logo

An Ozone Layer on Early Mars? Leveraging Techniques from Earth Science to Understand Habitability at the Red Planet

Sector: Aerospace & Defense • Location: United Kingdom

Source: EU Funding & Tenders Portal

Project
Forthcoming

For decades, Mars exploration has focused on evidence for life to answer the fundamental question: Are we alone in the universe? I will investigate the possibility of life on early Mars by leveraging decades of research on Earth’s atmosphere to understand that of the red planet. I will use a well-established photochemical model constrained by observations from complementary missions to explore whe

Project Information FAQ

Project Information

3 Q
The project “An Ozone Layer on Early Mars? Leveraging Techniques from Earth Science to Understand Habitability at the Red Planet” is an infrastructure initiative in the Aerospace & Defense sector, located in United Kingdom. Taiyo aggregates data on it from EU Funding & Tenders Portal.

Want to explore the full details? View the full report

Participants

Sponsoring Agency

Obfuscated Data

Company

Obfuscated Data

Status

Original status

forthcoming

Taiyo status

Obfuscated Data

Taiyo last update

00-00-0000

Available timestamps

00-00-0000

Available timestamp type

Obfuscated Data

Contact

Contact name

Obfuscated Data

Phone

0000000000

Email

ObfuscatedData@email.com

Address

Obfuscated Data, Obfuscated data, obfuscated data, Obfuscated data

Description

Description

For decades, Mars exploration has focused on evidence for life to answer the fundamental question: Are we alone in the universe? I will investigate the possibility of life on early Mars by leveraging decades of research on Earth’s atmosphere to understand that of the red planet. I will use a well-established photochemical model constrained by observations from complementary missions to explore whether ancient Mars ever had a protective ozone layer that could have shielded surface-dwelling life. The ozone layer is critical on Earth, securing surface habitability from DNA-damaging UV radiation and controlling the temperature structure of the middle atmosphere, with important climatic effects. Our understanding of how Earth’s ozone levels have changed has quickly expanded in recent decades. Here, I will apply lessons learned from Earth to the evolution of a second system—Mars—which will provide unique insights into factors that control planetary atmospheres and the search for life in the universe. Specifically, I will investigate the utility of ratios of the three oxygen isotopes, used extensively to understand oxidative chemistry and atmospheric composition changes on Earth, to constrain Mars ozone densities through the following three objectives. I will: 1) predict triple oxygen isotope signatures for the present-day Mars atmosphere and compare to observations, to better understand controls on isotope composition; 2) determine realistic palaeo-atmospheric conditions conducive to an ozone layer; and 3) predict the oxygen isotope composition of select geological materials for potential early Mars conditions and prioritise options for future exploration. We are in the midst of a revolutionary accumulation of spacecraft data and unprecedented Mars exploration, making this work perfectly timed. Preparation for interpretation of measurements from Mars via my proposed modelling is critical to focus future observational efforts from space agencies globally.

Original sub-sector

Obfuscated

Original Currency

USD

Original budget

000000000000000

Procurement method

Obfuscated Data

Budget

000000000000000

Location

Region

Obfuscated

Country

Obfuscated

State

Obfuscated Data

County

Obfuscated

Location

Obfuscated Data, Obfuscated data, obfuscated data, Obfuscated data

Source

Source reliability

High

Data quality score

100%

Source

Obfuscated Data

URL

obfuscated_data,obfuscateddata.com

More Details

Project Type

Obfuscated Data

Article Published Date

Obfuscated Data