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Cara Menjelajahi Venus Runaway Greenhouse Explorer 3D
Buka Venus Runaway Greenhouse Explorer 3D, geser kontrol CO2 atau tekan Reset, dan lihat mengapa selimut CO2 tebal membuat Venus lebih panas daripada Merkurius, meski Venus mengorbit hampir dua kali lebih jauh dari Matahari.
- Buka https://freetoolonline.com/space-3d/venus-runaway-greenhouse.html dan tunggu Venus selesai dirender.
- Geser kontrol CO2 menjauh dari 96% dan lihat lapisan kabut di sekitar Venus menipis dan berubah warna.
- Tekan "Reset" untuk mengembalikan kontrol ke komposisi terukur nyata Venus (96,5% CO2) dan baca suhu permukaan nyata 464 C / 737 K di panel data.
- Aktifkan pembanding Merkurius untuk melihat bola Merkurius berskala di samping Venus, lalu baca mengapa Merkurius - hampir dua kali lebih dekat ke Matahari - tetap lebih dingin secara rata-rata.
- Aktifkan batang pembanding tekanan untuk melihat tekanan permukaan Venus (92 bar) di samping Bumi (1 bar) dan Merkurius (hampir nol).
- Baca panel data untuk tabel referensi lengkap setiap angka terpublikasi yang digunakan di halaman ini.
Angka publikasi utama
| Figure | Value |
|---|---|
| Venus surface temperature | about 464 C (737 K), day and night |
| Venus surface pressure | about 92 bar |
| Venus atmosphere composition | about 96.5% CO2, about 3.5% N2 |
| Mercury dayside maximum | about 430 C at the equatorial hot poles |
| Mercury night minimum | about -180 C |
| Distance from the Sun | Venus about 0.72 AU, Mercury about 0.39 AU |
Selanjutnya: panduan kapan menggunakannya atau perbandingan dengan alternatif. Buka Venus Runaway Greenhouse Explorer 3D.
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