Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

What is Climate?01:16

What is Climate?

17.5K
Climate refers to the prevailing weather conditions in a specific area over an extended period. As the saying goes, “Climate is what you expect. Weather is what you get.” Climate is influenced by geographic factors, such as latitude, terrain, and proximity to bodies of water.
17.5K
Conditions on Early Earth02:06

Conditions on Early Earth

2.5K
2.5K
Conditions on Early Earth02:06

Conditions on Early Earth

67.0K
Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
67.0K
Global Climate Change01:50

Global Climate Change

24.4K
Throughout its ~4.5 billion year history, the Earth has experienced periods of warming and cooling. However, the current drastic increase in global temperatures is well outside of the Earth’s cyclic norms, and evidence for human-caused global climate change is compelling. Paleoclimatology, the study of ancient climate conditions, provides ample evidence for human-caused global climate change by comparing recent conditions with those in the past.
24.4K
Microbes and Climate Change01:27

Microbes and Climate Change

91
Microorganisms are pivotal agents in Earth's biogeochemical cycles, significantly influencing climate dynamics through their metabolic activities. These microbes modulate the levels of key greenhouse gases by both contributing to and helping mitigate climate change.Microbial Contributions to Greenhouse Gas EmissionsRising global temperatures accelerate microbial metabolism, which, in turn, speeds up the decomposition of organic matter. This process releases carbon dioxide (CO₂) through...
91
Radiation: Applications01:17

Radiation: Applications

1.8K
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
1.8K

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

The Martian mid-latitude subsurface ice is the remnant of a past ice sheet.

Communications earth & environment·2026
Same author

Phase II randomised study of magrolimab combined with bevacizumab-FOLFIRI in patients with previously treated advanced inoperable metastatic colorectal cancer.

ESMO gastrointestinal oncology·2026
Same author

Phase II study of magrolimab combination therapies in patients with head and neck squamous-cell carcinoma.

ESMO open·2026
Same author

Efficacy and safety of short-course radiotherapy versus total neoadjuvant therapy in older rectal cancer patients: a randomised pragmatic trial (SHAPERS).

ESMO gastrointestinal oncology·2026
Same author

Avelumab plus sacituzumab govitecan versus avelumab monotherapy as first-line maintenance treatment in patients with advanced urothelial carcinoma: JAVELIN Bladder Medley interim analysis.

Annals of oncology : official journal of the European Society for Medical Oncology·2025
Same author

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM.

Nature·2023

Related Experiment Video

Updated: May 1, 2026

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

3.0K

Possible climates on terrestrial exoplanets.

F Forget1, J Leconte

  • 1Laboratoire de Météorologie Dynamique, IPSL, Paris, France.

Philosophical Transactions. Series A, Mathematical, Physical, and Engineering Sciences
|March 26, 2014
PubMed
Summary

Scientists explore exoplanetary climates by modeling atmospheric composition, stellar flux, and planetary spin. This research helps assess habitable worlds and optimize telescope observations for exoplanets.

Keywords:
atmospheresclimatesextrasolar planets

More Related Videos

Simulating Temperature in a Soil Incubation Experiment
08:39

Simulating Temperature in a Soil Incubation Experiment

Published on: October 28, 2022

5.1K
Using Generative Art to Convey Past and Future Climate Transitions
06:10

Using Generative Art to Convey Past and Future Climate Transitions

Published on: March 31, 2023

1.7K

Related Experiment Videos

Last Updated: May 1, 2026

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

3.0K
Simulating Temperature in a Soil Incubation Experiment
08:39

Simulating Temperature in a Soil Incubation Experiment

Published on: October 28, 2022

5.1K
Using Generative Art to Convey Past and Future Climate Transitions
06:10

Using Generative Art to Convey Past and Future Climate Transitions

Published on: March 31, 2023

1.7K

Area of Science:

  • Planetary Science
  • Climate Modeling
  • Exoplanet Research

Background:

  • Exoplanetary climate prediction is crucial for identifying habitable worlds.
  • Climate depends on atmospheric composition, stellar flux, and planetary spin.

Purpose of the Study:

  • To speculate on exoplanetary climates despite limited direct observations.
  • To optimize future telescopic observations and assess habitability.
  • To develop reliable climate predictors for exoplanets.

Main Methods:

  • Discussing physical constraints on atmospheric properties (planet size, stellar distance, star type).
  • Utilizing global climate models analogous to Earth and solar system telluric atmospheres.
  • Developing realistic climate simulators by combining components like dynamical cores and radiative transfer solvers.

Main Results:

  • Climate models can be developed using components from Earth and solar system simulations.
  • Predicting specific exoplanet climates remains challenging due to strong positive feedbacks.
  • Instabilities like runaway glaciations and greenhouse effects can lead to divergent climate states.

Conclusions:

  • Reliable climate predictors for exoplanets can be built.
  • Climate systems are complex and sensitive to feedback loops.
  • Further research is needed to refine exoplanet climate predictions.