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Followers
1.1K
Account age
3 yrs
💰 Suggested sponsorship rate
$40 – $65 / sponsored post
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🧰 Free analysis for Tim Lichtenberg
Known for
4 views
Check out the new review paper "The distribution of volatile elements during rocky planet formation" led by Terry-Ann Suer: https://arxiv.org/abs/2311.18262. Very useful for improved models and observations of (hot) rocky exoplanets and atmospheric formation on rocky planets.
1 views
This is great news for using exoplanets surveys to better understand the chemical and physical conditions that may enable prebiotic chemistry on other worlds, and by that give us further clues on the prevalent conditions to kickstart life as we know it – also on our own planet!
1 views
In a magma ocean phase rocky planets glow strongly – they are still hot and molten from the primordial heat of formation – and Lorenzo quantified how much of an advantage this is when searching for these planets.
📊 Post engagement
5
Avg engagement / post
0.5%
Engagement vs followers
Nov 2022
On Mastodon since
🔥 Top post: Become my colleague at the University of Groningen! 🌏👽🔭🖥️ The K · 26 likes + reposts
📊 Activity & format
Posting cadence
0.19 / week
A lower-frequency account — each post lands with more weight.
Content mix
Mostly text
Recent: 8 text · 4 image · 0 video.
Follower / following
2.8×
Follows 376 back. A more reciprocal / networked account.
Recent posts
View on Mastodon ↗
Next steps: understand to what extent chemical atmospheric and surface conditions can be characterised on such planets with LIFE, to enable a detailed survey of what distinguishes abiotic from potentially biotic worlds. 🧬👾
This is great news for using exoplanets surveys to better understand the chemical and physical conditions that may enable prebiotic chemistry on other worlds, and by that give us further clues on the prevalent conditions to kickstart life …
He found that the intrinsic heat of transient magma ocean epochs make these planets detectable (and characterisable!) to vast distances (up to ~100 pc). LIFE will be able to find them typically within minutes in both G and M dwarf systems …
In a magma ocean phase rocky planets glow strongly – they are still hot and molten from the primordial heat of formation – and Lorenzo quantified how much of an advantage this is when searching for these planets.
Lorenzo – in his very first paper! 🎉🥳 – now tried to understand if LIFE could find the signature of rocky exoplanets in their early 'magma ocean' phase. From studies of the early Earth we think this phase is critically important in setting…
LIFE (https://life-space-mission.com) is an initiative to develop a space-based nulling interferometer for characterising potentially habitable exoplanets and search for biosignatures. However, LIFE will be capable of doing a lot more, and…
Today on arXiv (https://arxiv.org/abs/2410.13457): Large Interferometer For Exoplanets (LIFE). XIV. Finding terrestrial protoplanets in the galactic neighborhood. A new paper in the LIFE mission series led by Lorenzo Cesario from the Kapte…
A few days ago on arXiv by Joe Eatson: Devolatilization of extrasolar planetesimals by 60Fe and 26Al heating (https://arxiv.org/abs/2402.06476). 26Al the most important desiccating short-lived radionuclide for Solar System analogs, but in …
And now published in ApJL: https://iopscience.iop.org/article/10.3847/2041-8213/ad206e/meta
https://arxiv.org/abs/2401.05864
Check out the new review paper "The distribution of volatile elements during rocky planet formation" led by Terry-Ann Suer: https://arxiv.org/abs/2311.18262. Very useful for improved models and observations of (hot) rocky exoplanets and at…
This is great news for using exoplanets surveys to better understand the chemical and physical conditions that may enable prebiotic chemistry on other worlds, and by that give us further clues on the prevalent conditions to kickstart life …
He found that the intrinsic heat of transient magma ocean epochs make these planets detectable (and characterisable!) to vast distances (up to ~100 pc). LIFE will be able to find them typically within minutes in both G and M dwarf systems …
In a magma ocean phase rocky planets glow strongly – they are still hot and molten from the primordial heat of formation – and Lorenzo quantified how much of an advantage this is when searching for these planets.
Lorenzo – in his very first paper! 🎉🥳 – now tried to understand if LIFE could find the signature of rocky exoplanets in their early 'magma ocean' phase. From studies of the early Earth we think this phase is critically important in setting…
LIFE (https://life-space-mission.com) is an initiative to develop a space-based nulling interferometer for characterising potentially habitable exoplanets and search for biosignatures. However, LIFE will be capable of doing a lot more, and…
Today on arXiv (https://arxiv.org/abs/2410.13457): Large Interferometer For Exoplanets (LIFE). XIV. Finding terrestrial protoplanets in the galactic neighborhood. A new paper in the LIFE mission series led by Lorenzo Cesario from the Kapte…
A few days ago on arXiv by Joe Eatson: Devolatilization of extrasolar planetesimals by 60Fe and 26Al heating (https://arxiv.org/abs/2402.06476). 26Al the most important desiccating short-lived radionuclide for Solar System analogs, but in …
And now published in ApJL: https://iopscience.iop.org/article/10.3847/2041-8213/ad206e/meta
https://arxiv.org/abs/2401.05864
Check out the new review paper "The distribution of volatile elements during rocky planet formation" led by Terry-Ann Suer: https://arxiv.org/abs/2311.18262. Very useful for improved models and observations of (hot) rocky exoplanets and at…
🐘 Community & instance
Home server
fediscience.org
Their home server on the fediverse — the instance a creator picks signals the community they belong to.
✅ Link-verified
Verified link
Proved ownership of a website linked on their profile — Mastodon's green-check verification, a real identity signal rather than a paid badge.
On Mastodon since
Nov 2022
Joined in the Twitter-exodus wave of late 2022 — part of the migration that made Mastodon a real destination.
💡 Facts
🗓️Joined Mastodon in 2022 — 3 years ago.
👁️Averages 5 views per post.
📤Posts about 0.2× per week.
🕵️ Fake follower check
Estimated75/100
Good
Credibility score
92%
Real
Real audience
Low
Fake-follower risk
High
Data confidence
- Est. 92% real, active audience · Low fake-follower risk.
- Engagement (~0.5% of followers engage each post) is around typical for Mastodon.
- Verified account.
- Established account (3+ years old).
Heuristic estimate from engagement, follower ratios, account age & growth — a screening signal, not a guarantee.
About
Assistant Professor of Planetary Physics at Kapteyn Astronomical Institute, University of Groningen 🇪🇺 he/him 🌍🧬🌋🔭🖥️ #Exoplanets #Atmospheres #Astronomy #Geophysics #Geochemistry #PlanetaryScience #OriginOfLife #Astrodon
📸 Gallery
🔀 Audience overlap
EstimatedEstimated shared audience with similar creators — useful for avoiding overlap (or doubling down) when planning a campaign.
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