, Fermi Paradox, complexity of the universe's age, and potential alien civilizations.

  • Explaining language differences in Canada and the U.S., addressing suggestions on covering NASA's innovative awards.

  • Responding to queries about Europa's water, Jupiter's future, white dwarf dynamics, and NASA's role in space missions.


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